175 Commits
v0.13 ... v0.18

Author SHA1 Message Date
2fb9679e4d Merge branch 'master' of https://git.psi.ch/nemu/musrfit 2016-12-18 10:44:56 +01:00
dce31426a7 increased the version number form 0.17.0 to 0.18.0 2016-12-18 10:43:53 +01:00
43a8945109 update of the docu. 2016-12-18 10:43:00 +01:00
265fe18f36 adopted to the new features in musrview and some additional little improvements. 2016-12-18 10:41:34 +01:00
5d80c342e0 cleaned up some inconsistencies in the musrfit_startup.xml options 2016-12-18 10:39:43 +01:00
63516fc499 added a first version of a optimized phase correction for the real Fourier transform 2016-12-18 10:37:50 +01:00
c768c27898 for maxLH it is now possible to get the per-run-block maxLH, and the expected maxLH 2016-12-18 10:36:02 +01:00
65d40cfe97 improved user interface. (i) it is searching now not only in the current directory or file-path-name, but also in the default search paths for data files as defined in the musrfit_startup.xml. (ii) it is now also possible to use run numbers rather than full file names. 2016-12-18 10:31:16 +01:00
9c1144fa7b Deal with old pta runs. 2016-12-14 13:57:11 +01:00
b106ac61a1 added phase optimized Re FT for musrview. Still not perfect. 2016-12-07 17:02:18 +01:00
a361c7f7bb added locally the LD_LIBRARY_PATH. This is needed for macOS 10.12 if ROOT is installed in a local user directory. 2016-11-29 21:06:49 +01:00
f7834aaead added class PFTPhaseCorrection which allows to calculate the phase optimzied real part of the Fourier transform. musrFT is already using it, for musrview it is still missing. 2016-11-29 11:16:45 +01:00
1e5bfb8216 when activating the cross hair cursor in the musrview canvas, enable the event status bar as well. This allows the user to see exactly where the cursor is. This is for instance helpful for Fourier spectra. 2016-11-28 11:02:03 +01:00
4c24a1e481 prepare the FOURIER block command 'range_for_phase_correction' for the new FT Re-part automatic phase correction algorithm. 2016-11-28 10:13:38 +01:00
87c8860ef7 musredit_qt5: replaced QProcess::startDetached by QProcess::start for musrT0 and musrFT due to issues with macOS 10.12. I will need to investigate the ownership issue a bit more careful since this fix might lead to a memory leak. 2016-11-15 14:46:11 +01:00
19d5c09b45 musredit_qt5: adopted call of musrview such that it works under macOS 10.12 2016-11-15 08:58:13 +01:00
ea841ec186 got rid of direct 'system()' calls wherever possible. 2016-11-08 08:53:43 +01:00
d74588827e change the focus from 'cancel' to 'ok' 2016-10-28 15:57:57 +02:00
e32d0e912c update of the documentation 2016-08-25 07:54:25 +02:00
6585032df0 in musrview it is now possible to enable/disable a crosshair cursor by pressing 'c'. 2016-08-24 15:37:14 +02:00
ba11658e5b set permission of musredit_startup.xml under Mac OSX properly. 2016-08-22 11:10:38 +02:00
aae5762f7c yet another improvement for the new git-based NeXus versions >= 4.4 2016-08-17 08:27:13 +02:00
68a788c3c7 some fine tuning needed to make sure that the NeXus library is indeed found. 2016-08-16 07:44:54 +02:00
08848e68a8 drop NeXus support for Version < 4.4 2016-08-10 10:28:31 +02:00
5c69c21f56 should prevent crash if musrfit_startup.xml is NOT found anywhere. 2016-08-09 12:43:13 +02:00
4cdc4dbf1d musredit: run lists are now properly loaded if containing nS-nE elements. 2016-08-02 13:15:55 +02:00
852043f286 added a full user function example to doc/examples which should help a user to understand how to deal with the subclass plugin mechanism. 2016-06-22 09:39:13 +02:00
2f91278871 fixed a minor bug in the background handling. For now change over to un-weighted N0 estimate which seems to be slightly better. This only could mean, that the error estimate if M is NOT optimal. Eventually this needs some deeper investigation. 2016-05-06 18:54:36 +02:00
35198e46da marginal improved error estimate for single histo RRF 2016-05-06 16:58:43 +02:00
8d18ca7905 force to ignore freq < 10 MHz for single histo RRF to find max freq. This is needed for heavily damped high frequency signals. 2016-05-04 17:11:32 +02:00
6c9adda7d2 made start-/endTimeBin class variables. 2016-05-03 11:19:16 +02:00
8c2b38cd5e removed some leftover debug information 2016-04-28 13:06:33 +02:00
bb1f6b113b updated licence info and added paramList to the GUI. 2016-04-28 13:05:39 +02:00
c94acc8e26 update of the docu 2016-04-28 11:12:49 +02:00
cb14afbe07 msr2data gets a new option paramList which allows to select the number of parameters to be exported. 2016-04-28 11:11:06 +02:00
b0bb5f94a5 changed const to variable due compiler issues. 2016-04-27 11:03:21 +02:00
af7b729a5a start-/endTimeBin are now class members. This reduces the number of recalculations. 2016-04-26 12:39:27 +02:00
03667f9dfb added missing png's 2016-04-26 08:52:02 +02:00
0972843d30 updated of docu 2016-04-26 08:43:48 +02:00
9cf8a7287d added mu minus example with simulated data. 2016-04-26 07:56:32 +02:00
2c5765dd5d Merge branch 'master' of https://git.psi.ch/nemu/musrfit 2016-04-22 10:58:02 +02:00
ee064fc504 Added the theory function muMinusExpTF for mu minus fits 2016-04-22 10:56:52 +02:00
3dfd348d5e all mu minus fits to run log max likelihood minimization. 2016-04-22 10:54:09 +02:00
b65e07b8c8 added fractions for 34 and 14 lines for anisotropic Mu 2016-04-15 19:06:10 +02:00
908f728744 Changed calculation of charge-exchange processes to a product of complex polarization functions, as in the paper of M. Senba 2016-04-14 15:28:33 +02:00
2339ee9b80 musredit: improved path-file handling needed for musrview 2016-04-11 12:14:40 +02:00
82ba938c2d make sure that N0 is only estimated if N0 is NOT fixed. 2016-04-11 11:11:31 +02:00
666f2c49c3 added docu for the GbG LF user function 2016-03-29 15:35:45 +02:00
d5f7d9eb9d added necessary FFTW3 cflags 2016-03-16 07:26:26 +01:00
9f38d49773 removed the gsl part all together since it is not thread safe. 2016-03-16 07:10:59 +01:00
e0e4a1e17e added user function for GbG LF 2016-03-14 11:30:06 +01:00
ec5a26d96d Merge branch 'master' of ssh://gitorious.psi.ch/nemu/musrfit 2016-03-04 09:43:36 +01:00
47580b66d8 added a GbG LF calculator (standalone for now) 2016-03-04 09:43:05 +01:00
cd04164943 Fixed problems with run header 2016-03-03 17:28:50 +01:00
3ff1bebd9d centralize XML startup files 2016-02-26 08:30:50 +01:00
4d2d7c860e more work towards centralizing default startup XML files. 2016-02-25 21:07:30 +01:00
a5e9191f15 centralize more XML startup files. 2016-02-25 18:19:29 +01:00
a0f7d5e934 Merge branch 'master' of ssh://gitorious.psi.ch/nemu/musrfit 2016-02-23 13:24:19 +01:00
fe48da74a1 It is now possible to export the averaged data/Fourier 2016-02-23 13:22:41 +01:00
7ae1b9ab5e changed to complex Mu polarization function 2016-02-22 22:47:58 +01:00
1c5c94a86b Use Musr-Root run header 2016-02-17 20:42:13 +01:00
96ad763940 Removed faulty lines at the beginning and end of file 2016-02-17 14:27:11 +01:00
1c31fc88d0 Added Mu0 spin-flip process 2016-02-17 14:22:21 +01:00
352ac5db21 install default XML startup files under /home/nemu/.musrfit rather than /bin. Since this is a substantial indentation, the version number has been incremented. 2016-02-17 12:59:03 +01:00
bd05f57523 start moving startup XML-files to /home/nemu/.musrfit 2016-02-17 10:47:18 +01:00
4fec25e423 corrected wrong path to musredit icon under MacOSX 2016-02-17 07:38:22 +01:00
28dc4a5a41 added more svg icons and remove the old xpm icons 2016-02-17 07:38:16 +01:00
d553dcbb6a added missing icon files 2016-02-16 17:51:32 +01:00
f6cbb4d806 replace data-file-format tag from ROOT-NPP/PPC to MUSR-ROOT whenever possible. 2016-02-16 13:29:45 +01:00
1d98148d9d musredit_qt5 partially new icons (see ChangeLog) 2016-02-16 08:52:40 +01:00
1cf7fe9ec3 Merge branch 'master' of gitorious:nemu/musrfit 2016-02-03 08:56:05 +01:00
460d35defa Add HAL and move to MUSR-ROOT in MuSRFitGUI. Update msr template for libBNMR. 2016-02-03 08:55:20 +01:00
5ba2747929 added missing png's to the docu 2016-01-25 07:42:42 +01:00
d0da0dd063 update of the docu which now describes the RRF option. 2016-01-22 16:16:29 +01:00
a35884b86c merge the devel-rrf branch into the master branch 2016-01-22 15:39:32 +01:00
55f70cd526 Merge branch 'devel-rrf' 2016-01-22 15:25:53 +01:00
6c4c8eb74c currently working with 3 lines 2016-01-22 15:23:32 +01:00
7862c93c68 added first RRF memo version 2016-01-22 15:14:10 +01:00
eb482b9671 improved handling of RRF freq in the msr-file 2016-01-18 16:25:34 +01:00
c50a33243d fixed a compiler warning 2016-01-18 16:24:52 +01:00
02c82321de added RRF types to musrt0 2016-01-18 16:00:10 +01:00
71cac92d23 more work toward an asymmetry RRF fit. 2016-01-18 10:41:27 +01:00
b8b7b7665f some more work towards asymmetry RRF 2016-01-15 18:26:47 +01:00
5303f550b4 add the missed files. 2016-01-15 17:30:05 +01:00
8e399fa04e first steps towards asymmetry RRF fit. 2016-01-15 17:16:07 +01:00
6f79943ca2 Changed runMuSimulation.C according to chnages in PSimulateMuTransition.cpp 2016-01-14 13:56:27 +01:00
782eb4e1a4 better RRF labelling, and proper class variable naming. 2016-01-14 13:18:06 +01:00
8b2f0a16af Calculate for Mu Px(t) by a superposition of the 4 Mu frequencies 2016-01-14 11:55:43 +01:00
fd655e720b slightly improvement the N0 estimate 2016-01-14 11:24:49 +01:00
52e2c20527 some tweaking in order to supress ghost lines. 2016-01-07 16:10:47 +01:00
097a6db6b0 more work towards fully functional RRF single histo fit 2016-01-07 13:19:00 +01:00
7d315b2b86 implemented proper error propagation and improved N0 estimate. 2016-01-06 17:33:41 +01:00
6ee5d76b35 first implementation of the single histo RRF fit (no plotting yet). Seems to work but the error estimate of the RRF asymmetry seems to be too large. Needs to be checked. 2015-12-21 16:54:12 +01:00
99864b2b82 some more self-consistency checks with RRF. 2015-12-19 20:32:07 +01:00
c3b5a52519 start working on RRF. For now only work on the msr-file side is done. 2015-12-18 15:34:18 +01:00
18c90fef99 adopted to qt5 Mac OS X 2015-11-23 07:56:52 +01:00
4824937fa1 make it a bit more flexible 2015-11-20 08:47:36 +01:00
b7716938ae changed default font for musredit_qt5 from New Courier to Monospace 2015-11-19 13:29:19 +01:00
14e4b28946 removed unnecessary check form musredit_qt5 msr2data interface. 2015-11-15 11:41:56 +01:00
9c700a3773 Fixes the crash of Fourier if the maximal range given in the Fourier block is larger than the available. 2015-11-11 10:30:16 +01:00
c6f5c1205e fixed a bug with double vectors in TMusrRunHeader 2015-10-29 16:03:36 +01:00
f44a9e94cf updated ChangeLog 2015-10-28 14:06:32 +01:00
6433585d3b incorporate musredit_qt5 into the automake framework 2015-10-27 14:24:44 +01:00
d44c9a4fdc added a first port of musredit form Qt 4.x to Qt 5.x 2015-10-26 20:00:40 +01:00
f58cbf1874 added a yet experimental feature of a phase 'optimized' real Fourier transform. 2015-09-24 15:33:47 +02:00
1f95678764 generating global fit msr-files including a GLOBAL block is working now as expected. 2015-09-22 16:33:02 +02:00
fc9c573f2a some minor improvements proposed by BMW: fix data to graph 2015-09-20 19:06:38 +02:00
e55ac4ecee after cross-check with BMW cleaned up, removed one copy/paste error (break;) and re-enabled the other twos which are indeed needed. 2015-09-18 16:21:15 +02:00
cb73f8bfa0 in PMsr2Data::PrepareGlobalInputFile() there seem to be 'unmotivated' break; commands in some loops. They prevent a proper map handling. For now they are commented out, which results in a proper functioning. 2015-09-17 14:51:51 +02:00
6c0a266e6a any2many export of MusrRoot crashed when first histo group was != 0. This happend when exporting to PSI-BIN or WKM. This is fixed now. 2015-09-14 09:44:49 +02:00
24bc2cbb0b hopefully final fix for the FOURIER range output. 2015-09-08 15:50:06 +02:00
5a00d49bbd fixed error in view_packing for single histo (wrong norm of the theory). 2015-09-08 13:08:41 +02:00
8d496a41c0 added little root macro to check the c++ io formatting. 2015-09-08 08:50:26 +02:00
4d211ddcc1 updated to the previous incomplete fix. FOURIER range is not truncated anymore. 2015-09-04 17:36:57 +02:00
001aed134c minor change in Fourier-block output (PMsrHandler::WriteMsrLogFileand PMsrHandler::WriteMsrLogFile) to avoid truncated range labels. 2015-09-04 16:23:27 +02:00
2f671e1673 updated ChangeLog which was orphaned since V0.13.0 2015-08-17 09:55:47 +02:00
05430b8745 updated the docu 2015-08-16 11:45:58 +02:00
b113a94ee9 added the class PStringNumberList which allow to parse a generic encoded list of numbers. Used this class to improve PMsrHandler, and improved the runList feature of msr2data. For details see the documentation of msr2data. 2015-08-16 11:43:57 +02:00
bccc97ff22 changed setf/unsetf bug 2015-06-30 12:17:25 +02:00
012b2e5891 adopted the temperature dependence of the gap function (see Eq.(8) of the memo), which breaks the self-consistency. Makes it more flexible but requires that the user is using his brain. 2015-06-25 08:42:32 +02:00
da93db557f small correction of the skewed Gaussian for extrem parameter values. 2015-06-25 08:36:26 +02:00
93207782a9 updated docu and removed an unsed variable 2015-05-29 20:10:15 +02:00
fab7acfedc added a group histo selector in any2many for MusrRoot when exporting to a too limited file format as PSI-BIN. 2015-05-29 15:11:04 +02:00
e78619c33b another path check for HDF5 with ubuntu 15.04 2015-05-15 14:29:14 +02:00
e4f11aca8c update of the technical docu 2015-04-01 08:40:33 +02:00
ee617d4af5 some minor correction for ASCII export in any2many 2015-03-16 10:43:52 +01:00
6ce19bcf26 check that FOURIER block phase parameter as parX is not leading to an error message. 2015-02-28 11:30:09 +01:00
8cc07318eb some more bug fixing for average per data set. 2015-02-26 13:15:29 +01:00
59525a787e added missing background range from msr-file 2015-02-24 10:32:59 +01:00
78d98f7652 separated PSI-BIN and PSI-MDU file format 2015-02-24 10:02:04 +01:00
c938589286 implemented an average-per-data-set option for musrFT. 2015-02-23 16:30:14 +01:00
80b3952649 make sure that musrFT is found 2015-02-21 20:59:52 +01:00
e95a380bea add proper Mac icon to musredit 2015-02-21 20:38:33 +01:00
38be81d704 needed to adopted includes for dictionary generation due to adding fftw.h in PMusr.h 2015-02-21 15:33:07 +01:00
39f739e2c8 added vanilla README for automake 2015-02-21 14:43:50 +01:00
8c211167be changed name 2015-02-21 10:34:04 +01:00
d29688952d for graphical export in the batch mode, menus mustn't be set. 2015-02-20 12:57:40 +01:00
b7f882b39e Merge branch 'master' of https://bitbucket.org/muonspin/musrfit 2015-02-20 12:41:22 +01:00
2106c903df Merged in zaher-salman/musrfit (pull request #4)
Compilation errors distclean issues
2015-02-20 12:39:37 +01:00
a310c36a70 Merge branch 'master' of https://bitbucket.org/zaher-salman/musrfit 2015-02-20 12:32:49 +01:00
7be8b4c2ea add a switch to musrview that it plots initially the Fouier data rather than the time domain data. 2015-02-20 12:22:24 +01:00
6315076157 Merged muonspin/musrfit into master 2015-02-20 09:53:18 +01:00
c971aac129 added a first preliminary user interface for musrFT within musredit. 2015-02-19 17:24:00 +01:00
7351e10133 Fixed compilation problem with fftw3 and added fake automake files to musredit and musrgui. 2015-02-19 17:20:01 +01:00
68b071ec2e Fixed compilation problem with fftw3 and added fake automake files to musredit and musrgui. 2015-02-19 17:08:16 +01:00
ee02450af4 Merged muonspin/musrfit into master 2015-02-17 17:08:05 +01:00
741a9e7e48 fixed typos in the usage output. 2015-02-17 13:14:07 +01:00
ca48941deb bug fixing towards a musrFT feature complete state. 2015-02-17 12:46:30 +01:00
34da894f15 Merged muonspin/musrfit into master 2015-02-17 09:33:03 +01:00
0e6ceecf24 changed the data export handling from musrview. It is now more main line and follows the implementation of musrFT. At the same time removed an autodated comment in PFourierCanvas.h. 2015-02-16 17:23:39 +01:00
934764e810 Sync muonspin/musrfit into master 2015-02-16 15:58:05 +01:00
ce490b014a added missing header file 2015-02-16 15:50:50 +01:00
4da5c3a2da Merged muonspin/musrfit into master 2015-02-16 13:53:13 +01:00
34fe2e6220 Merged in zaher-salman/musrfit (pull request #3)
Integrate libBNMR in automake
2015-02-16 13:51:42 +01:00
b004354fe6 Merged muonspin/musrfit into master 2015-02-16 12:05:17 +01:00
f03ccacea4 Merge branch 'master' of https://bitbucket.org/zaher-salman/musrfit 2015-02-16 12:05:41 +01:00
5366295349 Updated ChangeLog for integration of libBNMR in automake 2015-02-16 12:04:55 +01:00
e097cc3119 added data export from the GUI menu. 2015-02-16 07:30:57 +01:00
f9197cb815 removed outdated help information. 2015-02-13 17:04:50 +01:00
2d2594c903 first almost feature complete version of musrFT 2015-02-13 16:56:19 +01:00
d4ba2f6d81 more work towards a standalone Fourier (mainly for HAL-9500). Add msr-file support. Still some severe flaws. 2015-02-11 15:35:14 +01:00
16c2723d6c Merged muonspin/musrfit into master 2015-02-04 10:09:30 +01:00
9793478b3c Minor cleaning up in libBNMR. 2015-02-04 09:49:39 +01:00
1f44fe33c1 libBNMR is now fully integrated into automake 2015-02-04 09:34:05 +01:00
f56c2b5fda Merge branch 'master' of ssh://gitorious.psi.ch/nemu/musrfit 2015-02-02 15:54:01 +01:00
c6900030c7 first partial implementation for a standalone Fourier transform calculator/plotter. Mainly meant for HAL-9500. Much more to come ... 2015-02-02 15:52:51 +01:00
b7bd3c286e Include libBNMR in standard configuration and automake (still not fully working). 2015-01-29 13:46:26 +01:00
7414011db6 Merged in zaher-salman/musrfit (pull request #2)
Save data to ascii in batch mode and bNMR template msr files
2015-01-27 20:29:00 +01:00
acb5a1af09 Remove redundant and optimize code for saving data to ascii in batch mode. 2015-01-27 11:17:06 +01:00
55fb9df820 Turn on batch mode for --ascii option. 2015-01-26 16:56:36 +01:00
cb2005dccd README edited online with Bitbucket 2015-01-26 07:56:15 +00:00
addb1d6830 Added .msr file for bNMR mud file fit. 2015-01-23 22:22:47 +01:00
8035bafec4 Added option to save data from canvas a quit for non-interactive mode (web). 2015-01-23 17:17:08 +01:00
be9bfdf091 Added option to save data from canvas a quit for non-interactive mode (web). 2015-01-23 15:58:53 +01:00
9fd8088764 slightly adopted the technical docu 2015-01-08 13:34:12 +01:00
413 changed files with 46906 additions and 7951 deletions

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ChangeLog
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# ChangeLog
#---------------------------------------------------------------------
changes since 0.18.0
===================================
changes since 0.17.0
===================================
NEW 2016-12-18 for maxLH it is now possible to get the per-run-block maxLH,
and the expected maxLH.
NEW 2016-12-18 musrview allows no to show directly the Fourier transform,
and the averaged data/Fourier transform.
NEW 2016-12-18 added a first full version of an automatic phase correction
for the real part of the Fourier transform. It is based on
the algorithm published in JMR 158, 164 (2002).
NEW 2016-12-18 a couple of improvements in dump_header: (i) it is not
only searching in the current directory, but also in all
default paths defined in musrfit_startup.xml. (ii) it is
now possible also to give only run numbers instead of the
full file name.
NEW 2016-08-24 in musrview it is now possible to enable/disable a
crosshair cursor by pressing 'c'.
NEW 2016-04-28 updated licence info in musredit and added paramList
feature to the msr2data GUI.
NEW 2016-04-28 msr2data gets a new option: paramList which allows to
extract a subset of all the parameters of a collection
of msr-files.
NEW 2016-04-22 Added the theory function muMinusExpTF for mu minus fits
NEW 2016-02-23 It is now possible to export the averaged data/Fourier
CHANGED 2016-12-18 updated the docu.
CHANGED 2016-12-18 a couple of little improvements in musredit.
CHANGED 2016-08-10 drop NeXus support for Version < 4.4
CHANGED 2016-04-26 start-/endTimeBin are now class members. This reduces
the number of recalculations.
FIXED 2016-08-02 run lists are now properly loaded if containing nS-nE elements.
changes since 0.16.0
===================================
NEW 2016-01-22 update of the docu which now describes the RRF option.
CHANGED 2016-02-17 move the startup XML-files to $HOME/.musrfit
rather than having it within $prefix/bin. Increase
therefore the version number to 0.17.0
CHANGED 2016-02-16 if the LEM file is created 2012 or later and the
data-file-format tag is still ROOT-NPP or ROOT-PPC, it
will automatically switched to MUSR-ROOT. This way red/green
issues should be prevented. (see MUSR-314).
CHANGED 2016-02-16 start migrating the icons of musredit_qt5 to the breeze
icons (https://github.com/NitruxSA/breeze-icon-theme).
At the same time I start to redesign the musrfit specific
icons accordingly (not yet happy with it, but ...).
changes since 0.15.0
===================================
NEW 2016-01-22 add RRF fit option. At the same time, the version has been
increased to 0.16.0. For details see the documentation.
FIXED 2015-10-29 TMusrRunHeader didn't map a double vector properly into a
string. The last element was a copy of the 2nd last instead
if the proper last. This is now fixed. Fixed also some
comment typo.
FIXED 2015-11-11 Fixes the crash of Fourier if the maximal range given in the
Fourier block is larger than the available.
CHANGED 2015-11-15 removed unnecessary check form musredit_qt5 msr2data interface.
changes since 0.14.0
===================================
NEW 2015-10-26 added a first ported musredit version (Qt4 -> Qt5). At the same
the version has been incremented to 0.15.0.
NEW 2015-09-24 adding a phase optimized real Fourier to musrFT. This is still VERY
experimental, and hence only available from within musrFT. Eventually
it should make its way into musrview as well. Furthermore the
documentation needs to be written yet. There is only a short not in
the command line present.
NEW 2015-02-23 implemented an average-per-data-set option for musrFT.
NEW 2015-02-21 add proper Mac icon to musredit
FIXED 2015-09-22 generating global fit msr-files including a GLOBAL block is working
now as expected.
FIXED 2015-09-17 in PMsr2Data::PrepareGlobalInputFile() there seem to be 'unmotivated'
break; commands in some loops. They prevent a proper map handling.
Since this is a real puzzle I contacted BMW for clarification.
2015-09-18: there is only one unmotivated break; cleaned up the code
accordingly.
FIXED 2015-09-14 any2many export of MusrRoot crashed when first histo group was != 0.
This happend when exporting to PSI-BIN or WKM. This is fixed now.
FIXED 2015-09-08 fixed error in view_packing for single histo (wrong norm of the theory).
FIXED 2015-09-04 minor change in Fourier-block output (PMsrHandler::WriteMsrLogFile
and PMsrHandler::WriteMsrLogFile) to avoid truncated range labels.
FIXED 2015-06-30 changed setf/unsetf bug (PMsr2Data.cpp)
FIXED 2015-05-15 another path check for HDF5 with ubuntu 15.04
FIXED 2015-03-16 some minor correction for ASCII export in any2many
FIXED 2015-02-26 some more bug fixing for average per data set.
FIXED 2015-02-20 for graphical export in the batch mode, menus mustn't be set.
CHANGED 2015-08-17 updated ChangeLog which was orphaned since V0.13.0
CHANGED 2015-08-16 updated the docu
CHANGED 2015-08-16 added the class PStringNumberList which allow to parse a
generic encoded list of numbers. Used this class to improve
PMsrHandler, and improved the runList feature of msr2data.
For details see the documentation of msr2data.
CHANGED 2015-06-25 adopted the temperature dependence of the gap function
(see Eq.(8) of the memo), which breaks the self-consistency.
Makes it more flexible but requires that the user is using
his brain.
CHANGED 2015-06-25 small correction of the skewed Gaussian for extrem parameter
values.
CHANGED 2015-05-29 updated docu and removed an unsed variable
CHANGED 2015-05-29 added a group histo selector in any2many for MusrRoot when
exporting to a too limited file format as PSI-BIN.
CHANGED 2015-04-01 update of the technical docu
CHANGED 2015-02-28 check that FOURIER block phase parameter as parX is not leading
to an error message.
CHANGED 2015-02-24 added missing background range from msr-file (musrFT)
CHANGED 2015-02-24 separated PSI-BIN and PSI-MDU file format
CHANGED 2015-02-21 make sure that musrFT is found
CHANGED 2015-02-21 needed to adopted includes for dictionary generation due to
adding fftw.h in PMusr.h
CHANGED 2015-02-21 have now README and README.md for automake and bitbucket,
respectively.
changes since 0.13.0
===================================
NEW 2015-02-23 implemented an average-per-data-set option for musrFT.
NEW 2015-02-20 add a switch to musrview that it plots initially the Fouier data rather
than the time domain data.
NEW 2015-02-19 added a first preliminary user interface for musrFT within musredit.
NEW 2015-02-16 changed the data export handling from musrview. It is now more
main line and follows the implementation of musrFT.
NEW 2015-02-13 first implementation of a standalone Fourier transform/plotter:
musrFT. Initially it is meant to be used for HAL-9500,
i.e. Fourier transform WITHOUT lifetime correction.
A first simple minded lifetime correction is implemented as well.
NEW 2015-02-04 Integration of libBNMR for fitting beta-NMR relaxation data
into automake of musrfit.
NEW 2014-12-18 first implementation of a GLOBAL block which allows to shorten
a typical msr-file. Duplicate entries from the RUN blocks can be
added here. Furthermore, the 'lifetimecorrection' flag is

68
README
View File

@ -1,33 +1,35 @@
# musrfit - muSR data analysis package #
### Contents ###
This is a data analysis package to analyze time differential muSR data.
Currently it allows the following things:
* setting up most commonly used fitting functions for muSR
* fitting data, including global fits
* showing the fit results and the residuals
* showing the Fourier transform of the data
* extracting easily the fitting parameters to be used in other programs (gnuplot, qtiplot/origin, ...)
* allows to generate fitting input files for follow-up runs
* allows to generate global fitting input files based on a single run template
* allows to implement more sophisticated user functions
(e.g. GL vortex lattice, Meissner screening including low-energy muon stopping profiles)
### Currently supported platforms: ###
* Linux
* Mac OS X
* Windows - not really, only for the very brave ones
### Documentation ####
For a more exhaustive user documentation see:
http://lmu.web.psi.ch/musrfit/user/MUSR/WebHome.html
### Contact ###
<andreas.suter@psi.ch>
README
musrfit - muSR data analysis package
Contents
--------
This is a data analysis package to analyze time differential muSR and beta-NMR data.
Currently it allows the following things:
* setting up most commonly used fitting functions for muSR and beta-NMR
* fitting data, including global fits
* showing the fit results and the residuals
* showing the Fourier transform of the data
* extracting easily the fitting parameters to be used in other programs (gnuplot, qtiplot/origin, ...)
* allows to generate fitting input files for follow-up runs
* allows to generate global fitting input files based on a single run template
* allows to implement more sophisticated user functions
(e.g. GL vortex lattice, Meissner screening including low-energy muon stopping profiles)
Currently supported platforms:
* Linux
* Mac OS X
* Windows - not really, only for the very brave ones
Documentation
For a more exhaustive user documentation see:
http://lmu.web.psi.ch/musrfit/user/MUSR/WebHome.html
Contact
<andreas.suter@psi.ch>

33
README.md Normal file
View File

@ -0,0 +1,33 @@
# musrfit - muSR data analysis package #
### Contents ###
This is a data analysis package to analyze time differential muSR and beta-NMR data.
Currently it allows the following things:
* setting up most commonly used fitting functions for muSR and beta-NMR
* fitting data, including global fits
* showing the fit results and the residuals
* showing the Fourier transform of the data
* extracting easily the fitting parameters to be used in other programs (gnuplot, qtiplot/origin, ...)
* allows to generate fitting input files for follow-up runs
* allows to generate global fitting input files based on a single run template
* allows to implement more sophisticated user functions
(e.g. GL vortex lattice, Meissner screening including low-energy muon stopping profiles)
### Currently supported platforms: ###
* Linux
* Mac OS X
* Windows - not really, only for the very brave ones
### Documentation ####
For a more exhaustive user documentation see:
http://lmu.web.psi.ch/musrfit/user/MUSR/WebHome.html
### Contact ###
<andreas.suter@psi.ch>

View File

@ -1,7 +1,7 @@
AC_REVISION([m4_esyscmd_s([git describe --always])])
AC_PREREQ(2.63)
AC_INIT([musrfit],[0.13.0],[andreas.suter@psi.ch])
AC_INIT([musrfit],[0.18.0],[andreas.suter@psi.ch])
AC_CONFIG_AUX_DIR(admin)
AC_CANONICAL_HOST
#AC_MSG_RESULT([${host} ${host_cpu} ${host_vendor} ${host_os}])
@ -35,7 +35,7 @@ dnl -----------------------------------------------
#release versioning
MUSR_MAJOR_VERSION=0
MUSR_MINOR_VERSION=13
MUSR_MINOR_VERSION=18
MUSR_MICRO_VERSION=0
#release versioning
@ -525,6 +525,9 @@ AC_ARG_ENABLE([NeXus], [AS_HELP_STRING([--enable-NeXus],[build optional NeXus su
elif test -r /usr/local/hdf5/include/hdf5.h; then
HDF5_PREFIX="/usr/local/hdf5"
AC_MSG_RESULT([${HDF5_PREFIX}])
elif test -r /usr/include/hdf5/serial/hdf5.h; then
HDF5_PREFIX="/usr/include/hdf5/serial"
AC_MSG_RESULT([${HDF5_PREFIX}])
elif test -r /usr/include/hdf5.h; then
HDF5_PREFIX="/usr"
AC_MSG_RESULT([${HDF5_PREFIX}])
@ -551,34 +554,31 @@ AC_ARG_ENABLE([NeXus], [AS_HELP_STRING([--enable-NeXus],[build optional NeXus su
[AS_HELP_STRING([--with-nexus],[prefix of the NeXus installation, e.g. /usr/local])],
[NEXUS_PREFIX=$with_nexus
AC_MSG_CHECKING([whether NeXus can be found at the specified location])
if !(test -r ${NEXUS_PREFIX}/include/napi.h); then
if !(test -r ${NEXUS_PREFIX}/include/nexus/napi.h); then
AC_MSG_RESULT([no])
AC_MSG_ERROR([NeXus cannot be found at the specified path!])
fi
AC_MSG_RESULT([${NEXUS_PREFIX}])],
[PKG_CHECK_MODULES(NEXUS, nexus >= 4.1, [NEXUS_FOUND=1],
[PKG_CHECK_MODULES(NEXUS, nexus >= 4.4, [NEXUS_FOUND=1],
[AC_MSG_CHECKING([whether NeXus is installed in a standard location])
if test -r /usr/local/include/napi.h; then
NEXUS_PREFIX="/usr/local"
AC_MSG_RESULT([${NEXUS_PREFIX}])
elif test -r /usr/local/nexus/include/napi.h; then
NEXUS_PREFIX="/usr/local/nexus"
if test -r /usr/local/include/nexus/napi.h; then
NEXUS_PREFIX="/usr/local"
AC_MSG_RESULT([${NEXUS_PREFIX}])
elif test -r /usr/include/napi.h; then
NEXUS_PREFIX="/usr"
AC_MSG_RESULT([${NEXUS_PREFIX}])
elif test -r /sw/include/napi.h; then
elif test -r /sw/include/nexus/napi.h; then
NEXUS_PREFIX="/sw"
AC_MSG_RESULT([${NEXUS_PREFIX}])
elif test -r /opt/local/include/napi.h; then
elif test -r /opt/local/include/nexus/napi.h; then
NEXUS_PREFIX="/opt/local"
AC_MSG_RESULT([${NEXUS_PREFIX}])
else
elif test -r /opt/nexus/include/nexus/napi.h; then
NEXUS_PREFIX="/opt/nexus"
AC_MSG_RESULT([${NEXUS_PREFIX}])
else
AC_MSG_RESULT([no])
AC_MSG_ERROR(
[NeXus not found. Please call configure with the --with-nexus option.
[NeXus Version >= 4.4 not found. Please call configure with the --with-nexus option.
This tells configure where to find the NeXus headers,
e.g. --with-nexus=/usr/local/nexus]
e.g. --with-nexus=/opt/nexus]
)
fi
]
@ -586,8 +586,27 @@ AC_ARG_ENABLE([NeXus], [AS_HELP_STRING([--enable-NeXus],[build optional NeXus su
)
AC_SUBST(NEXUS_PREFIX)
if test "${NEXUS_FOUND}" != "1"; then
NEXUS_LIBS="-L${NEXUS_PREFIX}/lib -lNeXus"
NEXUS_CFLAGS="-I${NEXUS_PREFIX}/include"
dnl get suffix for the NeXus library depending on the OS
AC_REQUIRE([AC_CANONICAL_HOST])
AS_CASE([$host_os],
[linux*], [NEXUS_SUFFIX="so"],
[darwin*], [NEXUS_SUFFIX="dylib"],
[*cygwin*], [NEXUS_SUFFIX="dll"],
[AC_MSG_ERROR([NeXus check: Your platform is not currently supported])]
)
AC_MSG_NOTICE([NeXus Suffix Result: "${NEXUS_SUFFIX}"])
if test -r ${NEXUS_PREFIX}/lib/libNeXus.${NEXUS_SUFFIX}; then
NEXUS_LIB_DIR="lib"
elif test -r ${NEXUS_PREFIX}/lib64/libNeXus.${NEXUS_SUFFIX}; then
NEXUS_LIB_DIR="lib64"
else
AC_MSG_ERROR(
[Couldn't find the NeXus library.]
)
fi
NEXUS_LIBS="-L${NEXUS_PREFIX}/${NEXUS_LIB_DIR} -lNeXus"
NEXUS_CFLAGS="-I${NEXUS_PREFIX}/include/nexus"
fi
AC_SUBST(NEXUS_LIBS)
AC_SUBST(NEXUS_CFLAGS)
@ -733,6 +752,12 @@ dnl -----------------------------------------------
AC_ARG_ENABLE([ASlibs], [AS_HELP_STRING([--enable-ASlibs],[build optional AS plug-ins [default=no]])],[BUILD_AS_LIBS=1], [BUILD_AS_LIBS=0])
dnl -----------------------------------------------
dnl Ask user if BNMRlibs should be built
dnl -----------------------------------------------
AC_ARG_ENABLE([BNMRlibs], [AS_HELP_STRING([--enable-BNMRlibs],[build optional BNMR plug-ins [default=no]])],[BUILD_BNMR_LIBS=1], [BUILD_BNMR_LIBS=0])
dnl -----------------------------------------------
dnl Set some paths and flags for PMusr, MusrRoot, TLemRunHeader, Class_MuSR_PSI, mud, NeXus (if enabled), etc.
dnl -----------------------------------------------
@ -780,6 +805,14 @@ if test "${PNEXUS_ENABLED}" = "1"; then
AC_SUBST(PNEXUS_CXXFLAGS)
fi
if test "${BUILD_BNMR_LIBS}" = "1"; then
BNMRLIBS_SRCDIR="${SRCDIR}/external/libBNMR"
BNMRLIBS_LIBS="${BNMRLIBS_SRCDIR}/libBNMR.la"
BNMRLIBS_CFLAGS="-I${BNMRLIBS_SRCDIR}"
AC_SUBST(BNMRLIBS_LIBS)
AC_SUBST(BNMRLIBS_CFLAGS)
fi
if test "${BUILD_BMW_LIBS}" = "1"; then
BMWTOOLS_SRCDIR="${SRCDIR}/external/BMWtools"
BMWTOOLS_LIBS="${BMWTOOLS_SRCDIR}/libBMWtools.la"
@ -841,6 +874,8 @@ if test "x$enable_editor" != "xno"; then
echo "Additional checks for musredit/musrgui ..."
QT5MINVER=5.4
case "$host" in
*-*-cygwin)
QT4MINVER=4.5
@ -853,6 +888,7 @@ if test "x$enable_editor" != "xno"; then
QT3_FOUND=no
QT3MT_FOUND=no
QT4_FOUND=no
QT5_FOUND=no
QMAKEBIN=""
QTEDITOR=none
@ -926,14 +962,58 @@ if test "x$enable_editor" != "xno"; then
fi]
)
AC_ARG_WITH([qt5],
[AS_HELP_STRING([--with-qt5],[prefix of the Qt5 installation, e.g. /usr/lib64/qt5/])],
[QT5_PREFIX=$with_qt5
AC_MSG_CHECKING([whether qmake for Qt5 can be found at the specified location])
for QMAKE in qmake qmake-qt5
do
if test -x "${QT5_PREFIX}/bin/${QMAKE}"; then
QMAKEVERSIONSTRING="$(${QT5_PREFIX}/bin/${QMAKE} -v 2>&1)"
for a in $QMAKEVERSIONSTRING
do
if test "$(expr "$a" : '\(..\)')" = "5."; then
QMAKEBIN="${QT5_PREFIX}/bin/${QMAKE}"
QTEDITOR=musredit_qt5
AC_MSG_RESULT([${QMAKEBIN}])
break
fi
done
if test "x${QMAKEBIN}" != "x"; then
break
fi
fi
done
if test "x${QMAKEBIN}" = "x"; then
AC_MSG_RESULT([no])
AC_MSG_ERROR([qmake for Qt5 cannot be found in ${QT5_PREFIX}/bin!])
fi
if test "x${QT4PRESENT}" = "xyes"; then
AC_MSG_WARN([Qt4 and Qt5 directories have been given -- only the Qt5 information will be used and only musredit will be built!])
fi],
[if test "x${QMAKEBIN}" = "x"; then
PKG_CHECK_MODULES(QT5, Qt5WebKit >= $QT5MINVER Qt5Xml >= $QT5MINVER, [QT5_FOUND=yes],
[AC_MSG_NOTICE([Qt5 (including Qt5WebKit and Qt5Xml) not found!])
PKG_CHECK_MODULES(QT3, qt >= 3.3.0 qt < 4.0, [QT3_FOUND=yes],
[PKG_CHECK_MODULES(QT3MT, qt-mt >= 3.3.0 qt-mt < 4.0, [QT3MT_FOUND=yes], [QT3MT_FOUND=no])]
)]
)
fi]
)
if test "x${QMAKEBIN}" = "x"; then
if test "x${QT3_FOUND}" = "xno" && test "x${QT3MT_FOUND}" = "xno" && test "x${QT4_FOUND}" = "xno"; then
AC_MSG_WARN([No suitable version of either Qt4 or Qt3 has been found! musredit/musrgui will not be built in this stage!])
if test "x${QT3_FOUND}" = "xno" && test "x${QT3MT_FOUND}" = "xno" && test "x${QT4_FOUND}" = "xno" && test "x${Qt5_FOUND}" = "xno"; then
AC_MSG_WARN([No suitable version of either Qt5, Qt4 or Qt3 has been found! musredit/musrgui will not be built in this stage!])
else
# Check for qmake on the basis of the pkg-config information
QTPATH=none
if test "x$QT4_FOUND" = "xyes"; then
if test "x$QT5_FOUND" = "xyes"; then
QTPATH=$(pkg-config --variable=prefix Qt5WebKit)
QTEDITOR=musredit_qt5
elif test "x$QT4_FOUND" = "xyes"; then
QTPATH=$(pkg-config --variable=prefix QtWebKit)
QTEDITOR=musredit
elif test "x$QT3_FOUND" = "xyes"; then
@ -946,7 +1026,29 @@ if test "x$enable_editor" != "xno"; then
AC_MSG_CHECKING([for qmake])
if test "x${QTPATH}" != "xnone"; then
if test "x$QTEDITOR" = "xmusredit"; then
if test "x$QTEDITOR" = "xmusredit_qt5"; then
for QMAKE in qmake-qt5 qmake-qt54 qmake-qt55
do
if test -x "${QTPATH}/bin/${QMAKE}"; then
QMAKEBIN="${QTPATH}/bin/${QMAKE}"
AC_MSG_RESULT([${QMAKEBIN}])
break
fi
done
if test "x${QMAKEBIN}" = "x"; then
if test -x "${QTPATH}/bin/qmake"; then
QMAKEVERSIONSTRING="$(${QTPATH}/bin/qmake -v 2>&1)"
for a in $QMAKEVERSIONSTRING
do
if test "$(expr "$a" : '\(..\)')" = "5."; then
QMAKEBIN="${QTPATH}/bin/qmake"
AC_MSG_RESULT([${QMAKEBIN}])
break
fi
done
fi
fi
elif test "x$QTEDITOR" = "xmusredit"; then
for QMAKE in qmake-qt4 qmake-qt46 qmake-qt47 qmake-qt48
do
if test -x "${QTPATH}/bin/${QMAKE}"; then
@ -993,13 +1095,14 @@ if test "x$enable_editor" != "xno"; then
fi
if test "x${QMAKEBIN}" = "x"; then
AC_MSG_RESULT([no])
AC_MSG_WARN([If Qt4 or Qt3 are present but have not been detected, try using the --with-qt4 or --with-qt3 options!])
AC_MSG_WARN([If Qt5, Qt4 or Qt3 are present but have not been detected, try using the --with-qt5, --with-qt4 or --with-qt3 options!])
fi
fi
fi
fi
fi
AM_CONDITIONAL([BUILD_MUSREDIT_QT5], [test "x$enable_editor" != "xno" && test "x${QMAKEBIN}" != "x" && test "x${QTEDITOR}" = "xmusredit_qt5"])
AM_CONDITIONAL([BUILD_MUSREDIT], [test "x$enable_editor" != "xno" && test "x${QMAKEBIN}" != "x" && test "x${QTEDITOR}" = "xmusredit"])
AM_CONDITIONAL([BUILD_MUSRGUI], [test "x$enable_editor" != "xno" && test "x${QMAKEBIN}" != "x" && test "x${QTEDITOR}" = "xmusrgui"])
@ -1111,6 +1214,7 @@ AM_CONDITIONAL([PNEXUS_ENABLED], [test "${PNEXUS_ENABLED}" = "1"])
AM_CONDITIONAL([BUILD_CUBALIB], [test "${BUILD_CUBA}" = "1"])
AM_CONDITIONAL([BUILD_BMWLIBS], [test "${BUILD_BMW_LIBS}" = "1"])
AM_CONDITIONAL([BUILD_ASLIBS], [test "${BUILD_AS_LIBS}" = "1"])
AM_CONDITIONAL([BUILD_BNMRLIBS], [test "${BUILD_BNMR_LIBS}" = "1"])
AC_CONFIG_FILES([Makefile \
src/Makefile \
@ -1151,6 +1255,12 @@ AC_CONFIG_FILES([Makefile \
src/external/libSpinValve/classes/Makefile \
src/external/libPhotoMeissner/Makefile \
src/external/libPhotoMeissner/classes/Makefile \
src/external/libGbGLF/Makefile \
src/external/libBNMR/Makefile \
src/musredit_qt5/Makefile \
src/musredit/Makefile \
src/musrgui/Makefile \
src/musredit_qt5/musredit_startup.xml \
src/musredit/musredit_startup.xml \
src/musrgui/musrgui_startup.xml])
@ -1160,10 +1270,16 @@ if test "x$enable_editor" != "xno" && test "x$QMAKEBIN" != "x"; then
echo "Configuring ${QTEDITOR} ..."
if test "x${QTEDITOR}" = "xmusredit_qt5"; then
QTEDITOR_PRO="musredit"
else
QTEDITOR_PRO=${QTEDITOR}
fi
echo "Changing directory to src/${QTEDITOR} and calling"
echo "${QMAKEBIN} CC=${CC} CXX=${CXX} PREFIX=${INSTALLDIR} ${QTEDITOR}.pro"
echo "${QMAKEBIN} CC=${CC} CXX=${CXX} PREFIX=${INSTALLDIR} ${QTEDITOR_PRO}.pro"
cd src/${QTEDITOR}
${QMAKEBIN} CC=${CC} CXX=${CXX} PREFIX=${INSTALLDIR} ${QTEDITOR}.pro
${QMAKEBIN} CC=${CC} CXX=${CXX} PREFIX=${INSTALLDIR} ${QTEDITOR_PRO}.pro
cd ../..
fi
@ -1270,6 +1386,11 @@ if test "${BUILD_AS_LIBS}" -eq 1; then
else
echo " ASlibs: no"
fi
if test "${BUILD_BNMR_LIBS}" -eq 1; then
echo " BNMRlibs: yes"
else
echo " BNMRlibs: no"
fi
if test "${BUILD_BMW_LIBS}" -eq 1; then
echo " BMWlibs: yes"
else
@ -1277,21 +1398,27 @@ else
fi
echo ""
echo " Qt musrfit editors:"
if test "x$enable_editor" != "xno" && test "x${QMAKEBIN}" != "x" && test "x${QTEDITOR}" = "xmusredit_qt5"; then
echo " musredit (Qt5): yes"
else
echo " musredit (Qt5): no"
fi
if test "x$enable_editor" != "xno" && test "x${QMAKEBIN}" != "x" && test "x${QTEDITOR}" = "xmusredit"; then
echo " musredit (Qt4): yes"
else
echo " musredit (Qt4): no"
fi
if test "x$enable_editor" != "xno" && test "x${QMAKEBIN}" != "x" && test "x${QTEDITOR}" = "xmusrgui"; then
echo " musrgui (Qt3): yes"
echo " musrgui (Qt3): yes"
else
echo " musrgui (Qt3): no"
echo " musrgui (Qt3): no"
fi
echo ""
echo ""
echo " Installation directories:"
echo " -------------------------"
echo ""
echo " Programs and XML configuration files: ${INSTALLDIR}/bin"
echo " Documentation: ${DOCDIR}"
echo " Programs: ${INSTALLDIR}/bin"
echo " XML configuration files: ${HOME}/.musrfit"
echo " Documentation: ${DOCDIR}"
echo ""

View File

@ -12,15 +12,25 @@ ENERGY: 4200
# here the data will follow
data
# x, y, error y
0.02, 12.0, 0.5
0.1, 11.8, 0.8
0.2, 9.9, 0.4
0.33, 7.2, 0.15
0.41, 3.8, 0.38
0.5, 2.7, 0.5
0.64, 1.0, 0.7
0.7, 0.1, 0.2
0.8, 0.0, 0.8
0.9, 0.1, 0.5
1.2, 0.0, 0.1
0.0318411, 7.77455, 0.2
0.0629929, 7.9869, 0.15
0.113914, 7.64209, 0.15
0.202492, 7.37699, 0.15
0.302725, 7.70893, 0.12
0.447456, 7.77565, 0.12
0.611685, 7.45768, 0.12
0.813613, 7.19287, 0.12
1.00822, 7.57813, 0.12
1.24793, 7.31343, 0.12
1.50635, 7.16818, 0.12
1.74591, 6.99634, 0.12
1.99795, 6.90414, 0.12
2.25061, 6.41393, 0.12
2.4958, 6.66666, 0.12
2.75514, 5.93766, 0.12
3.00753, 5.61992, 0.12
3.26056, 4.89091, 0.12
3.49414, 4.52005, 0.08
3.75356, 3.73799, 0.08
3.99425, 2.84974, 0.08
4.30518, 1.35139, 0.08

View File

@ -2,18 +2,16 @@ Test superconductor data
###############################################################
FITPARAMETER
# Nr. Name Value Step Pos_Error Boundaries
1 lambdaInvSq0 11.69 0.39 none
2 Tc 0.558 0.018 none 0 2
3 Delta0 0.0673 0.0035 none
4 aG 1 0 none
1 lambdaInvSq0 7.983 -0.042 0.042
2 Tc 4.470 -0.015 0.016 0 5
3 Delta0 1.547 -0.026 0.027
4 c0 1.468 0 none
5 aG 1.33333 0 none
###############################################################
THEORY
asymmetry 1
userFcn libGapIntegrals TGapSWave 2 3 4
###############################################################
#FUNCTIONS
userFcn libGapIntegrals TGapDWave 2 3 4 5
###############################################################
RUN data/libGapIntegrals-test PIM3 PSI ASCII (name beamline institute data-file-format)
@ -26,15 +24,15 @@ packing 1
###############################################################
COMMANDS
MINIMIZE
HESSE
#MINOS
#HESSE
MINOS
SAVE
###############################################################
PLOT 8 (non muSR plot)
runs 1
range 0 1.5
range 0 6
###############################################################
STATISTIC --- 2014-10-28 10:40:31
chisq = 14.3, NDF = 8, chisq/NDF = 1.790471
STATISTIC --- 2015-06-25 08:39:03
chisq = 58.3, NDF = 19, chisq/NDF = 3.066272

View File

@ -0,0 +1,60 @@
#---------------------------------------------------
# get compilation flags from root-config
ROOTCFLAGS = $(shell $(ROOTSYS)/bin/root-config --cflags)
#---------------------------------------------------
OS = LINUX
CXX = g++
CXXFLAGS = -O3 -Wall -Wno-trigraphs -fPIC
LOCALINCLUDE = .
ROOTINCLUDE = $(ROOTSYS)/include
INCLUDES = -I$(LOCALINCLUDE) -I$(ROOTINCLUDE)
LD = g++
LDFLAGS =
SOFLAGS = -O -shared
# the output from the root-config script:
CXXFLAGS += $(ROOTCFLAGS)
LDFLAGS +=
# some definitions: headers (used to generate *Dict* stuff), sources, objects,...
OBJS =
OBJS += PUserFcn.o PUserFcnDict.o
SHLIB = libPUserFcn.so
# make the shared lib:
#
all: $(SHLIB)
$(SHLIB): $(OBJS)
@echo "---> Building shared library $(SHLIB) ..."
/bin/rm -f $(SHLIB)
$(LD) $(OBJS) $(SOFLAGS) -o $(SHLIB)
@echo "done"
# clean up: remove all object file (and core files)
# semicolon needed to tell make there is no source
# for this target!
#
clean:; @rm -f $(OBJS) *Dict* core*
@echo "---> removing $(OBJS)"
#
$(OBJS): %.o: %.cpp
$(CXX) $(INCLUDES) $(CXXFLAGS) -c $<
# Generate the ROOT CINT dictionary
PUserFcnDict.cpp: PUserFcn.h PUserFcnLinkDef.h
@echo "Generating dictionary $@..."
rootcint -f $@ -c -p -I$(ROOTINCLUDE) $^
install: all
@echo "Installing shared lib: libTApproximation.so"
ifeq ($(OS),LINUX)
cp -pv $(SHLIB) $(ROOTSYS)/lib
cp -pv $(LOCALINCLUDE)/*.h $(ROOTSYS)/include
endif

View File

@ -0,0 +1,59 @@
/***************************************************************************
PUserFcn.cpp
Author: Andreas Suter
e-mail: andreas.suter@psi.ch
***************************************************************************/
/***************************************************************************
* Copyright (C) 2007-2016 by Andreas Suter *
* andreas.suter@psi.ch *
* *
* This program is free software; you can redistribute it and/or modify *
* it under the terms of the GNU General Public License as published by *
* the Free Software Foundation; either version 2 of the License, or *
* (at your option) any later version. *
* *
* This program is distributed in the hope that it will be useful, *
* but WITHOUT ANY WARRANTY; without even the implied warranty of *
* MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the *
* GNU General Public License for more details. *
* *
* You should have received a copy of the GNU General Public License *
* along with this program; if not, write to the *
* Free Software Foundation, Inc., *
* 59 Temple Place - Suite 330, Boston, MA 02111-1307, USA. *
***************************************************************************/
#include <iostream>
using namespace std;
#include <cassert>
#include "PUserFcn.h"
ClassImp(PUserFcn)
//------------------------------------------------------
/**
* <p> user function example: polynome of 3rd order
*
* \f[ = \sum_{k=0}^3 c_k t^k \f]
*
* <b>meaning of paramValues:</b> \f$c_0\f$, \f$c_1\f$, \f$c_2\f$, \f$c_3\f$
*
* <b>return:</b> function value
*
* \param t time in \f$(\mu\mathrm{s})\f$, or x-axis value for non-muSR fit
* \param param parameter vector
*/
Double_t PUserFcn::operator()(Double_t t, const std::vector<Double_t> &param) const
{
// expected parameters: c0, c1, c2, c3
assert(param.size() == 4);
return param[0] + param[1]*t + param[2]*t*t + param[3]*t*t*t;
}

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/***************************************************************************
PUserFcn.h
Author: Andreas Suter
e-mail: andreas.suter@psi.ch
***************************************************************************/
/***************************************************************************
* Copyright (C) 2007-2016 by Andreas Suter *
* andreas.suter@psi.ch *
* *
* This program is free software; you can redistribute it and/or modify *
* it under the terms of the GNU General Public License as published by *
* the Free Software Foundation; either version 2 of the License, or *
* (at your option) any later version. *
* *
* This program is distributed in the hope that it will be useful, *
* but WITHOUT ANY WARRANTY; without even the implied warranty of *
* MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the *
* GNU General Public License for more details. *
* *
* You should have received a copy of the GNU General Public License *
* along with this program; if not, write to the *
* Free Software Foundation, Inc., *
* 59 Temple Place - Suite 330, Boston, MA 02111-1307, USA. *
***************************************************************************/
#ifndef _PUSERFCN_H_
#define _PUSERFCN_H_
#include <vector>
#include "PUserFcnBase.h"
/**
* <p>User function example class. Polynome of 3rd order.
*/
class PUserFcn : public PUserFcnBase
{
public:
PUserFcn() {}
~PUserFcn() {}
// global user-function-access functions, here without any functionality
Bool_t NeedGlobalPart() const { return false; }
void SetGlobalPart(vector<void*> &globalPart, UInt_t idx) { }
Bool_t GlobalPartIsValid() const { return true; }
// function operator
Double_t operator()(Double_t t, const std::vector<Double_t> &param) const;
// definition of the class for the ROOT dictionary
ClassDef(PUserFcn, 1)
};
#endif // _PUSERFCN_H_

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/***************************************************************************
PUserFcnLinkDef.h
***************************************************************************/
#ifdef __CINT__
#pragma link off all globals;
#pragma link off all classes;
#pragma link off all functions;
#pragma link C++ class PUserFcn+;
#endif //__CINT__

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/_/_/_/_/_/_/_/_/_/_/_/_/_/_/_/_/_/_/_/_/_/_/_/_/_/_/_/
Simple Example for a User Function without Global Part
/_/_/_/_/_/_/_/_/_/_/_/_/_/_/_/_/_/_/_/_/_/_/_/_/_/_/_/
Goal: define a user function which implements a polynom
of 3rd order.
For details see: http://lmu.web.psi.ch/musrfit/user/MUSR/MusrFit.html#A_6_User_Functions
Implementation:
3 Files are needed:
1) A header file which defines your user function
interface.
In the example here it is called PUserFcn.h
Please rename it in your case to something more
sensible, e.g. PMyPoly.h. At the same time also
rename correspondingly the class name in your
header file, i.e. PUserFcn -> PMyPoly. This will
be at 4 places in the header file of this example.
2) The source file which defines your user function.
In the example here it is called PUserFcn.cpp
Please rename it accordingly to the header file.
In case the header file is called PMyPoly.h, the
source file will need to be called PMyPoly.cpp.
As for the header file, the class names need to
be adopted: PUserFcn -> PMyPoly.
In the source file change the operator implementation
(Double_t PUserFcn::operator()(Double_t t,
const std::vector<Double_t> &param) const)
to whatever you need.
3) There is another header file needed to generate
the necessary ROOT dictionary.
In this example it is called PUserFcnLinkDef.h
Here you only will need to find PUserFcn+ and
replace it with your class name, e.g. PMyPoly+
Generate Code:
You will find the Makefil.PUserFcn which generates
the needed shared library for your user function.
Again, if your user function is called PMyPoly, you
will need to replace things accordingly in the
Makefile, i.e.
Makefile.PUserFcn -> Makefile.PMyPoly
In the Makefile:
PUserFcn.o -> PMyPoly.o
PUserFcnDict.o -> PMyPolyDict.o
libPUserFcn.so -> libPMyPoly.so
To create the shared library do:
make -f Makefile.PUserFcn
on the command line. This should create a file
libPUserFcn.so.
Next call on the command line:
make -f Makefile.PUserFcn install
This will copy the shared library to the correct
place.
You also will need to make sure that the system is
finding the shared library, either by setting
LD_LIBRARY_PATH or by calling /sbin/ldconfig as
superuser/root assuming you are using linux.
Example msr-file:
You will find an example msr-file test-asy-MUS.msr
which is using PUserFcn. The example is UN-PHYSICALLY
it is just to show how to use a user function.

Binary file not shown.

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MgB12H12 No2 ZF T=150
###############################################################
FITPARAMETER
# Nr. Name Value Step Pos_Error Boundaries
1 alpha 1 0 none 0 2
2 asy 0.1650 0.0027 none 0 0.33
3 c0 1.047 0.016 none
4 c1 -0.1957 0.0038 none
5 c2 0.0216 0.0011 none
6 c3 -0.00119 0.00011 none
###############################################################
THEORY
asymmetry 2
userFcn libPUserFcn PUserFcn 3 4 5 6
###############################################################
RUN data/000100 XXXX TRIUMF MUD (name beamline institute data-file-format)
fittype 2 (asymmetry fit)
alpha 1
map 0 0 0 0 0 0 0 0 0 0 0
forward 1
backward 2
background 79 391 80 409 # estimated bkg: 21.0833 / 17.2249
data 438 12785 436 12787
t0 432.0 431.0
fit 0 8
packing 100
###############################################################
COMMANDS
MINIMIZE
MINOS
#HESSE
SAVE
###############################################################
FOURIER
units Gauss # units either 'Gauss', 'Tesla', 'MHz', or 'Mc/s'
fourier_power 12
apodization NONE # NONE, WEAK, MEDIUM, STRONG
plot POWER # REAL, IMAG, REAL_AND_IMAG, POWER, PHASE
phase 8
#range_for_phase_correction 50.0 70.0
range 0 2000
dc-corrected true
###############################################################
PLOT 2 (asymmetry plot)
runs 1
range 0 9 0 0.22
###############################################################
STATISTIC --- 2016-06-22 09:34:01
chisq = 152.4, NDF = 97, chisq/NDF = 1.571461

Binary file not shown.

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MnSi, FLC68.2, 50 K
###############################################################
FITPARAMETER
# Nr. Name Value Step Pos_Error Boundaries
1 rate_1 1.680 0.019 none
2 field_1 1589.71 0.20 none
3 rate_2 1.863 0.065 none
4 field_2 788.86 0.49 none
5 alpha_f15 1.0029 0.0015 none
6 frac_f15 0.7350 0.0090 none
7 asym_f15 0.2713 0.0043 none 0 none
8 phase_f15 79.37 0.80 none
9 alpha_f26 0.9996 0.0015 none
10 frac_f26 0.7408 0.0085 none
11 asym_f26 0.3029 0.0046 none 0 none
12 phase_f26 30.22 0.73 none
13 alpha_f37 1.0003 0.0015 none
14 frac_f37 0.88 0.23 none
15 asym_f37 0.0126 0.0045 none 0 none
16 phase_f37 58.0 15.0 none
17 alpha_f48 0.9999 0.0015 none
18 frac_f48 0.7344 0.0084 none
19 asym_f48 0.2929 0.0043 none 0 none
20 phase_f48 -33.13 0.76 none
21 alpha_b15 0.9991 0.0013 none
22 frac_b15 0.7439 0.0077 none
23 asym_b15 0.2807 0.0038 none 0 none
24 phase_b15 164.98 0.68 none
25 alpha_b26 1.0003 0.0013 none
26 frac_b26 0.7331 0.0078 none
27 asym_b26 0.2810 0.0038 none 0 none
28 phase_b26 119.49 0.70 none
29 alpha_b37 0.9989 0.0012 none
30 frac_b37 0.7504 0.0078 none
31 asym_b37 0.2755 0.0037 none 0 none
32 phase_b37 102.07 0.69 none
33 alpha_b48 0.9990 0.0012 none
34 frac_b48 0.7391 0.0080 none
35 asym_b48 0.2763 0.0039 none 0 none
36 phase_b48 37.66 0.67 none
###############################################################
THEORY
asymmetry fun1
simplExpo 1 (rate)
TFieldCos map3 fun3 (phase frequency)
+
asymmetry fun2
simplExpo 3 (rate)
TFieldCos map3 fun4 (phase frequency)
###############################################################
FUNCTIONS
fun1 = map1 * map2
fun2 = (1 - map1) * map2
fun3 = gamma_mu * par2
fun4 = gamma_mu * par4
###############################################################
GLOBAL
fittype 3 (asymmetry RRF fit)
fit 0.0005 6
rrf_freq 7.15 T
rrf_packing 300
rrf_phase 0.00
###############################################################
# Fw1-Fw5 +++++++
RUN data/tdc_hifi_2014_00153 PIE3 PSI PSI-MDU (name beamline institute data-file-format)
alpha 5
map 6 7 8 0 0 0 0 0 0 0 0
forward 2
backward 6
background 500 15000 500 15000 # estimated bkg: 0.0492 / 0.0501
data 20158 409500 20130 409500
t0 20108.0 20080.0
# Fw2-Fw6 +++++++
RUN data/tdc_hifi_2014_00153 PIE3 PSI PSI-MDU (name beamline institute data-file-format)
alpha 9
map 10 11 12 0 0 0 0 0 0 0 0
forward 3
backward 7
background 500 15000 500 15000 # estimated bkg: 0.0501 / 0.0451
data 20138 409500 20121 409500
t0 20088.0 20071.0
# Fw3-Fw7 +++++++
RUN data/tdc_hifi_2014_00153 PIE3 PSI PSI-MDU (name beamline institute data-file-format)
alpha 13
map 14 15 16 0 0 0 0 0 0 0 0
forward 3
backward 8
background 500 15000 500 15000 # estimated bkg: 0.0501 / 0.0449
data 20111 409500 20116 409500
t0 20061.0 20066.0
# Fw4-Fw8 +++++++
RUN data/tdc_hifi_2014_00153 PIE3 PSI PSI-MDU (name beamline institute data-file-format)
alpha 17
map 18 19 20 0 0 0 0 0 0 0 0
forward 5
backward 9
background 500 15000 500 15000 # estimated bkg: 0.0560 / 0.0462
data 20121 409500 20082 409500
t0 20071.0 20032.0
# Bw1-Bw5 +++++++
RUN data/tdc_hifi_2014_00153 PIE3 PSI PSI-MDU (name beamline institute data-file-format)
alpha 21
map 22 23 24 0 0 0 0 0 0 0 0
forward 10
backward 14
background 500 15000 500 15000 # estimated bkg: 0.0641 / 0.0806
data 20072 409500 20067 409500
t0 20022.0 20017.0
# Bw2-Bw6 +++++++
RUN data/tdc_hifi_2014_00153 PIE3 PSI PSI-MDU (name beamline institute data-file-format)
alpha 25
map 26 27 28 0 0 0 0 0 0 0 0
forward 11
backward 15
background 500 15000 500 15000 # estimated bkg: 0.0689 / 0.0768
data 20076 409500 20069 409500
t0 20026.0 20019.0
# Bw3-Bw7 +++++++
RUN data/tdc_hifi_2014_00153 PIE3 PSI PSI-MDU (name beamline institute data-file-format)
alpha 29
map 30 31 32 0 0 0 0 0 0 0 0
forward 12
backward 16
background 500 15000 500 15000 # estimated bkg: 0.0769 / 0.0795
data 20060 409500 20069 409500
t0 20010.0 20019.0
# Bw4-Bw8 +++++++
RUN data/tdc_hifi_2014_00153 PIE3 PSI PSI-MDU (name beamline institute data-file-format)
alpha 33
map 34 35 36 0 0 0 0 0 0 0 0
forward 13
backward 17
background 500 15000 500 15000 # estimated bkg: 0.0761 / 0.0702
data 20063 409500 20089 409500
t0 20013.0 20039.0
###############################################################
COMMANDS
#MAX_LIKELIHOOD
PRINT_LEVEL 2
MINIMIZE
#MINOS
SAVE
###############################################################
PLOT 3 (asymmetry RRF plot)
runs 1 2 3 4 5 6 7 8
range 0 9.07 -0.5 0.5
###############################################################
FOURIER
units Gauss # units either 'Gauss', 'Tesla', 'MHz', or 'Mc/s'
fourier_power 11
apodization STRONG # NONE, WEAK, MEDIUM, STRONG
plot POWER # REAL, IMAG, REAL_AND_IMAG, POWER, PHASE
###############################################################
STATISTIC --- 2016-01-18 16:23:00
chisq = 7402.2, NDF = 6516, chisq/NDF = 1.135997

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@ -0,0 +1,235 @@
MnSi, FLC68.2, 50 K
###############################################################
FITPARAMETER
# Nr. Name Value Step Pos_Error Boundaries
1 Rate_1 1.678 0.018 none
2 Field_1_RRF 1589.66 0.19 none
3 Rate_2 1.948 0.064 none
4 Field_2_RRF 788.93 0.47 none
5 Asym_1 0.3102 0.0067 none
6 Frc_1 0.728 0.012 none
7 Phase_1 57.3 1.1 none
8 Asym_2 0.3073 0.0066 none
9 Frc_2 0.748 0.012 none
10 Phase_2 30.6 1.0 none
11 Asym_3 0.3245 0.0065 none
12 Frc_3 0.728 0.011 none
13 Phase_3 18.70 0.96 none
14 Asym_4 0.3290 0.0062 none
15 Frc_4 0.733 0.011 none
16 Phase_4 339.27 0.96 none
17 Asym_5 0.3213 0.0062 none
18 Frc_5 0.730 0.011 none
19 Phase_5 282.5 1.0 none
20 Asym_6 0.3424 0.0072 none
21 Frc_6 0.726 0.012 none
22 Phase_6 211.3 1.0 none
23 Asym_7 0.3321 0.0069 none
24 Frc_7 0.731 0.012 none
25 Phase_7 161.7 1.1 none
26 Asym_8 0.3219 0.0067 none
27 Frc_8 0.730 0.012 none
28 Phase_8 133.7 1.1 none
29 Asym_9 0.3030 0.0058 none
30 Frc_9 0.730 0.011 none
31 Phase_9 158.87 0.97 none
32 Asym_10 0.3046 0.0057 none
33 Frc_10 0.731 0.011 none
34 Phase_10 129.97 0.97 none
35 Asym_11 0.2898 0.0055 none
36 Frc_11 0.754 0.011 none
37 Phase_11 101.80 0.96 none
38 Asym_12 0.3013 0.0055 none
39 Frc_12 0.740 0.010 none
40 Phase_12 43.00 0.88 none
41 Asym_13 0.3009 0.0054 none
42 Frc_13 0.747 0.010 none
43 Phase_13 351.72 0.88 none
44 Asym_14 0.3054 0.0053 none
45 Frc_14 0.729 0.010 none
46 Phase_14 289.91 0.91 none
47 Asym_15 0.2931 0.0053 none
48 Frc_15 0.740 0.010 none
49 Phase_15 282.39 0.94 none
50 Asym_16 0.2814 0.0058 none
51 Frc_16 0.729 0.011 none
52 Phase_16 212.89 0.99 none
###############################################################
THEORY
asymmetry fun1
simplExpo 1 (rate)
TFieldCos map3 fun3 (phase frequency)
+
asymmetry fun2
simplExpo 3 (rate)
TFieldCos map3 fun4 (phase frequency)
###############################################################
FUNCTIONS
fun1 = map1 * map2
fun2 = map1 * (1 - map2)
fun3 = par2 * gamma_mu
fun4 = par4 * gamma_mu
###############################################################
GLOBAL
fittype 1 (single histogram RRF fit)
rrf_freq 7.15 T
rrf_packing 300
rrf_phase 0.00
fit 0.0005 10
###############################################################
RUN data/tdc_hifi_2014_00153 PIE3 PSI PSI-MDU (name beamline institute data-file-format)
map 5 6 7 0 0 0 0 0 0 0 0
forward 2
background 100 18000 # estimated bkg: 0.0476
data 20208 409500
t0 20108.0
#--------------------------------------------------------------
RUN data/tdc_hifi_2014_00153 PIE3 PSI PSI-MDU (name beamline institute data-file-format)
map 8 9 10 0 0 0 0 0 0 0 0
forward 3
background 100 18000 # estimated bkg: 0.0490
data 20188 409500
t0 20088.0
#--------------------------------------------------------------
RUN data/tdc_hifi_2014_00153 PIE3 PSI PSI-MDU (name beamline institute data-file-format)
map 11 12 13 0 0 0 0 0 0 0 0
forward 4
background 100 18000 # estimated bkg: 0.0582
data 20161 409500
t0 20061.0
#--------------------------------------------------------------
RUN data/tdc_hifi_2014_00153 PIE3 PSI PSI-MDU (name beamline institute data-file-format)
map 14 15 16 0 0 0 0 0 0 0 0
forward 5
background 100 18000 # estimated bkg: 0.0553
data 20171 409500
t0 20071.0
#--------------------------------------------------------------
RUN data/tdc_hifi_2014_00153 PIE3 PSI PSI-MDU (name beamline institute data-file-format)
map 17 18 19 0 0 0 0 0 0 0 0
forward 6
background 100 18000 # estimated bkg: 0.0515
data 20180 409500
t0 20080.0
#--------------------------------------------------------------
RUN data/tdc_hifi_2014_00153 PIE3 PSI PSI-MDU (name beamline institute data-file-format)
map 20 21 22 0 0 0 0 0 0 0 0
forward 7
background 100 18000 # estimated bkg: 0.0458
data 20171 409500
t0 20071.0
#--------------------------------------------------------------
RUN data/tdc_hifi_2014_00153 PIE3 PSI PSI-MDU (name beamline institute data-file-format)
map 23 24 25 0 0 0 0 0 0 0 0
forward 8
background 100 18000 # estimated bkg: 0.0466
data 20166 409500
t0 20066.0
#--------------------------------------------------------------
RUN data/tdc_hifi_2014_00153 PIE3 PSI PSI-MDU (name beamline institute data-file-format)
map 26 27 28 0 0 0 0 0 0 0 0
forward 9
background 100 18000 # estimated bkg: 0.0457
data 20132 409500
t0 20032.0
#--------------------------------------------------------------
RUN data/tdc_hifi_2014_00153 PIE3 PSI PSI-MDU (name beamline institute data-file-format)
map 29 30 31 0 0 0 0 0 0 0 0
forward 10
background 100 18000 # estimated bkg: 0.0635
data 20122 409500
t0 20022.0
#--------------------------------------------------------------
RUN data/tdc_hifi_2014_00153 PIE3 PSI PSI-MDU (name beamline institute data-file-format)
map 32 33 34 0 0 0 0 0 0 0 0
forward 11
background 100 18000 # estimated bkg: 0.0685
data 20126 409500
t0 20026.0
#--------------------------------------------------------------
RUN data/tdc_hifi_2014_00153 PIE3 PSI PSI-MDU (name beamline institute data-file-format)
map 35 36 37 0 0 0 0 0 0 0 0
forward 12
background 100 18000 # estimated bkg: 0.0752
data 20110 409500
t0 20010.0
#--------------------------------------------------------------
RUN data/tdc_hifi_2014_00153 PIE3 PSI PSI-MDU (name beamline institute data-file-format)
map 38 39 40 0 0 0 0 0 0 0 0
forward 13
background 100 18000 # estimated bkg: 0.0760
data 20113 409500
t0 20013.0
#--------------------------------------------------------------
RUN data/tdc_hifi_2014_00153 PIE3 PSI PSI-MDU (name beamline institute data-file-format)
map 41 42 43 0 0 0 0 0 0 0 0
forward 14
background 100 18000 # estimated bkg: 0.0809
data 20117 409500
t0 20017.0
#--------------------------------------------------------------
RUN data/tdc_hifi_2014_00153 PIE3 PSI PSI-MDU (name beamline institute data-file-format)
map 44 45 46 0 0 0 0 0 0 0 0
forward 15
background 100 18000 # estimated bkg: 0.0755
data 20119 409500
t0 20019.0
#--------------------------------------------------------------
RUN data/tdc_hifi_2014_00153 PIE3 PSI PSI-MDU (name beamline institute data-file-format)
map 47 48 49 0 0 0 0 0 0 0 0
forward 16
background 100 18000 # estimated bkg: 0.0796
data 20119 409500
t0 20019.0
#--------------------------------------------------------------
RUN data/tdc_hifi_2014_00153 PIE3 PSI PSI-MDU (name beamline institute data-file-format)
map 50 51 52 0 0 0 0 0 0 0 0
forward 17
background 100 18000 # estimated bkg: 0.0702
data 20139 409500
t0 20039.0
###############################################################
COMMANDS
#MAX_LIKELIHOOD
PRINT_LEVEL 2
MINIMIZE
#MINOS
SAVE
###############################################################
PLOT 1 (single histo RRF plot)
runs 1 2 3 4 5 6 7 8 9 10 11 12 13 14 15 16
range 0 9.07 -0.5 0.5
###############################################################
FOURIER
units Gauss # units either 'Gauss', 'Tesla', 'MHz', or 'Mc/s'
fourier_power 12
apodization MEDIUM # NONE, WEAK, MEDIUM, STRONG
plot POWER # REAL, IMAG, REAL_AND_IMAG, POWER, PHASE
#range 7.1 7.5
###############################################################
STATISTIC --- 2016-01-14 13:24:36
chisq = 22007.6, NDF = 20700, chisq/NDF = 1.063168

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@ -0,0 +1,199 @@
07770 - test
###############################################################
FITPARAMETER
# Nr. Name Value Step Pos_Error Boundaries
1 N_0 321.0 1.4 none
2 tau_0 1.9066 0.0038 none 0 none
3 Rate_0 0.0983 0.0052 none 0 none
4 Freq_0 135.53824 0.00073 none
5 N_1 306.1 1.3 none
6 tau_1 0.7409 0.0026 none 0 none
7 Rate_1 0.026 0.027 none 0 none
8 Freq_1 136.8968 0.0033 none
9 Asym_F1_0 0.0490 0.0015 none 0 none
10 Asym_F1_1 0.0501 0.0029 none 0 none
11 Phase_F1 4.9 1.5 none
12 N_bgk_F1 1.880 0.034 none
13 Asym_F2_0 0.0496 0.0015 none 0 none
14 Asym_F2_1 0.0581 0.0030 none 0 none
15 Phase_F2 52.4 1.5 none
16 N_bgk_F2 1.508 0.033 none
17 Asym_F3_0 0.0486 0.0015 none 0 none
18 Asym_F3_1 0.0593 0.0030 none 0 none
19 Phase_F3 95.2 1.5 none
20 N_bgk_F3 1.465 0.033 none
21 Asym_F4_0 0.0512 0.0015 none 0 none
22 Asym_F4_1 0.0521 0.0029 none 0 none
23 Phase_F4 144.6 1.5 none
24 N_bgk_F4 2.311 0.034 none
25 Asym_F5_0 0.0542 0.0015 none 0 none
26 Asym_F5_1 0.0537 0.0030 none 0 none
27 Phase_F5 188.4 1.4 none
28 N_bgk_F5 1.799 0.033 none
29 Asym_F6_0 0.0502 0.0015 none 0 none
30 Asym_F6_1 0.0517 0.0030 none 0 none
31 Phase_F6 232.1 1.5 none
32 N_bgk_F6 1.735 0.033 none
33 Asym_F7_0 0.0488 0.0015 none 0 none
34 Asym_F7_1 0.0575 0.0030 none 0 none
35 Phase_F7 273.0 1.5 none
36 N_bgk_F7 1.593 0.033 none
37 Asym_F8_0 0.0547 0.0015 none 0 none
38 Asym_F8_1 0.0468 0.0029 none 0 none
39 Phase_F8 321.7 1.4 none
40 N_bgk_F8 1.469 0.033 none
41 Asym_B1_0 0.0476 0.0015 none 0 none
42 Asym_B1_1 0.0535 0.0029 none 0 none
43 Phase_B1 3.6 1.5 none
44 N_bgk_B1 1.378 0.033 none
45 Asym_B2_0 0.0524 0.0015 none 0 none
46 Asym_B2_1 0.0495 0.0030 none 0 none
47 Phase_B2 53.7 1.5 none
48 N_bgk_B2 1.272 0.032 none
49 Asym_B3_0 0.0494 0.0015 none 0 none
50 Asym_B3_1 0.0555 0.0030 none 0 none
51 Phase_B3 98.1 1.5 none
52 N_bgk_B3 0.969 0.032 none
53 Asym_B4_0 0.0505 0.0015 none 0 none
54 Asym_B4_1 0.0527 0.0030 none 0 none
55 Phase_B4 141.8 1.5 none
56 N_bgk_B4 1.233 0.032 none
57 Asym_B5_0 0.0515 0.0015 none 0 none
58 Asym_B5_1 0.0584 0.0030 none 0 none
59 Phase_B5 182.2 1.4 none
60 N_bgk_B5 1.642 0.033 none
61 Asym_B6_0 0.0512 0.0015 none 0 none
62 Asym_B6_1 0.0477 0.0029 none 0 none
63 Phase_B6 231.7 1.5 none
64 N_bgk_B6 1.650 0.033 none
65 Asym_B7_0 0.0514 0.0015 none 0 none
66 Asym_B7_1 0.0539 0.0030 none 0 none
67 Phase_B7 275.2 1.5 none
68 N_bgk_B7 1.729 0.033 none
69 Asym_B8_0 0.0541 0.0015 none 0 none
70 Asym_B8_1 0.0444 0.0030 none 0 none
71 Phase_B8 321.0 1.5 none
72 N_bgk_B8 1.136 0.032 none
###############################################################
THEORY
muMinusExpTF 1 2 map1 3 map3 4 (N0 tau A lambda phase nu)
+
muMinusExpTF 5 6 map2 7 map3 8 (N0 tau A lambda phase nu)
+
asymmetry map4
###############################################################
GLOBAL
fittype 4 (mu minus fit)
t0 20000.0
data 20100 409500
fit 0.0005 9
packing 25
###############################################################
RUN data/07770 PIE3 PSI MUSR-ROOT (name beamline institute data-file-format)
map 9 10 11 12 0 0 0 0 0 0 0 0
forward 1
#--------------------------------------------------------------
RUN data/07770 PIE3 PSI MUSR-ROOT (name beamline institute data-file-format)
map 13 14 15 16 0 0 0 0 0 0 0 0
forward 2
#--------------------------------------------------------------
RUN data/07770 PIE3 PSI MUSR-ROOT (name beamline institute data-file-format)
map 17 18 19 20 0 0 0 0 0 0 0 0
forward 3
#--------------------------------------------------------------
RUN data/07770 PIE3 PSI MUSR-ROOT (name beamline institute data-file-format)
map 21 22 23 24 0 0 0 0 0 0 0 0
forward 4
#--------------------------------------------------------------
RUN data/07770 PIE3 PSI MUSR-ROOT (name beamline institute data-file-format)
map 25 26 27 28 0 0 0 0 0 0 0 0
forward 5
#--------------------------------------------------------------
RUN data/07770 PIE3 PSI MUSR-ROOT (name beamline institute data-file-format)
map 29 30 31 32 0 0 0 0 0 0 0 0
forward 6
#--------------------------------------------------------------
RUN data/07770 PIE3 PSI MUSR-ROOT (name beamline institute data-file-format)
map 33 34 35 36 0 0 0 0 0 0 0 0
forward 7
#--------------------------------------------------------------
RUN data/07770 PIE3 PSI MUSR-ROOT (name beamline institute data-file-format)
map 37 38 39 40 0 0 0 0 0 0 0 0
forward 8
#--------------------------------------------------------------
RUN data/07770 PIE3 PSI MUSR-ROOT (name beamline institute data-file-format)
map 41 42 43 44 0 0 0 0 0 0 0 0
forward 9
#--------------------------------------------------------------
RUN data/07770 PIE3 PSI MUSR-ROOT (name beamline institute data-file-format)
map 45 46 47 48 0 0 0 0 0 0 0 0
forward 10
#--------------------------------------------------------------
RUN data/07770 PIE3 PSI MUSR-ROOT (name beamline institute data-file-format)
map 49 50 51 52 0 0 0 0 0 0 0 0
forward 11
#--------------------------------------------------------------
RUN data/07770 PIE3 PSI MUSR-ROOT (name beamline institute data-file-format)
map 53 54 55 56 0 0 0 0 0 0 0 0
forward 12
#--------------------------------------------------------------
RUN data/07770 PIE3 PSI MUSR-ROOT (name beamline institute data-file-format)
map 57 58 59 60 0 0 0 0 0 0 0 0
forward 13
#--------------------------------------------------------------
RUN data/07770 PIE3 PSI MUSR-ROOT (name beamline institute data-file-format)
map 61 62 63 64 0 0 0 0 0 0 0 0
forward 14
#--------------------------------------------------------------
RUN data/07770 PIE3 PSI MUSR-ROOT (name beamline institute data-file-format)
map 65 66 67 68 0 0 0 0 0 0 0 0
forward 15
#--------------------------------------------------------------
RUN data/07770 PIE3 PSI MUSR-ROOT (name beamline institute data-file-format)
map 69 70 71 72 0 0 0 0 0 0 0 0
forward 16
###############################################################
COMMANDS
MAX_LIKELIHOOD
PRINT_LEVEL 2
MINIMIZE
#MINOS
SAVE
###############################################################
PLOT 4 (mu minus plot)
runs 1-16
range 0 9
###############################################################
FOURIER
units Tesla # units either 'Gauss', 'Tesla', 'MHz', or 'Mc/s'
fourier_power 14
apodization MEDIUM # NONE, WEAK, MEDIUM, STRONG
plot POWER # REAL, IMAG, REAL_AND_IMAG, POWER, PHASE
range 0.8 1.2
###############################################################
STATISTIC --- 2016-04-25 17:05:56
maxLH = 238962.5, NDF = 230264, maxLH/NDF = 1.037776

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<h1><a name="BMWlibs_for_61musrfit_61"></a> BMWlibs for <code>musrfit</code> </h1> <ul>
<h1 id="BMWlibs_for_61musrfit_61"> BMWlibs for <code>musrfit</code> </h1> <ul>
<li> <a href="LibFitPofB.html"> <code>libFitPofB</code>: routines for calculating transverse-field muon-spin depolarization functions from various static field distributions in superconductors</a>
</li> <li> <a href="LibZFRelaxation.html"> <code>libZFRelaxation</code>: routines for calculating zero-field muon-spin depolarization functions from various static field distributions</a>
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</div><div class="patternContent"><div class="foswikiTopic"><h1><a name="How_to_Cite_61musrfit_61_63"></a> How to Cite <code>musrfit</code>? </h1>
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<div class="patternContent"><div class="foswikiTopic"> <h1 id="How_to_Cite_61musrfit_61_63"> How to Cite <code>musrfit</code>? </h1>
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Since quite some effort is going into the development and maintenance of the <code>musrfit</code> package, you should at least acknowledge it in your publication if you have used it to analyze your data. Even better of course is to cite it properly by the reference given beneath
<p></p> <ul>
<li> <a href="http://dx.doi.org/10.1016/j.phpro.2012.04.042" target="_top">A. Suter, B.M. Wojek, "Musrfit: A Free Platform-Independent Framework for &mu;SR Data Analysis", Physics Procedia 30, 69 (2012).</a>
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<li> <a href="http://dx.doi.org/10.1016/j.phpro.2012.04.042">A. Suter, B.M. Wojek, "Musrfit: A Free Platform-Independent Framework for &mu;SR Data Analysis", Physics Procedia 30, 69 (2012).</a>
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</div></div><div class="patternInfo"><span class="patternRevInfo">Topic revision: r2 - 19 Jun 2012, <a href="https://intranet.psi.ch/Main/AndreasSuter">AndreasSuter</a></span></div>
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<h1><a name="libFitPofB"></a> libFitPofB </h1>
<a name="foswikiTOC"></a><div class="foswikiToc"> <ul>
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<h1 id="libFitPofB"> libFitPofB </h1>
<div class="foswikiToc" id="foswikiTOC"> <ul>
<li> <a href="LibFitPofB.html#libFitPofB"> libFitPofB </a>
</li> <li> <a href="LibFitPofB.html#A_1_Introduction"> 1 Introduction </a>
</li> <li> <a href="LibFitPofB.html#A_2_LE_45SR"> 2 LE-&mu;SR </a> <ul>
@ -130,28 +137,28 @@ pre {
</li> <li> <a href="LibFitPofB.html#A_4_The_XML_startup_file"> 4 The XML startup file </a>
</li></ul>
</div>
<a name="IntroDuction"></a>
<h1><a name="A_1_Introduction"></a> 1 Introduction </h1>
<span id="IntroDuction"></span>
<h1 id="A_1_Introduction"> 1 Introduction </h1>
<p></p>
<code>libFitPofB</code> is a collection of <code>C++</code> classes using the <code><a href="MusrFit.html">musrfit</a></code> <code><a href="MusrFit.html#UserFunctions1">user-function interface</a></code> in order to facilitate the usage in conjunction with <code>musrfit</code>. The classes contained in this library generally implement calculations of one-dimensional static magnetic field distributions <img alt="P(B)" class="mmpImage" src="../pub/MUSR/LibFitPofB/_MathModePlugin_9cc0fd47eedada7247b14775bd308deb.png" title="PofB" /> which lead to muon-spin depolarization functions
<p style="text-align:center">
<img alt="\mathcal{P}(t) &#61; \int P(B)\cos\left(\gamma&#95;{\mu} B t + \varphi\right) \mathrm{d}B," class="mmpImage" src="../pub/MUSR/LibFitPofB/_MathModePlugin_70e57aa1afa7d337fa46f427b34feb54.png" title="PofT" />
</p>
where <img alt="\gamma&#95;{\mu} &#61; 2\pi\times 135.54~\mathrm{MHz/T}" class="mmpImage" src="../pub/MUSR/LibFitPofB/_MathModePlugin_9bb7e08c8e276a92650d89d6918b3769.png" title="gamma_mu" /> is the gyromagnetic ratio of the muon and <img alt="\varphi" class="mmpImage" src="../pub/MUSR/LibFitPofB/_MathModePlugin_2339fd9b358ebe241da05c665668d48b.png" title="phi" /> is the initial phase of the muon spins with respect to the positron detector.<br>
At the moment the only available implementations deal with field distributions measured in local isotropic superconductors, either by means of <a href="http://lmu.web.psi.ch/lem/" target="_top">low-energy &mu;SR</a> in the Meissner state or by conventional &mu;SR in the mixed state. In the following the basic usage of the library in <code>musrfit</code> is explained&mdash;the calculations by themselves are only outlined. For further information please refer to the original literature and/or the source code of the implementation.
At the moment the only available implementations deal with field distributions measured in local isotropic superconductors, either by means of <a href="http://lmu.web.psi.ch/lem/">low-energy &mu;SR</a> in the Meissner state or by conventional &mu;SR in the mixed state. In the following the basic usage of the library in <code>musrfit</code> is explained&mdash;the calculations by themselves are only outlined. For further information please refer to the original literature and/or the source code of the implementation.
<p></p>
<hr />
<strong><span class='foswikiBlackFG'>Remark 1:</span></strong> In order to supply certain information needed for the calculations but not suited to be stored in the <code>musrfit</code> msr files an XML configuration file in the working directory is used. For details, see <a href="#XmlFile" class="foswikiCurrentTopicLink">below</a>.
<strong><span class='foswikiBlackFG'>Remark 1:</span></strong> In order to supply certain information needed for the calculations but not suited to be stored in the <code>musrfit</code> msr files an XML configuration file in the working directory is used. For details, see <a class="foswikiCurrentTopicLink" href="#XmlFile">below</a>.
<p></p>
<strong><span class='foswikiBlackFG'>Remark 2:</span></strong> The implementations in this library heavily rely on <code><a href="http://www.fftw.org/" target="_top">FFTW3</a></code>. In principle, it always checks what is the best way to do efficient Fourier transforms for a given machine before the transforms are actually done. If repeatedly Fourier transforms of the same (sizable) length should be done, it might be worth storing the once obtained information in an external file and just load it the next time this information is needed (<a href="http://fftw.org/fftw3_doc/Wisdom.html" target="_top">"wisdom handling"</a>). In case this feature shall be used, a valid wisdom file has to be specified in the <a href="#XmlFile" class="foswikiCurrentTopicLink">XML file</a>.
<strong><span class='foswikiBlackFG'>Remark 2:</span></strong> The implementations in this library heavily rely on <code><a href="http://www.fftw.org/">FFTW3</a></code>. In principle, it always checks what is the best way to do efficient Fourier transforms for a given machine before the transforms are actually done. If repeatedly Fourier transforms of the same (sizable) length should be done, it might be worth storing the once obtained information in an external file and just load it the next time this information is needed (<a href="http://fftw.org/fftw3_doc/Wisdom.html">"wisdom handling"</a>). In case this feature shall be used, a valid wisdom file has to be specified in the <a class="foswikiCurrentTopicLink" href="#XmlFile">XML file</a>.
<p></p>
<strong><span class='foswikiBlackFG'>Remark 3:</span></strong> The model functions described in the following do generally not behave nicely in conjunction with <code>MINUIT</code> function minimizations (or maximizations). The analysis process at the moment in most cases involves some tedious <em>trial-and-error</em> procedure, where the displayed <code>MINUIT</code> information as always deserves attention. This is especially true if small effects should be analyzed (e.g. small diamagnetic shifts in superconductors). The parameter uncertainty in many cases has to be estimated independently. Due to these limitations, also the use of the fit option of <code><a href="Msr2Data.html">msr2data</a></code> cannot be advised.
<p></p>
<strong><span class='foswikiBlackFG'>Remark 4:</span></strong> If these classes still prove useful and results obtained through them are part of scientific publications,
an acknowledgement of the use of the library is appreciated.
<p></p>
<h1><a name="A_2_LE_45SR"></a> 2 LE-&mu;SR </h1>
<h2><a name="A_2.1_One_45dimensional_London_model_for_the_Meissner_state_of_isotropic_superconductors"></a> 2.1 One-dimensional London model for the Meissner state of isotropic superconductors </h2>
<h1 id="A_2_LE_45SR"> 2 LE-&mu;SR </h1>
<h2 id="A_2.1_One_45dimensional_London_model_for_the_Meissner_state_of_isotropic_superconductors"> 2.1 One-dimensional London model for the Meissner state of isotropic superconductors </h2>
<p></p>
The models for analyzing LE-&mu;SR data assume the magnetic induction <img alt="B(z)" class="mmpImage" src="../pub/MUSR/LibFitPofB/_MathModePlugin_532f98969690650ac4d127919a0eda38.png" title="BofZ" /> to vary only in the dimension parallel to the momentum of the incident muons. In such a case the magnetic field distribution is given by
<p style="text-align:center">
@ -163,7 +170,7 @@ Assuming an array of <img alt="N" class="mmpImage" src="../pub/MUSR/LibFitPofB/_
<p style="text-align:center">
<img alt="\frac{\partial^2}{\partial z^2}B&#95;i(z) &#61; \frac{1}{\lambda&#95;i^2}B&#95;i(z)" class="mmpImage" src="../pub/MUSR/LibFitPofB/_MathModePlugin_dfd02951094e1cb98f48e3f6d4562f38.png" title="London-eq" />
</p>
for each layer <img alt="i" class="mmpImage" src="../pub/MUSR/LibFitPofB/_MathModePlugin_c465118a8d86d5f25bba37cc1dcb38a0.png" title="i" /> taking into account the boundary conditions<a name="FootNote1text"></a><span class='FootNoteTextLink' title='F. London, Superfluids: Macroscopic Theory of Superconductivity, Dover (1961), p. 34'><a href="#FootNote1note" class="foswikiCurrentTopicLink">(1)</a></span>
for each layer <img alt="i" class="mmpImage" src="../pub/MUSR/LibFitPofB/_MathModePlugin_c465118a8d86d5f25bba37cc1dcb38a0.png" title="i" /> taking into account the boundary conditions<a name="FootNote1text"></a><span class="FootNoteTextLink" title="F&#46; London&#44; Superfluids&#58; Macroscopic Theory of Superconductivity&#44; Dover &#40;1961&#41;&#44; p&#46; 34"><a class="foswikiCurrentTopicLink" href="#FootNote1note">(1)</a></span>
<p style="text-align:center">
<img alt="B&#95;1(0) &#61; B&#95;N(d) &#61; \mu&#95;0H" class="mmpImage" src="../pub/MUSR/LibFitPofB/_MathModePlugin_432d7664e0756ded77e7423dd256c122.png" title="cond1" />
</p>
@ -182,19 +189,19 @@ userFcn libFitPofB TLondon1DHS 1 2 3 4 5
</dd></dl>
The parameters are: <ol>
<li> phase (deg)
</li> <li> muon implantation energy as specified in the <a href="#XmlFile" class="foswikiCurrentTopicLink">XML startup file</a> (keV)
</li> <li> muon implantation energy as specified in the <a class="foswikiCurrentTopicLink" href="#XmlFile">XML startup file</a> (keV)
</li> <li> applied field (G)
</li> <li> thickness of the dead layer (nm)
</li> <li> magnetic field penetration depth (nm)
</li></ol>
<p></p> <dl>
<dt> Superconducting thin film (one layer) </dt><dd> <pre>
userFcn libFitPofB TLondon1D1L 1 2 3 4 5 6 &#91;a b]
userFcn libFitPofB TLondon1D1L 1 2 3 4 5 6 &#91;a b&#93;
</pre>
</dd></dl>
The mandatory parameters are: <ol>
<li> phase (deg)
</li> <li> muon implantation energy as specified in the <a href="#XmlFile" class="foswikiCurrentTopicLink">XML startup file</a> (keV)
</li> <li> muon implantation energy as specified in the <a class="foswikiCurrentTopicLink" href="#XmlFile">XML startup file</a> (keV)
</li> <li> applied field (G)
</li> <li> thickness of the dead layer (nm)
</li> <li> thickness of the actually superconducting layer (nm)
@ -202,17 +209,17 @@ The mandatory parameters are: <ol>
</li></ol>
<p></p>
The optional parameters are: <ol>
<li type="a"> fraction <i>f</i><sub>1</sub> of muons in the thin film contributing to the signal (0 &le; <i>f</i><sub>1</sub> &le; 1)
</li> <li type="a"> fraction <i>f</i><sub>s</sub> of muons in the substrate contributing to the signal (0 &le; <i>f</i><sub>s</sub> &le; 1)
<li style="list-style-type:lower-alpha"> fraction <i>f</i><sub>1</sub> of muons in the thin film contributing to the signal (0 &le; <i>f</i><sub>1</sub> &le; 1)
</li> <li style="list-style-type:lower-alpha"> fraction <i>f</i><sub>s</sub> of muons in the substrate contributing to the signal (0 &le; <i>f</i><sub>s</sub> &le; 1)
</li></ol>
<p></p> <dl>
<dt> Superconducting thin-film bilayer heterostructure </dt><dd> <pre>
userFcn libFitPofB TLondon1D2L 1 2 3 4 5 6 7 8 &#91;a b c]
userFcn libFitPofB TLondon1D2L 1 2 3 4 5 6 7 8 &#91;a b c&#93;
</pre>
</dd></dl>
The mandatory parameters are: <ol>
<li> phase (deg)
</li> <li> muon implantation energy as specified in the <a href="#XmlFile" class="foswikiCurrentTopicLink">XML startup file</a> (keV)
</li> <li> muon implantation energy as specified in the <a class="foswikiCurrentTopicLink" href="#XmlFile">XML startup file</a> (keV)
</li> <li> applied field (G)
</li> <li> thickness of the dead layer (nm)
</li> <li> thickness of the actually superconducting first layer (nm)
@ -222,18 +229,18 @@ The mandatory parameters are: <ol>
</li></ol>
<p></p>
The optional parameters are: <ol>
<li type="a"> fraction <i>f</i><sub>1</sub> of muons in the dead and first layer contributing to the signal (0 &le; <i>f</i><sub>1</sub> &le; 1)
</li> <li type="a"> fraction <i>f</i><sub>2</sub> of muons in the second layer contributing to the signal (0 &le; <i>f</i><sub>2</sub> &le; 1)
</li> <li type="a"> fraction <i>f</i><sub>s</sub> of muons in the substrate contributing to the signal (0 &le; <i>f</i><sub>s</sub> &le; 1)
<li style="list-style-type:lower-alpha"> fraction <i>f</i><sub>1</sub> of muons in the dead and first layer contributing to the signal (0 &le; <i>f</i><sub>1</sub> &le; 1)
</li> <li style="list-style-type:lower-alpha"> fraction <i>f</i><sub>2</sub> of muons in the second layer contributing to the signal (0 &le; <i>f</i><sub>2</sub> &le; 1)
</li> <li style="list-style-type:lower-alpha"> fraction <i>f</i><sub>s</sub> of muons in the substrate contributing to the signal (0 &le; <i>f</i><sub>s</sub> &le; 1)
</li></ol>
<p></p> <dl>
<dt> Superconducting thin-film trilayer heterostructure </dt><dd> <pre>
userFcn libFitPofB TLondon1D3L 1 2 3 4 5 6 7 8 9 10 &#91;a b c d]
userFcn libFitPofB TLondon1D3L 1 2 3 4 5 6 7 8 9 10 &#91;a b c d&#93;
</pre>
</dd></dl>
The mandatory parameters are: <ol>
<li> phase (deg)
</li> <li> muon implantation energy as specified in the <a href="#XmlFile" class="foswikiCurrentTopicLink">XML startup file</a> (keV)
</li> <li> muon implantation energy as specified in the <a class="foswikiCurrentTopicLink" href="#XmlFile">XML startup file</a> (keV)
</li> <li> applied field (G)
</li> <li> thickness of the dead layer (nm)
</li> <li> thickness of the actually superconducting first layer (nm)
@ -245,39 +252,39 @@ The mandatory parameters are: <ol>
</li></ol>
<p></p>
The optional parameters are: <ol>
<li type="a"> fraction <i>f</i><sub>1</sub> of muons in the dead and first layer contributing to the signal (0 &le; <i>f</i><sub>1</sub> &le; 1)
</li> <li type="a"> fraction <i>f</i><sub>2</sub> of muons in the second layer contributing to the signal (0 &le; <i>f</i><sub>2</sub> &le; 1)
</li> <li type="a"> fraction <i>f</i><sub>3</sub> of muons in the third layer contributing to the signal (0 &le; <i>f</i><sub>3</sub> &le; 1)
</li> <li type="a"> fraction <i>f</i><sub>s</sub> of muons in the substrate contributing to the signal (0 &le; <i>f</i><sub>s</sub> &le; 1)
<li style="list-style-type:lower-alpha"> fraction <i>f</i><sub>1</sub> of muons in the dead and first layer contributing to the signal (0 &le; <i>f</i><sub>1</sub> &le; 1)
</li> <li style="list-style-type:lower-alpha"> fraction <i>f</i><sub>2</sub> of muons in the second layer contributing to the signal (0 &le; <i>f</i><sub>2</sub> &le; 1)
</li> <li style="list-style-type:lower-alpha"> fraction <i>f</i><sub>3</sub> of muons in the third layer contributing to the signal (0 &le; <i>f</i><sub>3</sub> &le; 1)
</li> <li style="list-style-type:lower-alpha"> fraction <i>f</i><sub>s</sub> of muons in the substrate contributing to the signal (0 &le; <i>f</i><sub>s</sub> &le; 1)
</li></ol>
<p></p>
<p></p>
<p></p>
Notes
<p></p>
<a name="FootNote1note"></a><span class="FootNoteLabel"><a href="#FootNote1text" class="foswikiCurrentTopicLink"> <strong>1</strong> </a></span>: <span class="FootNote">F. London, Superfluids: Macroscopic Theory of Superconductivity, Dover (1961), p. 34</span>
<a name="FootNote1note"></a><span class="FootNoteLabel"><a href="#FootNote1text"><b>1</b></a></span>: <span class="FootNote">F. London, Superfluids: Macroscopic Theory of Superconductivity, Dover (1961), p. 34</span>
<p></p>
<p></p>
<p></p>
<hr />
<p></p>
<h1><a name="A_3_Conventional_40bulk_41_SR"></a> 3 Conventional (bulk) &mu;SR </h1>
<h2><a name="A_3.1_Field_distributions_in_the_mixed_state_of_isotropic_superconductors"></a> 3.1 Field distributions in the mixed state of isotropic superconductors </h2>
<h1 id="A_3_Conventional_40bulk_41_SR"> 3 Conventional (bulk) &mu;SR </h1>
<h2 id="A_3.1_Field_distributions_in_the_mixed_state_of_isotropic_superconductors"> 3.1 Field distributions in the mixed state of isotropic superconductors </h2>
<p></p>
When investigating superconductors in the mixed state by means of conventional &mu;SR a two-dimensional flux-line lattice is probed randomly by the muons. The spatial field distributions within such an ordered lattice are modeled using the Fourier series
<p style="text-align:center">
<img alt="B(\mathbf{r}) &#61; \langle B \rangle \sum\limits&#95;{\mathbf{K}}B&#95;{\mathbf{K}}\exp(-\imath\mathbf{K}\mathbf{r})," class="mmpImage" src="../pub/MUSR/LibFitPofB/_MathModePlugin_c25933e91d56089992506f463d71de8f.png" title="spatialB" />
</p>
where <img alt="\mathbf{r}&#61;(x,y)" class="mmpImage" src="../pub/MUSR/LibFitPofB/_MathModePlugin_e47f33589d28eaa3f9baccb7a80fdbaa.png" title="r" />, <img alt="\mathbf{K}" class="mmpImage" src="../pub/MUSR/LibFitPofB/_MathModePlugin_e6688a12ee4e821abc31b4c1dd511539.png" title="K" /> are the reciprocal lattice vectors of a two-dimensional vortex lattice and the <img alt="B&#95;{\mathbf{K}}" class="mmpImage" src="../pub/MUSR/LibFitPofB/_MathModePlugin_8fa3ac8f18b7bc49eb89163d6528684c.png" title="Bk" /> are the Fourier coefficients depending on the magnetic penetration depth <img alt="\lambda" class="mmpImage" src="../pub/MUSR/LibFitPofB/_MathModePlugin_28f3ed750a4819b4256c2f9be649f594.png" title="lambda" /> and the superconducting coherence length <img alt="\xi" class="mmpImage" src="../pub/MUSR/LibFitPofB/_MathModePlugin_e8414d477977d226317c020980b7d34f.png" title="xi" />. The <img alt="B&#95;{\mathbf{K}}" class="mmpImage" src="../pub/MUSR/LibFitPofB/_MathModePlugin_8fa3ac8f18b7bc49eb89163d6528684c.png" title="Bk" /> for some specific models are as follows: <dl>
<dt> London model with Gaussian cutoff<a name="FootNote2text"></a><span class='FootNoteTextLink' title='E.H. Brandt, <a href="http://dx.doi.org/10.1007/BF00683568" target="_top">J. Low Temp. Phys. <strong>73</strong>, 355 (1988)</a>.'><a href="#FootNote2note" class="foswikiCurrentTopicLink">(2)</a></span> </dt><dd> <p style="text-align:center"><img alt="B&#95;{\mathbf{K}} &#61; \frac{\exp\left({-K^2\xi^2/2}\right)}{1 + K^2\lambda^2}" class="mmpImage" src="../pub/MUSR/LibFitPofB/_MathModePlugin_469d5d1b83125e4915e2f073d8150b12.png" title="BkLondon" /></p>
</dd> <dt> Modified London model<a name="FootNote3text"></a><span class='FootNoteTextLink' title='T.M. Riseman <em>et al.</em>, <a href="http://dx.doi.org/10.1103/PhysRevB.52.10569" target="_top">Phys. Rev. B <strong>52</strong>, 10569 (1995)</a>.'><a href="#FootNote3note" class="foswikiCurrentTopicLink">(3)</a></span> </dt><dd> <p style="text-align:center"><img alt="B&#95;{\mathbf{K}} &#61; \frac{\exp\left({-K^2\xi^2/2(1-b)}\right)}{1 + K^2\lambda^2/(1-b)}," class="mmpImage" src="../pub/MUSR/LibFitPofB/_MathModePlugin_b6719fad8e30208538b34bc94040b7a5.png" title="BkML" /></p> where <img alt="b &#61; \langle B \rangle/\mu&#95;0H&#95;{\mathrm{c}2}." class="mmpImage" src="../pub/MUSR/LibFitPofB/_MathModePlugin_039b3b38df7c6f284089c14f1efdf643.png" title="b" />
</dd> <dt> Analytical Ginzburg-Landau model<a name="FootNote4text"></a><span class='FootNoteTextLink' title='A. Yaouanc, P. Dalmas de R&eacute;otier and E.H. Brandt, <a href="http://dx.doi.org/10.1103/PhysRevB.55.11107" target="_top">Phys. Rev. B <strong>55</strong>, 11107 (1997)</a>.'><a href="#FootNote4note" class="foswikiCurrentTopicLink">(4)</a></span> </dt><dd> <p style="text-align:center"><img alt="B&#95;{\mathbf{K}} &#61; \frac{f&#95;{\infty}K&#95;1\left(\frac{\xi&#95;v}{\lambda}\sqrt{f&#95;{\infty}^2+\lambda^2K^2}\right)}{K&#95;1\left(\frac{\xi&#95;v}{\lambda}f&#95;{\infty}\right)\sqrt{f&#95;{\infty}^2+\lambda^2K^2}}," class="mmpImage" src="../pub/MUSR/LibFitPofB/_MathModePlugin_3146cb17887e3a20cc2078f103605af5.png" title="BkAGL" /></p> where <img alt="f&#95;{\infty} &#61; 1 - b^4,~\xi&#95;v &#61; \xi\left(\sqrt{2}-{3\xi}/\left({4\lambda}\right)\right)\sqrt{(1+b^4)(1-2b(1-b)^2)}" class="mmpImage" src="../pub/MUSR/LibFitPofB/_MathModePlugin_e0b0e98f9a3974249b42b6910523c8a4.png" title="f_inf_and_xi_v" /> and <img alt="K&#95;1" class="mmpImage" src="../pub/MUSR/LibFitPofB/_MathModePlugin_3cee3cc69dbe918398ec39a72a465014.png" title="K1" /> is a modified Bessel function.
<dt> London model with Gaussian cutoff<a name="FootNote2text"></a><span class="FootNoteTextLink" title="E&#46;H&#46; Brandt&#44; &#91;&#91;http&#58;&#47;&#47;dx&#46;doi&#46;org&#47;10&#46;1007&#47;BF00683568&#93;&#91;J&#46; Low Temp&#46; Phys&#46; &#42;73&#42;&#44; 355 &#40;1988&#41;&#93;&#93;&#46;"><a class="foswikiCurrentTopicLink" href="#FootNote2note">(2)</a></span> </dt><dd> <p style="text-align:center"><img alt="B&#95;{\mathbf{K}} &#61; \frac{\exp\left({-K^2\xi^2/2}\right)}{1 + K^2\lambda^2}" class="mmpImage" src="../pub/MUSR/LibFitPofB/_MathModePlugin_469d5d1b83125e4915e2f073d8150b12.png" title="BkLondon" /></p>
</dd> <dt> Modified London model<a name="FootNote3text"></a><span class="FootNoteTextLink" title="T&#46;M&#46; Riseman _et al&#46;_&#44; &#91;&#91;http&#58;&#47;&#47;dx&#46;doi&#46;org&#47;10&#46;1103&#47;PhysRevB&#46;52&#46;10569&#93;&#91;Phys&#46; Rev&#46; B &#42;52&#42;&#44; 10569 &#40;1995&#41;&#93;&#93;&#46;"><a class="foswikiCurrentTopicLink" href="#FootNote3note">(3)</a></span> </dt><dd> <p style="text-align:center"><img alt="B&#95;{\mathbf{K}} &#61; \frac{\exp\left({-K^2\xi^2/2(1-b)}\right)}{1 + K^2\lambda^2/(1-b)}," class="mmpImage" src="../pub/MUSR/LibFitPofB/_MathModePlugin_b6719fad8e30208538b34bc94040b7a5.png" title="BkML" /></p> where <img alt="b &#61; \langle B \rangle/\mu&#95;0H&#95;{\mathrm{c}2}." class="mmpImage" src="../pub/MUSR/LibFitPofB/_MathModePlugin_039b3b38df7c6f284089c14f1efdf643.png" title="b" />
</dd> <dt> Analytical Ginzburg-Landau model<a name="FootNote4text"></a><span class="FootNoteTextLink" title="A&#46; Yaouanc&#44; P&#46; Dalmas de R&#38;eacute&#59;otier and E&#46;H&#46; Brandt&#44; &#91;&#91;http&#58;&#47;&#47;dx&#46;doi&#46;org&#47;10&#46;1103&#47;PhysRevB&#46;55&#46;11107&#93;&#91;Phys&#46; Rev&#46; B &#42;55&#42;&#44; 11107 &#40;1997&#41;&#93;&#93;&#46;"><a class="foswikiCurrentTopicLink" href="#FootNote4note">(4)</a></span> </dt><dd> <p style="text-align:center"><img alt="B&#95;{\mathbf{K}} &#61; \frac{f&#95;{\infty}K&#95;1\left(\frac{\xi&#95;v}{\lambda}\sqrt{f&#95;{\infty}^2+\lambda^2K^2}\right)}{K&#95;1\left(\frac{\xi&#95;v}{\lambda}f&#95;{\infty}\right)\sqrt{f&#95;{\infty}^2+\lambda^2K^2}}," class="mmpImage" src="../pub/MUSR/LibFitPofB/_MathModePlugin_3146cb17887e3a20cc2078f103605af5.png" title="BkAGL" /></p> where <img alt="f&#95;{\infty} &#61; 1 - b^4,~\xi&#95;v &#61; \xi\left(\sqrt{2}-{3\xi}/\left({4\lambda}\right)\right)\sqrt{(1+b^4)(1-2b(1-b)^2)}" class="mmpImage" src="../pub/MUSR/LibFitPofB/_MathModePlugin_e0b0e98f9a3974249b42b6910523c8a4.png" title="f_inf_and_xi_v" /> and <img alt="K&#95;1" class="mmpImage" src="../pub/MUSR/LibFitPofB/_MathModePlugin_3cee3cc69dbe918398ec39a72a465014.png" title="K1" /> is a modified Bessel function.
</dd></dl>
Apart from the mentioned analytical models the <strong>numerical Ginzburg-Landau model</strong> <a name="FootNote5text"></a><span class='FootNoteTextLink' title='E.H. Brandt, <a href="http://dx.doi.org/10.1103/PhysRevB.68.054506" target="_top">Phys. Rev. B <strong>68</strong>, 054506 (2003)</a>.'><a href="#FootNote5note" class="foswikiCurrentTopicLink">(5)</a></span> is available. In this case <img alt="B(\mathbf{r})" class="mmpImage" src="../pub/MUSR/LibFitPofB/_MathModePlugin_373e9bf1fc97e2c6aacf93bcc090402c.png" title="BofR" /> is obtained by an iterative minimization of the free energy of the vortex lattice.
Apart from the mentioned analytical models the <strong>numerical Ginzburg-Landau model</strong> <a name="FootNote5text"></a><span class="FootNoteTextLink" title="E&#46;H&#46; Brandt&#44; &#91;&#91;http&#58;&#47;&#47;dx&#46;doi&#46;org&#47;10&#46;1103&#47;PhysRevB&#46;68&#46;054506&#93;&#91;Phys&#46; Rev&#46; B &#42;68&#42;&#44; 054506 &#40;2003&#41;&#93;&#93;&#46;"><a class="foswikiCurrentTopicLink" href="#FootNote5note">(5)</a></span> is available. In this case <img alt="B(\mathbf{r})" class="mmpImage" src="../pub/MUSR/LibFitPofB/_MathModePlugin_373e9bf1fc97e2c6aacf93bcc090402c.png" title="BofR" /> is obtained by an iterative minimization of the free energy of the vortex lattice.
<p></p>
<span class='foswikiRedFG'>Concerning the applicability (e.g. field regions) of each of the mentioned models please refer to the original publications!</span>
<p></p>
At the moment, the calculation of the field distribution has been implemented for triangular flux-line lattices. The number of grid lines in which the inter-vortex distance is divided for the calculations to be specified through the <a href="#XmlFile" class="foswikiCurrentTopicLink">XML file</a>.<br>The muon-spin depolarization functions finally are calculated using the following lines in the THEORY block of a <code>musrfit</code> msr file: <dl>
At the moment, the calculation of the field distribution has been implemented for triangular flux-line lattices. The number of grid lines in which the inter-vortex distance is divided for the calculations to be specified through the <a class="foswikiCurrentTopicLink" href="#XmlFile">XML file</a>.<br>The muon-spin depolarization functions finally are calculated using the following lines in the THEORY block of a <code>musrfit</code> msr file: <dl>
<dt> 2D triangular vortex lattice, London model with Gaussian cutoff </dt><dd> <pre>
userFcn libFitPofB TBulkTriVortexLondon 1 2 3 4
</pre>
@ -336,23 +343,23 @@ SAVE
<p></p>
Notes
<p></p>
<a name="FootNote2note"></a><span class="FootNoteLabel"><a href="#FootNote2text" class="foswikiCurrentTopicLink"> <strong>2</strong> </a></span>: <span class="FootNote">E.H. Brandt, <a href="http://dx.doi.org/10.1007/BF00683568" target="_top">J. Low Temp. Phys. <strong>73</strong>, 355 (1988)</a>.</span>
<a name="FootNote2note"></a><span class="FootNoteLabel"><a href="#FootNote2text"><b>2</b></a></span>: <span class="FootNote">E.H. Brandt, <a href="http://dx.doi.org/10.1007/BF00683568">J. Low Temp. Phys. <strong>73</strong>, 355 (1988)</a>.</span>
<p></p>
<a name="FootNote3note"></a><span class="FootNoteLabel"><a href="#FootNote3text" class="foswikiCurrentTopicLink"> <strong>3</strong> </a></span>: <span class="FootNote">T.M. Riseman <em>et al.</em>, <a href="http://dx.doi.org/10.1103/PhysRevB.52.10569" target="_top">Phys. Rev. B <strong>52</strong>, 10569 (1995)</a>.</span>
<a name="FootNote3note"></a><span class="FootNoteLabel"><a href="#FootNote3text"><b>3</b></a></span>: <span class="FootNote">T.M. Riseman <em>et al.</em>, <a href="http://dx.doi.org/10.1103/PhysRevB.52.10569">Phys. Rev. B <strong>52</strong>, 10569 (1995)</a>.</span>
<p></p>
<a name="FootNote4note"></a><span class="FootNoteLabel"><a href="#FootNote4text" class="foswikiCurrentTopicLink"> <strong>4</strong> </a></span>: <span class="FootNote">A. Yaouanc, P. Dalmas de R&eacute;otier and E.H. Brandt, <a href="http://dx.doi.org/10.1103/PhysRevB.55.11107" target="_top">Phys. Rev. B <strong>55</strong>, 11107 (1997)</a>.</span>
<a name="FootNote4note"></a><span class="FootNoteLabel"><a href="#FootNote4text"><b>4</b></a></span>: <span class="FootNote">A. Yaouanc, P. Dalmas de R&eacute;otier and E.H. Brandt, <a href="http://dx.doi.org/10.1103/PhysRevB.55.11107">Phys. Rev. B <strong>55</strong>, 11107 (1997)</a>.</span>
<p></p>
<a name="FootNote5note"></a><span class="FootNoteLabel"><a href="#FootNote5text" class="foswikiCurrentTopicLink"> <strong>5</strong> </a></span>: <span class="FootNote">E.H. Brandt, <a href="http://dx.doi.org/10.1103/PhysRevB.68.054506" target="_top">Phys. Rev. B <strong>68</strong>, 054506 (2003)</a>.</span>
<a name="FootNote5note"></a><span class="FootNoteLabel"><a href="#FootNote5text"><b>5</b></a></span>: <span class="FootNote">E.H. Brandt, <a href="http://dx.doi.org/10.1103/PhysRevB.68.054506">Phys. Rev. B <strong>68</strong>, 054506 (2003)</a>.</span>
<p></p>
<p></p>
<p></p>
<hr />
<p></p>
<a name="XmlFile"></a>
<h1><a name="A_4_The_XML_startup_file"></a> 4 The XML startup file </h1>
<span id="XmlFile"></span>
<h1 id="A_4_The_XML_startup_file"> 4 The XML startup file </h1>
<code><b>BMW_startup.xml</b></code> is a configuration file located in the working directory. In this file some settings like the time and field resolution of the calculations as well as the present muon implantation profiles for a LE-&mu;SR analysis have to be defined. The following XML tags are allowed to define settings: <dl>
<dt> &lt;debug&gt;ONE_OR_ZERO&lt;/debug&gt; </dt><dd> activate the debugging output of the settings read from the XML file by setting <strong>1</strong>, deactivate it with <strong>0</strong>
</dd> <dt> &lt;wisdom&gt;PATH_TO_FILE&lt;/wisdom&gt; </dt><dd> specify the <strong>PATH_TO_FILE</strong> to an <a href="http://fftw.org/fftw3_doc/Wisdom.html#Wisdom" target="_top">FFTW3 wisdom file</a> that should be used; if the <strong>PATH_TO_FILE</strong> is invalid, no FFTW3 wisdom will be used
</dd> <dt> &lt;wisdom&gt;PATH_TO_FILE&lt;/wisdom&gt; </dt><dd> specify the <strong>PATH_TO_FILE</strong> to an <a href="http://fftw.org/fftw3_doc/Wisdom.html#Wisdom">FFTW3 wisdom file</a> that should be used; if the <strong>PATH_TO_FILE</strong> is invalid, no FFTW3 wisdom will be used
</dd> <dt> &lt;delta_t&gt;ResT&lt;/delta_t&gt; </dt><dd> set the time resolution <strong>ResT</strong> for the calculated depolarization function in <strong>microseconds</strong>
</dd> <dt> &lt;delta_B&gt;ResB&lt;/delta_B&gt; </dt><dd> set the field resolution <strong>ResB</strong> for the calculated field distribution in <strong>Gauss</strong>
</dd> <dt> &lt;VortexLattice&gt;&lt;/VortexLattice&gt; </dt><dd> set the parameters used for the calculation of the spatial field distribution of a vortex lattice <dl>
@ -398,83 +405,29 @@ An example XML file looks as follows:
&#60;/BMW&#62;
</pre>
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<h1><a name="libZFRelaxation"></a> libZFRelaxation </h1>
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<h1 id="libZFRelaxation"> libZFRelaxation </h1>
<div class="foswikiToc" id="foswikiTOC"> <ul>
<li> <a href="LibZFRelaxation.html#libZFRelaxation"> libZFRelaxation </a>
</li> <li> <a href="LibZFRelaxation.html#A_1_Introduction"> 1 Introduction </a>
</li> <li> <a href="LibZFRelaxation.html#A_2_Isotropic_static_Gaussian_broadened_randomly_oriented_internal_fields"> 2 Isotropic static Gaussian broadened randomly oriented internal fields </a>
@ -126,8 +133,8 @@ pre {
</li> <li> <a href="LibZFRelaxation.html#A_4_Static_Gaussian_distributed_fields_with_uniaxial_anisotropy"> 4 Static Gaussian distributed fields with uniaxial anisotropy </a>
</li></ul>
</div>
<a name="IntroDuction"></a>
<h1><a name="A_1_Introduction"></a> 1 Introduction </h1>
<span id="IntroDuction"></span>
<h1 id="A_1_Introduction"> 1 Introduction </h1>
<p></p>
<code>libZFRelaxation</code> is a collection of <code>C++</code> classes using the <code><a href="MusrFit.html">musrfit</a></code> <code><a href="MusrFit.html#UserFunctions1">user-function interface</a></code> in order to facilitate the usage in conjunction with <code>musrfit</code>. The classes contained in this library implement the calculation of some additional zero-field &mu;SR relaxation functions which are not built-in into <code>musrfit</code>.
<p></p>
@ -136,9 +143,9 @@ In the following the use of the implemented functions is shortly introduced&mdas
If these classes prove useful and results obtained through them are part of scientific publications,
an acknowledgement of the use of the library is appreciated.
<p></p>
<h1><a name="A_2_Isotropic_static_Gaussian_broadened_randomly_oriented_internal_fields"></a> 2 Isotropic static Gaussian broadened randomly oriented internal fields </h1>
<h1 id="A_2_Isotropic_static_Gaussian_broadened_randomly_oriented_internal_fields"> 2 Isotropic static Gaussian broadened randomly oriented internal fields </h1>
<p></p>
E. I. Kornilov and V. Yu. Pomjakushin, Phys. Lett. A <b>153</b>, 364&#150;367 (1991), doi: <a href="http://dx.doi.org/10.1016/0375-9601(91)90959-C" target="_top">10.1016/0375-9601(91)90959-C</a>
E. I. Kornilov and V. Yu. Pomjakushin, Phys. Lett. A <b>153</b>, 364&#150;367 (1991), doi: <a href="http://dx.doi.org/10.1016/0375-9601(91)90959-C">10.1016/0375-9601(91)90959-C</a>
<p></p>
<p style="text-align:center">
<img alt="\mathcal{P}(t) &#61; \left(1-\alpha\right)\exp\left(-\frac{\sigma&#95;{\mathrm{L}}^2t^2}{2}\right)+\alpha\left(\cos\left(2\pi\nu t\right)-\frac{\sigma&#95;{\mathrm{T}}^2t}{2\pi\nu}\sin\left(2\pi\nu t\right)\right)\exp\left(-\frac{\sigma&#95;{\mathrm{T}}^2t^2}{2}\right)" class="mmpImage" src="../pub/MUSR/LibZFRelaxation/_MathModePlugin_fca91646b118061038b53ada5563c17c.png" title="ZFMagGss" />
@ -154,9 +161,9 @@ The parameters are: <ol>
</li> <li> the "longitudinal depolarization rate" &sigma;<sub>L</sub> (&mu;s<sup>-1</sup>) (= 0 in the article).
</li></ol>
<p></p>
<h1><a name="A_3_Isotropic_static_Lorentzian_broadened_randomly_oriented_internal_fields"></a> 3 Isotropic static Lorentzian broadened randomly oriented internal fields </h1>
<h1 id="A_3_Isotropic_static_Lorentzian_broadened_randomly_oriented_internal_fields"> 3 Isotropic static Lorentzian broadened randomly oriented internal fields </h1>
<p></p>
M. I. Larkin, Y. Fudamoto, I. M. Gat, A. Kinkhabwala, K. M. Kojima, G. M. Luke, J. Merrin, B. Nachumi, Y. J. Uemura, M. Azuma, T. Saito, and M. Takano, Physica B <b>289&#150;290</b>, 153&#150;156 (2000), doi: <a href="http://dx.doi.org/10.1016/S0921-4526(00)00337-9"" target="_top">10.1016/S0921-4526(00)00337-9</a>
M. I. Larkin, Y. Fudamoto, I. M. Gat, A. Kinkhabwala, K. M. Kojima, G. M. Luke, J. Merrin, B. Nachumi, Y. J. Uemura, M. Azuma, T. Saito, and M. Takano, Physica B <b>289&#150;290</b>, 153&#150;156 (2000), doi: <a href="http://dx.doi.org/10.1016/S0921-4526(00)00337-9"">10.1016/S0921-4526(00)00337-9</a>
<p></p>
<p style="text-align:center">
<img alt="\mathcal{P}(t) &#61; \left(1-\alpha\right)\exp\left(-a&#95;{\mathrm{L}}t\right) + \alpha\left(\cos\left(2\pi\nu t\right)-\frac{a&#95;{\mathrm{T}}}{2\pi\nu}\sin\left(2\pi\nu t\right)\right)\exp\left(-a&#95;{\mathrm{T}}t\right)" class="mmpImage" src="../pub/MUSR/LibZFRelaxation/_MathModePlugin_975f948b57199037b2b8bfb5e986b6a9.png" title="ZFMagExp" />
@ -172,9 +179,9 @@ The parameters are: <ol>
</li> <li> the "longitudinal depolarization rate" a<sub>L</sub> (&mu;s<sup>-1</sup>) (= 0 in the article).
</li></ol>
<p></p>
<h1><a name="A_4_Static_Gaussian_distributed_fields_with_uniaxial_anisotropy"></a> 4 Static Gaussian distributed fields with uniaxial anisotropy </h1>
<h1 id="A_4_Static_Gaussian_distributed_fields_with_uniaxial_anisotropy"> 4 Static Gaussian distributed fields with uniaxial anisotropy </h1>
<p></p>
G. Solt, Hyperfine Interactions <b>96</b>, 167&#150;175 (1995), doi: <a href="http://dx.doi.org/10.1007/BF02066280" target="_top">10.1007/BF02066280</a>
G. Solt, Hyperfine Interactions <b>96</b>, 167&#150;175 (1995), doi: <a href="http://dx.doi.org/10.1007/BF02066280">10.1007/BF02066280</a>
<p></p>
<p style="text-align:center">
<img alt="\mathcal{P}(t) &#61; \frac{1}{2}\sin^2\Theta + \left(\frac{3}{2}\cos^2\Theta-\frac{1}{2}\right)f&#95;1\left(\epsilon\right) + \sin^2\Theta f&#95;2(\epsilon, \sigma&#95;1, t) + \left(\frac{3}{2}\cos^2\Theta-\frac{1}{2}\right)f&#95;3\left(\epsilon, \sigma&#95;1, t\right)," class="mmpImage" src="../pub/MUSR/LibZFRelaxation/_MathModePlugin_4611c56f1556464dd8a6eaabbe070c05.png" title="UniaxialStatGssKT" />
@ -203,83 +210,29 @@ The parameters are: <ol>
</li> <li> &Theta; (&deg;).
</li></ol>
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<h1 id="A_61_61msr2data_61_61"> <code><b>msr2data</b></code> </h1>
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<h1><a name="A_61_61msr2data_61_61"></a> <code><b>msr2data</b></code> </h1>
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<a name="foswikiTOC"></a><div class="foswikiToc"> <ul>
<div class="foswikiToc" id="foswikiTOC"> <ul>
<li> <a href="Msr2Data.html#A_61_61msr2data_61_61"> msr2data </a>
</li> <li> <a href="Msr2Data.html#A_1_Introduction"> 1 Introduction </a>
</li> <li> <a href="Msr2Data.html#A_2_Basic_Types_of_Usage"> 2 Basic Types of Usage </a>
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<a name="IntroDuction"></a>
<h1><a name="A_1_Introduction"></a> 1 Introduction </h1>
<code>msr2data</code> (originally written by B. M. Wojek) is a program implemented in <code>C++</code>. Its purpose is to process multiple <code><a href="MusrFit.html">musrfit</a></code> msr files with the same parameters and summarize the fitting results either in a TRIUMF <strong>DB</strong> <a name="FootNote1text"></a><span class='FootNoteTextLink' title=' For an abridged description of this format see <a href="http://musr.org/xyfit/dbformat.html" target="_top">here</a>. The <strong>DB</strong> files produced by <code>msr2data</code> can be viewed for instance with <a href="http://musr.org/muview/" target="_top">&mu;View</a>, however, they are <em>not completely</em> backward-compatible to the original "db language" since the parameter names can be longer than five or six characters! In order to establish this backward compatibility (if needed) the user has to ensure the correct length of the parameter names in the msr files!'><a href="#FootNote1note" class="foswikiCurrentTopicLink">(1)</a></span> or a <strong>column ASCII</strong> file. It evolved from a script called <code>mlog2db</code> which has been written only for collecting fit results of <a href="http://lmu.web.psi.ch/lem/" target="_top">LEM</a> data stored in mlog files generated by <code>musrfit</code> and putting them together in a file with the <strong>DB</strong> format for further analysis. Therefore, any peculiarities, e.g. in supplying options to <code>msr2data</code> are owed its original purpose.
<code>msr2data</code> is <a href="http://www.gnu.org/philosophy/free-sw.html" target="_top">free software</a> and licensed under the <a href="http://www.gnu.org/licenses/old-licenses/gpl-2.0.html" target="_top">GNU GPL version 2</a> or any later version (at your option).
<span id="IntroDuction"></span>
<h1 id="A_1_Introduction"> 1 Introduction </h1>
<code>msr2data</code> (originally written by B. M. Wojek) is a program implemented in <code>C++</code>. Its purpose is to process multiple <code><a href="MusrFit.html">musrfit</a></code> msr files with the same parameters and summarize the fitting results either in a TRIUMF <strong>DB</strong> <a name="FootNote1text"></a><span class="FootNoteTextLink" title=" For an abridged description of this format see &#91;&#91;http&#58;&#47;&#47;musr&#46;org&#47;xyfit&#47;dbformat&#46;html&#93;&#91;here&#93;&#93;&#46; The &#42;DB&#42; files produced by &#61;msr2data&#61; can be viewed for instance with &#91;&#91;http&#58;&#47;&#47;musr&#46;org&#47;muview&#47;&#93;&#91;&#38;mu&#59;View&#93;&#93;&#44; however&#44; they are <em>not completely</em> backward&#45;compatible to the original &#34;db language&#34; since the parameter names can be longer than five or six characters&#33; In order to establish this backward compatibility &#40;if needed&#41; the user has to ensure the correct length of the parameter names in the msr files&#33;"><a class="foswikiCurrentTopicLink" href="#FootNote1note">(1)</a></span> or a <strong>column ASCII</strong> file. It evolved from a script called <code>mlog2db</code> which has been written only for collecting fit results of <a href="http://lmu.web.psi.ch/lem/">LEM</a> data stored in mlog files generated by <code>musrfit</code> and putting them together in a file with the <strong>DB</strong> format for further analysis. Therefore, any peculiarities, e.g. in supplying options to <code>msr2data</code> are owed its original purpose.
<code>msr2data</code> is <a href="http://www.gnu.org/philosophy/free-sw.html">free software</a> and licensed under the <a href="http://www.gnu.org/licenses/old-licenses/gpl-2.0.html">GNU GPL version 2</a> or any later version (at your option).
<p></p>
Before the usage of msr2data will be explained in greater detail first be aware of the following:
<p></p>
<strong><span class='foswikiRedFG'>If using msr2data always bear in mind <a href="#KnownLimitations" class="foswikiCurrentTopicLink">its limitations</a>!</span></strong>
<strong><span class='foswikiRedFG'>If using msr2data always bear in mind <a class="foswikiCurrentTopicLink" href="#KnownLimitations">its limitations</a>!</span></strong>
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Notes
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<a name="FootNote1note"></a><span class="FootNoteLabel"><a href="#FootNote1text" class="foswikiCurrentTopicLink"> <strong>1</strong> </a></span>: <span class="FootNote"> For an abridged description of this format see <a href="http://musr.org/xyfit/dbformat.html" target="_top">here</a>. The <strong>DB</strong> files produced by <code>msr2data</code> can be viewed for instance with <a href="http://musr.org/muview/" target="_top">&mu;View</a>, however, they are <em>not completely</em> backward-compatible to the original "db language" since the parameter names can be longer than five or six characters! In order to establish this backward compatibility (if needed) the user has to ensure the correct length of the parameter names in the msr files!</span>
<a name="FootNote1note"></a><span class="FootNoteLabel"><a href="#FootNote1text"><b>1</b></a></span>: <span class="FootNote"> For an abridged description of this format see <a href="http://musr.org/xyfit/dbformat.html">here</a>. The <strong>DB</strong> files produced by <code>msr2data</code> can be viewed for instance with <a href="http://musr.org/muview/">&mu;View</a>, however, they are <em>not completely</em> backward-compatible to the original "db language" since the parameter names can be longer than five or six characters! In order to establish this backward compatibility (if needed) the user has to ensure the correct length of the parameter names in the msr files!</span>
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<a name="BasicTypesOfUsage"></a>
<h1><a name="A_2_Basic_Types_of_Usage"></a> 2 Basic Types of Usage </h1>
Apart from numerous <a href="#OptionalParameters" class="foswikiCurrentTopicLink">optional parameters</a> that might be set or not, in principle there are four different ways of calling <code>msr2data</code>. These differ in how the list of runs which should be processed is supplied: <dl>
<span id="BasicTypesOfUsage"></span>
<h1 id="A_2_Basic_Types_of_Usage"> 2 Basic Types of Usage </h1>
Apart from numerous <a class="foswikiCurrentTopicLink" href="#OptionalParameters">optional parameters</a> that might be set or not, in principle there are four different ways of calling <code>msr2data</code>. These differ in how the list of runs which should be processed is supplied: <dl>
<dt> msr2data &lt;run&gt; &lt;extension&gt; [optional parameters] </dt><dd> A single run number.
</dd> <dt> msr2data &lt;firstRunNo&gt; &lt;lastRunNo&gt; &lt;extension&gt; [optional parameters] </dt><dd> An interval of run numbers is specified through the first and the last run number. The condition <strong>&lt;firstRunNo&gt; &lt; &lt;lastRunNo&gt;</strong> is <em>not</em> necessary.
</dd> <dt> msr2data \[&lt;run1&gt; &lt;run2&gt; ... &lt;runN&gt; \] &lt;extension&gt; [optional parameters] </dt><dd> A space separated list of run numbers can be enclosed in <strong>[</strong> and <strong>]</strong>. Every run that should be processed has to be specified explicitly by its run number.
</dd> <dt> msr2data &lt;runListFileName&gt; &lt;extension&gt; [optional parameters] </dt><dd> An ASCII file containing a list of run numbers and optional external parameters is passed to <code>msr2data</code>. For the structure of the ASCII file see <a href="#RunListStructure" class="foswikiCurrentTopicLink">below</a>.
</dd> <dt> msr2data \[ &lt;runList&gt; \] &lt;extension&gt; [optional parameters] </dt><dd> Where &lt;runList&gt; is one or a combination of the following:(i) <strong>&lt;run0&gt;, &lt;run1&gt;, &lt;run2&gt;, ... &lt;runN&gt;</strong> : run numbers, e.g. 123 124, (ii) <strong>&lt;run0&gt;-&lt;runN&gt;</strong> : a range, e.g. 123-125 -&gt; 123 124 125, (iii) <strong>&lt;run0&gt;:&lt;runN&gt;:&lt;step&gt;</strong> : a sequence, e.g. 123:127:2 -&gt; 123 125 127. &lt;step&gt; has to be a <strong>positive</strong> integer. A &lt;runList&gt; can also combine (i)-(iii), e.g. 123 128-130 133, etc.
</dd> <dt> msr2data &lt;runListFileName&gt; &lt;extension&gt; [optional parameters] </dt><dd> An ASCII file containing a list of run numbers and optional external parameters is passed to <code>msr2data</code>. For the structure of the ASCII file see <a class="foswikiCurrentTopicLink" href="#RunListStructure">below</a>.
</dd></dl>
<p></p>
All four basic types of calling <code>msr2data</code> contain the <em>mandatory</em> file-name <strong>&lt;extension&gt;</strong> passed right after the list of runs. The meaning of this <strong>&lt;extension&gt;</strong> should become clear after giving examples for all four cases:
<pre class="bash">msr2data 8472 &#95;tf&#95;h13</pre> generates the <strong>DB</strong> file <code><b>out.db</b></code> (can be changed by using <a href="#OptionalParameters" class="foswikiCurrentTopicLink">the -o option</a>) from <code><b>8472_tf_h13.msr</b></code>.
<pre class="bash">msr2data 8472 8474 &#95;tf&#95;h13</pre> generates the <strong>DB</strong> file <code><b>out.db</b></code> (can be changed by using <a href="#OptionalParameters" class="foswikiCurrentTopicLink">the -o option</a>) from <code><b>8472_tf_h13.msr</b></code>, <code><b>8473_tf_h13.msr</b></code>, and <code><b>8474_tf_h13.msr</b></code>.
<pre class="bash">msr2data &#91;8472 8470] &#95;tf&#95;h13</pre> generates the <strong>DB</strong> file <code><b>out.db</b></code> (can be changed by using <a href="#OptionalParameters" class="foswikiCurrentTopicLink">the -o option</a>) from <code><b>8472_tf_h13.msr</b></code> and <code><b>8470_tf_h13.msr</b></code>.
<pre class="bash">msr2data run.list &#95;tf&#95;h13</pre> generates the <strong>DB</strong> file <code><b>out.db</b></code> (can be changed by using <a href="#OptionalParameters" class="foswikiCurrentTopicLink">the -o option</a>) from all runs listed in the ASCII file <code><b>run.list</b></code> in the working directory. In this file it is also possible to include external parameters which should be put in the resulting <strong>DB</strong> file. The structure of the <code><b>run.list</b></code> is the following:
<a name="RunListStructure"></a>
<pre class="bash">msr2data 8472 &#95;tf&#95;h13</pre> generates the <strong>DB</strong> file <code><b>out.db</b></code> (can be changed by using <a class="foswikiCurrentTopicLink" href="#OptionalParameters">the -o option</a>) from <code><b>8472_tf_h13.msr</b></code>.
<pre class="bash">msr2data 8472 8474 &#95;tf&#95;h13</pre> generates the <strong>DB</strong> file <code><b>out.db</b></code> (can be changed by using <a class="foswikiCurrentTopicLink" href="#OptionalParameters">the -o option</a>) from <code><b>8472_tf_h13.msr</b></code>, <code><b>8473_tf_h13.msr</b></code>, and <code><b>8474_tf_h13.msr</b></code>.
<pre class="bash">msr2data &#91;8472 8470&#93; &#95;tf&#95;h13</pre> generates the <strong>DB</strong> file <code><b>out.db</b></code> (can be changed by using <a class="foswikiCurrentTopicLink" href="#OptionalParameters">the -o option</a>) from <code><b>8472_tf_h13.msr</b></code> and <code><b>8470_tf_h13.msr</b></code>.
<pre class="bash">msr2data &#91;8470:8474:2&#93; &#95;tf&#95;h13</pre> generates the <strong>DB</strong> file <code><b>out.db</b></code> (can be changed by using <a class="foswikiCurrentTopicLink" href="#OptionalParameters">the -o option</a>) from <code><b>8470_tf_h13.msr</b></code>, <code><b>8472_tf_h13.msr</b></code>, and <code><b>8474_tf_h13.msr</b></code>.
<pre class="bash">msr2data run.list &#95;tf&#95;h13</pre> generates the <strong>DB</strong> file <code><b>out.db</b></code> (can be changed by using <a class="foswikiCurrentTopicLink" href="#OptionalParameters">the -o option</a>) from all runs listed in the ASCII file <code><b>run.list</b></code> in the working directory. In this file it is also possible to include external parameters which should be put in the resulting <strong>DB</strong> file. The structure of the <code><b>run.list</b></code> is the following:
<span id="RunListStructure"></span>
<pre>
RUN VAR1 VAR2 VAR3 ...
8460 200 27.1 46.2 ...
8472 205 27.1 46.3 ...
8453 210 27.2 45.9 ...
<EFBFBD> <EFBFBD> <EFBFBD> <EFBFBD>
<EFBFBD> <EFBFBD> <EFBFBD> <EFBFBD>
<EFBFBD> <EFBFBD> <EFBFBD> <EFBFBD>
· · · ·
· · · ·
· · · ·
</pre>
<span class='foswikiRedFG'>The first not commented and not empty line determines the parameter names and labels and has to be present!</span><br/>
It is allowed to add comments (with a preceding <strong>#</strong>) or empty lines to the run-list file.
<p></p>
The following should be mentioned together with the above examples: <ul>
<li> The output files in the examples above are only newly created if they did not exist before invoking <strong>msr2data</strong>. If the files were already present the msr-file data would be appended!
</li> <li> If the files have been newly created, also the <strong>DB</strong> file header is written. If the files were present before, only the data blocks are appended. The output of the header can either be forced or completely suppressed with the <a href="#OptionalParameters" class="foswikiCurrentTopicLink">header and noheader options</a> as shall be seen later.
</li> <li> If the files have been newly created, also the <strong>DB</strong> file header is written. If the files were present before, only the data blocks are appended. The output of the header can either be forced or completely suppressed with the <a class="foswikiCurrentTopicLink" href="#OptionalParameters">header and noheader options</a> as shall be seen later.
</li></ul>
<a name="NoExtension"></a> <ul>
<span id="NoExtension"></span> <ul>
<li> <span class='foswikiRedFG'>If the <code>musrfit</code> output files do not have an &lt;extension&gt; as specified above like <code><b>8472.msr</b></code> one has to call <code>msr2data</code> like in the following example:</span> <pre class="bash">
msr2data 8472 8460 &#34;&#34;
</pre>
</li></ul>
<p></p>
<a name="OptionalParameters"></a>
<h1><a name="A_3_Optional_Parameters"></a> 3 Optional Parameters </h1>
<span id="OptionalParameters"></span>
<h1 id="A_3_Optional_Parameters"> 3 Optional Parameters </h1>
As mentioned already above there are some optional parameters which change the behavior of <code>msr2data</code> and can be passed in any order. Here is a complete list: <dl>
<dt> data </dt><dd> The output file format is changed to a simple column ASCII file (default output file name: <code><b>out.dat</b></code>).
</dd> <dt> new </dt><dd> An existing output file is deleted before new information is written to it.
</dd> <dt> header </dt><dd> Force the output of the file header&#151;even if the output file was present before.
</dd> <dt> noheader </dt><dd> The output of the file header is suppressed&#151;also if the output file is newly created.<br>If either both or none of the header options are given, <code>msr2data</code> writes the file header only to new files and it solely appends the data blocks to an existing output file assuming that the header is present already.
</dd> <dt> nosummary </dt><dd> There will be no attempt to read additional information like the temperature or the applied magnetic field from the data files even if these information were present there.
</dd> <dt> paramList &lt;param&gt; </dt><dd> option used to select the parameters which shall be exported. &lt;param&gt; is a list of parameter numbers to be exported. Allowed lists are: &lt;startNo&gt;-&lt;endNo&gt;, e.g. 1-16 will export parameters 1 to 16. Space separated numbers, e.g.: 1 3 5. A combination of both is possible, e.g. 1-16 19 31 62, and so on.
</dd> <dt> -o&lt;outputFileName&gt;, -o &lt;outputFileName&gt; </dt><dd> The processed data will be written to the file <strong>&lt;outputFileName&gt;</strong> instead of the default <code><b>out.db</b></code> or <code><b>out.dat</b></code>. If <strong>&lt;outputFileName&gt;</strong> is equal to <strong>none</strong> (case-insensitive) the parameter data are <em>not appended</em> to any output file.
</dd> <dt> fit </dt><dd> Additionally to the final data collection <code>msr2data</code> will invoke musrfit to fit the specified runs. All msr files are assumed to be present, none is newly generated!
</dd> <dt> fit-&lt;template&gt;[!] </dt><dd> Additionally to the final data collection <code>msr2data</code> will generate msr files for the runs specified in the list of runs and invoke <code>musrfit</code> for performing fits of the data. As template for the first run the file <code><b>&lt;template&gt;&lt;extension&gt;.msr</b></code> (or if not available: <code><b>&lt;template&gt;&lt;extension&gt;.mlog</b></code>) is used; the subsequent input files will be created using the msr output of the last processed runs ("chain fit"). However, if for <em>all</em> runs only the given template should be used one has to append an exclamation mark (<strong>!</strong>) to the <strong>&lt;template&gt;</strong>.
@ -212,9 +256,9 @@ msr2data 8400 8460 &#95;tf&#95;h13 -oABC.db fit-8472
</pre>
Using <code><b>8472_tf_h13.msr</b></code> as first template, <code>msr2data</code> generates subsequent msr input files <code><b>8400_tf_h13.msr</b></code> through <code><b>8460_tf_h13.msr</b></code>, calls <code>musrfit</code> to perform a fit of these files and collects the results of the fits together with the <strong>DB</strong> header in the new file <code><b>ABC.db</b></code>. Additionally, some information about external parameters like the temperature will be passed to <code><b>ABC.db</b></code> if it is present in the data files.
<pre class="bash">
msr2data &#91;8500 8505] &#95;zf fit-8472 noheader nosummary -o DEF.db
msr2data &#91;8500 8502-8504 8507&#93; &#95;zf fit-8472 noheader nosummary -o DEF.db
</pre>
Using <code><b>8472_zf.msr</b></code> as first template, <code>msr2data</code> generates subsequent msr input files <code><b>8500_zf.msr</b></code> and <code><b>8505_zf.msr</b></code>, calls <code>musrfit</code> to perform a fit of these files and collects the results of the fits in the file <code><b>DEF.db</b></code> without writing the <strong>DB</strong> file header or attempting to read additional information from the data files.
Using <code><b>8472_zf.msr</b></code> as first template, <code>msr2data</code> generates subsequent msr input files <code><b>8500_zf.msr</b></code>, <code><b>8502_zf.msr</b></code>, <code><b>8503_zf.msr</b></code>, <code><b>8504_zf.msr</b></code> and <code><b>8507_zf.msr</b></code>, calls <code>musrfit</code> to perform a fit of these files and collects the results of the fits in the file <code><b>DEF.db</b></code> without writing the <strong>DB</strong> file header or attempting to read additional information from the data files.
<pre class="bash">
msr2data 8595 8585 &#34;&#34; noheader fit-8472! -oGHI.dat data nosummary -k
</pre>
@ -227,13 +271,19 @@ Take the <strong>given</strong> msr files <code><b>8472.msr</b></code> through <
msr2data 8472 8475 &#95;tf&#95;h13 msr-8471!
</pre>
Using <code><b>8471_tf_h13.msr</b></code> as template for <em>all</em> runs, <code>msr2data</code> generates the msr input files <code><b>8472_tf_h13.msr</b></code> through <code><b>8475_tf_h13.msr</b></code>. <span class='foswikiRedFG'>No fitting will be performed and no DB or ASCII output will be generated!</span>
<pre class="bash">
msr2data &#91;8472 8475-8479&#93; &#95;tf&#95;h13 paramList 1-16 data -o bestData.dat
</pre>
Will collect the parameters 1 to 16 from the msr-files <code><b>8472_tf_h13.msr</b></code>, <code><b>8475_tf_h13.msr</b></code>, <code><b>8476_tf_h13.msr</b></code>, <code><b>8477_tf_h13.msr</b></code>, <code><b>8478_tf_h13.msr</b></code>, and <code><b>8479_tf_h13.msr</b></code> and write these parameters into a column like output file <code><b>bestData.dat</b></code>.
<p></p>
<a name="TheGlobalMode"></a>
<h1><a name="A_4_The_Global_Mode"></a> 4 The Global Mode </h1>
Apart from all the options described <a href="#OptionalParameters" class="foswikiCurrentTopicLink">above</a> there is another program option: <strong>global</strong>. This option changes the general behavior of <code>msr2data</code> in that way that instead of processing one msr file for each run it combines all specified runs in one single msr file with the possibility to define common parameters for all runs as well as run-specific parameters. When writing the obtained parameters to a DB file or a column-structured ASCII file that single msr file is read and the parameters valid for each run are extracted. The <strong>global</strong> option can be used in conjunction with any of the described <a href="#BasicTypesOfUsage" class="foswikiCurrentTopicLink">invocations</a> of <code>msr2data</code> and together with all options stated <a href="#OptionalParameters" class="foswikiCurrentTopicLink">above</a>.
<p></p>
<a name="GlobalFileGeneration"></a>
<h2><a name="A_4.1_File_Generation"></a> 4.1 File Generation </h2>
<p></p>
<span id="TheGlobalMode"></span>
<h1 id="A_4_The_Global_Mode"> 4 The Global Mode </h1>
Apart from all the options described <a class="foswikiCurrentTopicLink" href="#OptionalParameters">above</a> there is another program option: <strong>global</strong>. This option changes the general behavior of <code>msr2data</code> in that way that instead of processing one msr file for each run it combines all specified runs in one single msr file with the possibility to define common parameters for all runs as well as run-specific parameters. When writing the obtained parameters to a DB file or a column-structured ASCII file that single msr file is read and the parameters valid for each run are extracted. The <strong>global</strong> option can be used in conjunction with any of the described <a class="foswikiCurrentTopicLink" href="#BasicTypesOfUsage">invocations</a> of <code>msr2data</code> and together with all options stated <a class="foswikiCurrentTopicLink" href="#OptionalParameters">above</a>.
<p></p>
<span id="GlobalFileGeneration"></span>
<h2 id="A_4.1_File_Generation"> 4.1 File Generation </h2>
The general idea of this mode is to generate a global msr file on the basis of a working single-run msr file. For this purpose a single-run template containing information about common and run-specific parameters should be created. These parameters are identified through their parameter names: <dl>
<dt> run-specific parameters </dt><dd> these parameters are tagged with the current run number in the format <strong>%0Xu</strong>, i.e. <strong>X</strong> digits with leading zeros, at the end of the parameter name, e.g. for a 4-digit-formatted run number <strong>alpha0123</strong> if the run number was <strong>123</strong> or for a 8-digit-formatted run number <strong>alpha00123456</strong> if the run number was <strong>123456</strong>. <strong>X</strong> has to be at least 4.
</dd> <dt> common parameters </dt><dd> all parameters that are not run specific
@ -278,32 +328,32 @@ During this reorganization all the affected parameter occurrences are changed ac
<p></p>
<span class='foswikiRedFG'>Please be aware of the fact that comments in the template msr file are <em>not</em> propagated to the newly generated global msr file!</span>
<p></p>
<h2><a name="A_4.2_Parameter_Extraction"></a> 4.2 Parameter Extraction </h2>
After fitting some model to the specified data the fit parameters can be extracted from the global msr file to a <strong>DB</strong> or column-structured ASCII file&mdash;as usual this includes also parameters stored in the run data files or externally specified parameters given in a <a href="#RunListStructure" class="foswikiCurrentTopicLink">run-list file</a>.
<h2 id="A_4.2_Parameter_Extraction"> 4.2 Parameter Extraction </h2>
After fitting some model to the specified data the fit parameters can be extracted from the global msr file to a <strong>DB</strong> or column-structured ASCII file&mdash;as usual this includes also parameters stored in the run data files or externally specified parameters given in a <a class="foswikiCurrentTopicLink" href="#RunListStructure">run-list file</a>.
In order to reach this goal the global msr file has to obey certain rules: <ul>
<li> The order of the parameters has to match the one described <a href="#GlobalFileGeneration" class="foswikiCurrentTopicLink">above</a>, meaning the common parameters are listed first followed by the same number of parameters specific to each run tagged by the according run numbers at the end of the parameter names and having the same order as the specified list of runs.
<li> The order of the parameters has to match the one described <a class="foswikiCurrentTopicLink" href="#GlobalFileGeneration">above</a>, meaning the common parameters are listed first followed by the same number of parameters specific to each run tagged by the according run numbers at the end of the parameter names and having the same order as the specified list of runs.
</li> <li> The RUN blocks have to be ordered according to the list of runs to be processed.
</li></ul>
Following these rules&mdash;which is achieved most easily by generating the global msr file using <code>msr2data</code> as shown <a href="#GlobalFileGeneration" class="foswikiCurrentTopicLink">above</a>&mdash;the parameters can be extracted e.g. like <pre class="bash">
Following these rules&mdash;which is achieved most easily by generating the global msr file using <code>msr2data</code> as shown <a class="foswikiCurrentTopicLink" href="#GlobalFileGeneration">above</a>&mdash;the parameters can be extracted e.g. like <pre class="bash">
msr2data 8471 8470 &#95;example global data -o globalFit.dat
</pre>
This will read in the file <code><b>8471+global_example.msr</b></code>, extract for each run all relevant parameters from the msr file as well as from the according data files (if available) and append all of them in columns to the ASCII file <code><b>globalFit.dat</b></code>.
<p></p>
<a name="GlobalPlus"></a>
<h2><a name="A_4.3_The_Extended_Global_Mode"></a> 4.3 The Extended Global Mode </h2>
<span id="GlobalPlus"></span>
<h2 id="A_4.3_The_Extended_Global_Mode"> 4.3 The Extended Global Mode </h2>
If a new global input file is generated, it is also possible to do an automatic pre-analysis for each single run using the specified template first; afterwards the run-specific parameters of these single-run msr files are collected in the global msr file. In special cases this might be useful to obtain a better set of starting values for the parameters, however, in most cases it will not replace the "manual review" of the generated global input file. The option is activated by choosing the keyword <strong>global+</strong>. For example <pre class="bash">
msr2data 8471 8470 &#95;example global+ msr-8472
</pre>
Here, <code><b>8472_example.msr</b></code> is first used as template to generate the file <code><b>8471-OneRunFit_example.msr</b></code>, then <code>musrfit</code> is called for it, the result is used to generate <code><b>8470-OneRunFit_example.msr</b></code> and <code>musrfit</code> is called for that file. Finally, the global fit file <code><b>8471+global_example.msr</b></code> is produced&mdash;including the fit results of the OneRunFit files for the run-specific parameters.<br>
By appending an exclamation mark <strong>!</strong> to the <strong>global+</strong> option, the given template will be used for every new file generation (similar to the <strong>fit</strong> option explained <a href="#OptionalParameters" class="foswikiCurrentTopicLink">before</a>). The <strong>+[!]</strong> extension will be ignored, if no new global input file is generated.<br>
By appending an exclamation mark <strong>!</strong> to the <strong>global+</strong> option, the given template will be used for every new file generation (similar to the <strong>fit</strong> option explained <a class="foswikiCurrentTopicLink" href="#OptionalParameters">before</a>). The <strong>+[!]</strong> extension will be ignored, if no new global input file is generated.<br>
The single run msr files are not deleted at the moment. The information contained in them might be useful for some people. Of course the data can also be collected by <code>msr2data</code>. E.g. in order to produce a <strong>DB</strong> file <code><b>OneRunFits.db</b></code> one could call <pre class="bash">
msr2data 8471 8470 -OneRunFit&#95;example -o OneRunFits.db
</pre>
<p></p>
<span class='foswikiRedFG'>Please be aware that the program in this mode always generates new single-run msr files and always calls <code>musrfit</code> for them. In case there are already single-run fits present, these cannot be used in conjunction with this option. The program on purpose behaves in this way in order to ensure the file integrity and correct parameter order within these files.</span>
<p></p>
<a name="KnownLimitations"></a>
<h1><a name="A_5_Known_Limitations"></a> 5 Known Limitations </h1> <ul>
<span id="KnownLimitations"></span>
<h1 id="A_5_Known_Limitations"> 5 Known Limitations </h1> <ul>
<li> The indexing run number of the msr file has to be at the begin of every filename.
</li> <li> Within the data file name the <strong>RUN#</strong> has the format <strong>%0Xu</strong>, i.e. <strong>X</strong> digits with leading zeros, and has to be the rightmost number given in this format in the file name. <strong>X</strong> has to be at least 4. The highest treatable run number is 2<sup>32</sup>-1 = 4294967295.
</li> <li> In order to keep <code>msr2data</code> working properly the msr files should only contain <em><span class='foswikiRedFG'>one</span> STATISTIC block at the end of the file</em> and <i><span class='foswikiRedFG'>one</span> FITPARAMETER block right after the TITLE</i>&mdash;<code>musrfit</code> itself allows to have more creative msr files...
@ -311,12 +361,12 @@ msr2data 8471 8470 -OneRunFit&#95;example -o OneRunFits.db
</li> <li> <code>msr2data</code> will write only up to <em>two successive</em> empty lines in newly generated msr files. In case more subsequent empty lines are encountered in a template file, these are <em>not</em> copied! Actually, this measure is not a limitation but has been introduced to keep the msr files in a reasonable shape.
</li></ul>
<p></p>
<a name="MusrGuiInterface"></a>
<h1><a name="A_6_The_Graphical_User_Interface_Provided_by_61_61musrgui_61_61_47_61_61musredit_61_61"></a> 6 The Graphical User Interface Provided by <code><b>musrgui</b></code> / <code><b>musredit</b></code> </h1>
<span id="MusrGuiInterface"></span>
<h1 id="A_6_The_Graphical_User_Interface_Provided_by_61_61musrgui_61_61_47_61_61musredit_61_61"> 6 The Graphical User Interface Provided by <code><b>musrgui</b></code> / <code><b>musredit</b></code> </h1>
<code><a href="MusrGui.html">musrgui/musredit</a></code>, editors designed especially for the manipulation of <code>musrfit</code> msr files and graphical front ends to <code><a href="MusrFit.html">musrfit</a></code>, offer an almost self-explanatory graphical user interface to <code>msr2data</code> depicted below:<br>
<img src="../pub/MUSR/Msr2Data/msr2data-input-tabs.png" alt="msr2data-input-tabs.png" width='612' height='605' align="right" /> <dl>
<dt> <span class='foswikiRedFG'>1&ndash;3</span> </dt><dd> Choose one of the <a href="#BasicTypesOfUsage" class="foswikiCurrentTopicLink">ways</a> to specify your list of runs.
</dd> <dt> <span class='foswikiRedFG'>4</span> </dt><dd> Give the file extension here, e.g. <strong>_zf</strong> for files like <code><b>8472_zf.msr</b></code>. If the files do not have an extension this field stays empty. <code>musrgui</code> / <code>musredit</code> take care of passing the <strong>""</strong> to <code>msr2data</code> as mentioned <a href="#NoExtension" class="foswikiCurrentTopicLink">above</a>.
<img class='imagePlain imagePlain_right ' src='../pub/MUSR/Msr2Data/igp_589e1dc22ab7bf8fd9d5889da6e407f1_msr2data-input-tabs.png' alt='msr2data-input-tabs.png' title='msr2data-input-tabs.png' width='612' height='605' style='' /> <dl>
<dt> <span class='foswikiRedFG'>1&ndash;3</span> </dt><dd> Choose one of the <a class="foswikiCurrentTopicLink" href="#BasicTypesOfUsage">ways</a> to specify your list of runs.
</dd> <dt> <span class='foswikiRedFG'>4</span> </dt><dd> Give the file extension here, e.g. <strong>_zf</strong> for files like <code><b>8472_zf.msr</b></code>. If the files do not have an extension this field stays empty. <code>musrgui</code> / <code>musredit</code> take care of passing the <strong>""</strong> to <code>msr2data</code> as mentioned <a class="foswikiCurrentTopicLink" href="#NoExtension">above</a>.
</dd> <dt> <span class='foswikiRedFG'>5</span> </dt><dd> Activates the <strong>fit-&lt;template&gt;</strong> option if <strong>&lt;template&gt;</strong> is entered. In case the option "Chain Fit" is <em>not</em> set the given template will be used for the input-file generation for <em>all</em> runs to be fitted&mdash;otherwise the output of the first fit serves as template for the second and so on. The template field stays empty if no fits should be performed!
</dd> <dt> <span class='foswikiRedFG'>6</span> </dt><dd> Activates the <strong>-o&lt;outputFileName&gt;</strong> option if <strong>&lt;outputFileName&gt;</strong> is entered. If nothing is entered the default output file <code><b>out.db</b></code> or <code><b>out.dat</b></code> is used.
</dd> <dt> <span class='foswikiRedFG'>7</span> </dt><dd> If <em>not</em> set, the <strong>noheader</strong> option is passed to <code>msr2data</code>.
@ -328,104 +378,63 @@ msr2data 8471 8470 -OneRunFit&#95;example -o OneRunFits.db
</dd> <dt> <span class='foswikiRedFG'>13</span> </dt><dd> If set, the <strong>-t</strong> option is passed to <code>msr2data</code>.
</dd> <dt> <span class='foswikiRedFG'>14</span> </dt><dd> If set, <code>msr2data</code> is called with the option <strong>msr-&lt;template&gt;</strong> (instead of <strong>fit-&lt;template&gt;</strong>) and hence is only producing the msr input files without any fitting.
</dd> <dt> <span class='foswikiRedFG'>15</span> </dt><dd> If set, <code>msr2data</code> is called with the option <strong>fit</strong>, i.e. no template will be used to generate new msr input files; only existing files are fed to <code>musrfit</code>.
</dd> <dt> <span class='foswikiRedFG'>16</span> </dt><dd> If set, <code>msr2data</code> is operating in the <a href="#TheGlobalMode" class="foswikiCurrentTopicLink">global mode</a>.
</dd> <dt> <span class='foswikiRedFG'>17</span> </dt><dd> If set, <code>msr2data</code> is operating in the <a href="#GlobalPlus" class="foswikiCurrentTopicLink">extended global mode</a>.
</dd> <dt> <span class='foswikiRedFG'>16</span> </dt><dd> If set, <code>msr2data</code> is operating in the <a class="foswikiCurrentTopicLink" href="#TheGlobalMode">global mode</a>.
</dd> <dt> <span class='foswikiRedFG'>17</span> </dt><dd> If set, <code>msr2data</code> is operating in the <a class="foswikiCurrentTopicLink" href="#GlobalPlus">extended global mode</a>.
</dd></dl>
<p></p>
<a name="BugTracking"></a>
<h1><a name="A_7_Bugtracking"></a> 7 Bugtracking </h1>
<span id="BugTracking"></span>
<h1 id="A_7_Bugtracking"> 7 Bugtracking </h1>
<p></p>
For reporting bugs or requesting new features and improvements please use the <a href="https://tracker.intranet.psi.ch/jira/browse/MUSR" target="_top">PSI Tracker</a> or send an e-mail to A. Suter.
For reporting bugs or requesting new features and improvements please use the <a href="https://bitbucket.org/muonspin/musrfit/issues?status=new&amp;status=open">Bitbucket Issues</a>, <a href="https://tracker.psi.ch/jira/browse/MUSR">PSI Tracker</a> or send an e-mail to A. Suter.
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<td class="foswikiTableCol3 foswikiLast" style="text-align:right"> 36 K </td>
<td class="foswikiTableCol4 foswikiLast"> <span class="foswikiNoBreak">20 Jul 2011 - 12:13</span> </td>
<td class="foswikiTableCol5 foswikiLast"> <a href="https://intranet.psi.ch/Main/UnknownUser">UnknownUser</a> </td>
<td class="foswikiTableCol6 foswikiLastCol foswikiLast"> graphical interface to msr2data </td>
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</div><div class="patternContent"><div class="foswikiTopic"><h1><a name="Acknowledgements_45_61_61musrfit_61_61"></a> Acknowledgements - <code><b>musrfit</b></code> </h1>
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<dt> Bastian M. Wojek </dt><dd> I am very much indebted to <a href="http://www.fsf.org/register_form?referrer=8369" target="_top">BMW</a> for his rigorous testing of <code><a href="MusrFit.html">musrfit</a></code>, his many useful suggestions, contributions, and for the largest part of the <a href="WebHome.html" class="foswikiCurrentWebHomeLink">user manual of <code>musrfit</code></a> which makes it accessible to a broader audience! Many thanks Bastian!
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<dt> Bastian M. Wojek </dt><dd> I am very much indebted to <a href="http://www.fsf.org/register_form?referrer=8369">BMW</a> for his rigorous testing of <code><a href="MusrFit.html">musrfit</a></code>, his many useful suggestions, contributions, and for the largest part of the <a class="foswikiCurrentWebHomeLink" href="WebHome.html">user manual of <code>musrfit</code></a> which makes it accessible to a broader audience! Many thanks Bastian!
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<h1 id="A_61_61musredit_47_40musrgui_41_61_61"> <code><b>musredit / (musrgui)</b></code> </h1>
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<h1><a name="A_61_61musrgui_47_musredit_61_61"></a> <code><b>musrgui / musredit</b></code> </h1>
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<a name="foswikiTOC"></a><div class="foswikiToc"> <ul>
<li> <a href="MusrGui.html#A_61_61musrgui_47_musredit_61_61"> musrgui / musredit </a>
<div class="foswikiToc" id="foswikiTOC"> <ul>
<li> <a href="MusrGui.html#A_61_61musredit_47_40musrgui_41_61_61"> musredit / (musrgui) </a>
</li> <li> <a href="MusrGui.html#A_1_Introduction"> 1 Introduction </a>
</li> <li> <a href="MusrGui.html#A_2_Available_Executables_44_Configuration_Files_and_their_Basic_Usage"> 2 Available Executables, Configuration Files and their Basic Usage </a> <ul>
<li> <a href="MusrGui.html#A_2.1_musrgui_47_musredit"> 2.1 musrgui / musredit </a>
</li> <li> <a href="MusrGui.html#A_2.2_musrgui_startup.xml_47_musredit_startup.xml"> 2.2 musrgui_startup.xml / musredit_startup.xml </a>
<li> <a href="MusrGui.html#A_2.1_musredit_47_40musrgui_41"> 2.1 musredit / (musrgui) </a>
</li> <li> <a href="MusrGui.html#A_2.2_musredit_startup.xml_47_musrgui_startup.xml"> 2.2 musredit_startup.xml / musrgui_startup.xml </a>
</li></ul>
</li> <li> <a href="MusrGui.html#A_3_61_61musrfit_61_61_Features"> 3 musrfit Features </a>
</li> <li> <a href="MusrGui.html#A_4_Editor_Features"> 4 Editor Features </a>
@ -131,15 +173,15 @@ pre {
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<h1><a name="A_1_Introduction"></a> 1 Introduction </h1>
<code>musrgui</code> and <code>musredit</code> are editors which also provide a graphical user interface to the programs contained in the <code><a href="MusrFit.html">musrfit</a></code> suite and are intended to help the user handle <code>musrfit</code> msr files. They are implemented in <code>C++</code> and use the <a href="http://qt.nokia.com/" target="_top">Qt</a> framework. Principally, <code>musrgui</code> and <code>musredit</code> are doing the same, but are based on different Qt versions. <code>musrgui</code> is based on Qt 3.x and will only be maintained on bug-fixing level since the Qt 3.x licensing is less straight forward than the Qt 4.x one. <code>musredit</code> is based on Qt 4.6 (or above) and this is the program which will be developed further.<br>
<h1 id="A_1_Introduction"> 1 Introduction </h1>
<code>musredit</code> and <code>musrgui</code> are editors which also provide a graphical user interface to the programs contained in the <code><a href="MusrFit.html">musrfit</a></code> suite and are intended to help the user handle <code>musrfit</code> msr files. They are implemented in <code>C++</code> and use the <a href="http://qt.nokia.com/">Qt</a> framework. Principally, <code>musrgui</code> and <code>musredit</code> are doing the same, but are based on different Qt versions. <code>musrgui</code> is based on Qt 3.x and will only be maintained on bug-fixing level since the Qt 3.x licensing is less straight forward than the Qt 4.x one. <code>musredit</code> is based on Qt 4.6 (or above) and this is the program which will be developed further.<br>
On this documentation page only the features related to <code>musrfit</code> are described&mdash;the basic editor functions which should be self-explanatory are not.
<strong><span class='foswikiRedFG'>Before going on using <code>musrgui</code> / <code>musredit</code> it is strongly recommended to read the <a href="MusrFit.html">manual</a> of <code>musrfit</code> first!</span></strong>
<p></p>
<h1><a name="A_2_Available_Executables_44_Configuration_Files_and_their_Basic_Usage"></a> 2 Available Executables, Configuration Files and their Basic Usage </h1>
<a name="MusrEdit"></a>
<h2><a name="A_2.1_musrgui_47_musredit"></a> 2.1 musrgui / musredit </h2>
<code>musrgui</code> / <code>musredit</code> are the editor executables. If called from within a shell they accept a few optional parameters: <dl>
<h1 id="A_2_Available_Executables_44_Configuration_Files_and_their_Basic_Usage"> 2 Available Executables, Configuration Files and their Basic Usage </h1>
<span id="MusrEdit"></span>
<h2 id="A_2.1_musredit_47_40musrgui_41"> 2.1 musredit / (musrgui) </h2>
<code>musredit</code> / <code>musrgui</code> are the editor executables. If called from within a shell they accept a few optional parameters: <dl>
<dt> &lt;msr_files&gt; </dt><dd> file names of the msr files that should be opened in separate editor tabs on startup of <code>musrgui</code> / <code>musredit</code>.
</dd> <dt> --help </dt><dd> displays a small help notice in the shell explaining the basic usage of the program
</dd> <dt> --version </dt><dd> prints the version number of <code>musrgui</code> / <code>musredit</code>
@ -147,15 +189,15 @@ On this documentation page only the features related to <code>musrfit</code> are
<p></p>
If called without any parameters an empty editor window opens.
<p></p>
<a name="MusreditStartupXml"></a>
<h2><a name="A_2.2_musrgui_startup.xml_47_musredit_startup.xml"></a> 2.2 musrgui_startup.xml / musredit_startup.xml </h2>
<code><b>musrgui_startup.xml</b></code> / <code><b>musredit_startup.xml</b></code> are configuration files located at the <code>musrgui</code> / <code>musredit</code> binary path. It is also possible to have another version of this file in the working directory which then will be used!
<span id="MusreditStartupXml"></span>
<h2 id="A_2.2_musredit_startup.xml_47_musrgui_startup.xml"> 2.2 musredit_startup.xml / musrgui_startup.xml </h2>
<code><b>musredit_startup.xml</b></code> / <code><b>musrgui_startup.xml</b></code> are configuration files located at the <code>musredit</code> / <code>musrgui</code> binary path. It is also possible to have another version of this file in the working directory which then will be used!
<p></p>
In this file the following XML tags are allowed to define settings and might proof useful for all users of <code>musrgui</code> / <code>musredit</code>: <dl>
In this file the following XML tags are allowed to define settings and might proof useful for all users of <code>musredit</code> / <code>musrgui</code>: <dl>
<dt> &lt;general&gt;&lt;/general&gt; </dt><dd> set the default paths to executables and files in this environment <dl>
<dt> &lt;exec_path&gt;PATH_TO_EXEC&lt;/exec_path&gt; </dt><dd> set the path <strong>PATH_TO_EXEC</strong> where the executables <code>musrfit</code>, <code>musrview</code>, <code>musrt0</code>, etc. can be found (inside the &lt;general&gt; environment)
</dd> <dt> &lt;default_save_path&gt;SAV_PATH&lt;/default_save_path&gt; </dt><dd> specify the path <strong>SAV_PATH</strong> where <code>musrgui</code> / <code>musredit</code> point by default when opening and saving msr files (inside the &lt;general&gt; environment)
</dd> <dt> &lt;msr_default_file_path&gt;MSR_DEF_PATH&lt;/msr_default_file_path&gt; </dt><dd> set the path <strong>MSR_DEF_PATH</strong> where the <a href="#MusrfitFeatures" class="foswikiCurrentTopicLink">default msr files provided by</a> <code>musrgui</code> are stored (inside the &lt;general&gt; environment)
</dd> <dt> &lt;msr_default_file_path&gt;MSR_DEF_PATH&lt;/msr_default_file_path&gt; </dt><dd> set the path <strong>MSR_DEF_PATH</strong> where the <a class="foswikiCurrentTopicLink" href="#MusrfitFeatures">default msr files provided by</a> <code>musrgui</code> are stored (inside the &lt;general&gt; environment)
</dd> <dt> &lt;title_from_data_file&gt;y/n&lt;/title_from_data_file&gt; </dt><dd> specify if <code>musrfit</code> should be called with the <a href="MusrFit.html#MusrFit">-t option</a> by default (inside the &lt;general&gt; environment)
</dd> <dt> &lt;enable_musrt0&gt;y/n&lt;/enable_musrt0&gt; </dt><dd> specify if <code><a href="MusrFit.html#MusrT0">musrt0</a></code> can be called from within <code>musrgui</code> / <code>musredit</code> (inside the &lt;general&gt; environment)
</dd></dl>
@ -264,143 +306,94 @@ An example of the <code><b>musrgui_startup.xml</b></code> looks like:
&#60;/musrgui&#95;startup&#62;
</pre>
<p></p>
<a name="MusrfitFeatures"></a>
<h1><a name="A_3_61_61musrfit_61_61_Features"></a> 3 <code><b>musrfit</b></code> Features </h1>
<span id="MusrfitFeatures"></span>
<h1 id="A_3_61_61musrfit_61_61_Features"> 3 <code><b>musrfit</b></code> Features </h1>
The features of <code>musrfit</code> which can be accessed by the graphical front ends <code>musrgui</code> / <code>musredit</code> are described in the following. All functions can either be called by choosing them from the MusrFit menu, by clicking the respective button in the MusrFit bar, or by using a keyboard shortcut.
<p></p> <dl>
<dt> <img alt="musrasym.png" src="../pub/MUSR/MusrGui/musrasym.png" /> Asymmetry Default (Alt+a) </dt><dd> Generate a full msr file suitable for the <a href="MusrFit.html#FitTypes">fit type</a> <strong>2</strong> of <code>musrfit</code> from defaults. Calling this function opens a window where the relative path and file name to a data file as well as the file format that should be used have to be specified. For instance if the data file <code><b>/path-to-datadir/2007/lem07_his_8472.root</b></code> should be used and <code><b>/path-to-datadir</b></code> is on the path where <code>musrfit</code> <a href="MusrFit.html#PathToDataFiles">looks for data files</a> then the file name would be <code><b>2007/lem07_his_8472</b></code> and the file format either <strong>ROOT-NPP</strong> or <strong>ROOT-PPC</strong>.
</dd></dl>
<p></p> <dl>
<dt> <img alt="musrsinglehisto.png" src="../pub/MUSR/MusrGui/musrsinglehisto.png" /> Single-Histogram Default (Alt+h) </dt><dd> Generate a full msr file suitable for the <a href="MusrFit.html#FitTypes">fit type</a> <strong>0</strong> of <code>musrfit</code> from defaults. Calling this function opens a window where the relative path and file name to a data file as well as the file format that should be used have to be specified. For instance if the data file <code><b>/path-to-datadir/d2007/deltat_pta_gps_8472.bin</b></code> should be used and <code><b>/path-to-datadir</b></code> is on the path where <code>musrfit</code> <a href="MusrFit.html#PathToDataFiles">looks for data files</a> then the file name would be <code><b>d2007/deltat_pta_gps_8472</b></code> and the file format <strong>PSI-BIN</strong>.
</dd></dl>
<p></p> <dl>
<dt> <img alt="musrcalcchisq.png" src="../pub/MUSR/MusrGui/musrcalcchisq.png" /> Calculate Chisq (Alt+c) </dt><dd> <pre class="bash">musrfit &#60;msr&#95;file&#62; --chisq-only</pre> is called for the <strong>&lt;msr_file&gt;</strong> selected in the editor. For further information refer to the <a href="MusrFit.html#MusrFit">manual</a> of <code>musrfit</code>.
</dd></dl>
<p></p> <dl>
<dt> <img alt="musrfit.png" src="../pub/MUSR/MusrGui/musrfit.png" /> Fit (Alt+f) </dt><dd> <pre class="bash">musrfit &#60;msr&#95;file&#62; &#91;optional parameters]</pre> is called for the <strong>&lt;msr_file&gt;</strong> selected in the editor. The optional parameters may be chosen under <a href="#MusrPrefs" class="foswikiCurrentTopicLink">Preferences</a>. For further information refer to the <a href="MusrFit.html#MusrFit">manual</a> of <code>musrfit</code>.
</dd></dl>
<p></p> <dl>
<dt> <img alt="musrswap.png" src="../pub/MUSR/MusrGui/musrswap.png" /> Swap Msr &#8596; Mlog (Alt+s) </dt><dd> Swap the msr and mlog files. E.g., for a file called <code><b>8472_zf.msr</b></code>, this is copied to <code><b>8472_zf.mlog</b></code> and vice versa.
</dd></dl>
<p></p> <dl>
<dt> <img alt="musrmsr2data.png" src="../pub/MUSR/MusrGui/musrmsr2data.png" /> Msr2data (Alt+m) </dt><dd> Opens a graphical interface to the <code>msr2data</code> program described in detail in its own <a href="Msr2Data.html#MusrGuiInterface">manual</a>.
</dd></dl>
<p></p> <dl>
<dt> <img alt="musrview.png" src="../pub/MUSR/MusrGui/musrview.png" /> View (Alt+v) </dt><dd> <pre class="bash">musrview &#60;msr&#95;file&#62;</pre> is called for the <strong>&lt;msr_file&gt;</strong> selected in the editor. For further information refer to the <a href="MusrFit.html#MusrView">manual</a> of <code>musrfit</code>.
</dd></dl>
<p></p> <dl>
<dt> <img alt="musrt0.png" src="../pub/MUSR/MusrGui/musrt0.png" /> T0 (Alt+t) </dt><dd> <pre class="bash">musrt0 &#60;msr&#95;file&#62;</pre> is called for the <strong>&lt;msr_file&gt;</strong> selected in the editor. For further information refer to the <a href="MusrFit.html#MusrT0">manual</a> of <code>musrfit</code>.
</dd></dl>
<p></p>
<a name="MusrPrefs"></a> <dl>
<dt> <img alt="musrprefs.png" src="../pub/MUSR/MusrGui/musrprefs.png" /> Preferences (Alt+p) </dt><dd> Opens a window in which the optional parameters that should be passed to <code>musrfit</code> can be chosen. These options are <code><b>--keep-mn2-output</b></code>, <code><b>--dump ascii</b></code>, <code><b>--dump root</b></code>, and <code><b>--title-from-data-file</b></code>. For further information refer to the <a href="MusrFit.html#MusrFit">manual</a> of <code>musrfit</code>. Additionally, the access to <code>musrt0</code> can be enabled temporarily.
</dd></dl>
<p></p> <dl>
<dt> <img alt="musrdump.png" src="../pub/MUSR/MusrGui/musrdump.png" /> Dump Header </dt><dd> Opens a file dialog which allows to select a &mu;SR data file. When this file can be read, the run header info is dumped into a dialog window. Essentially this calls <code><b>dump_header</b></code> internally.
</dd></dl>
$ <img alt="musrasym.png" src="../pub/MUSR/MusrGui/musrasym.png" /> Asymmetry Default (Alt+a): Generate a full msr file suitable for the <a href="MusrFit.html#FitTypes">fit type</a> <strong>2</strong> of <code>musrfit</code> from defaults. Calling this function opens a window where the relative path and file name to a data file as well as the file format that should be used have to be specified. For instance if the data file <code><b>/path-to-datadir/2007/lem07_his_8472.root</b></code> should be used and <code><b>/path-to-datadir</b></code> is on the path where <code>musrfit</code> <a href="MusrFit.html#PathToDataFiles">looks for data files</a> then the file name would be <code><b>2007/lem07_his_8472</b></code> and the file format either <strong>ROOT-NPP</strong> or <strong>ROOT-PPC</strong>.
<p></p>
<a name="EditorFeatures"></a>
<h1><a name="A_4_Editor_Features"></a> 4 Editor Features </h1>
$ <img alt="musrsinglehisto.png" src="../pub/MUSR/MusrGui/musrsinglehisto.png" /> Single-Histogram Default (Alt+h): Generate a full msr file suitable for the <a href="MusrFit.html#FitTypes">fit type</a> <strong>0</strong> of <code>musrfit</code> from defaults. Calling this function opens a window where the relative path and file name to a data file as well as the file format that should be used have to be specified. For instance if the data file <code><b>/path-to-datadir/d2007/deltat_pta_gps_8472.bin</b></code> should be used and <code><b>/path-to-datadir</b></code> is on the path where <code>musrfit</code> <a href="MusrFit.html#PathToDataFiles">looks for data files</a> then the file name would be <code><b>d2007/deltat_pta_gps_8472</b></code> and the file format <strong>PSI-BIN</strong>.
<p></p>
$ <img alt="musrcalcchisq.png" src="../pub/MUSR/MusrGui/musrcalcchisq.png" /> Calculate Chisq (Alt+c): <pre class="bash">musrfit &#60;msr&#95;file&#62; --chisq-only</pre> is called for the <strong>&lt;msr_file&gt;</strong> selected in the editor. For further information refer to the <a href="MusrFit.html#MusrFit">manual</a> of <code>musrfit</code>.
<p></p>
$ <img alt="musrfit.png" src="../pub/MUSR/MusrGui/musrfit.png" /> Fit (Alt+f): <pre class="bash">musrfit &#60;msr&#95;file&#62; &#91;optional parameters&#93;</pre> is called for the <strong>&lt;msr_file&gt;</strong> selected in the editor. The optional parameters may be chosen under <a class="foswikiCurrentTopicLink" href="#MusrPrefs">Preferences</a>. For further information refer to the <a href="MusrFit.html#MusrFit">manual</a> of <code>musrfit</code>.
<p></p>
$ <img alt="musrswap.png" src="../pub/MUSR/MusrGui/musrswap.png" /> Swap Msr &#8596; Mlog (Alt+s): Swap the msr and mlog files. E.g., for a file called <code><b>8472_zf.msr</b></code>, this is copied to <code><b>8472_zf.mlog</b></code> and vice versa.
<p></p>
$ <img alt="musrmsr2data.png" src="../pub/MUSR/MusrGui/musrmsr2data.png" /> Msr2data (Alt+m): Opens a graphical interface to the <code>msr2data</code> program described in detail in its own <a href="Msr2Data.html#MusrGuiInterface">manual</a>.
<p></p>
$ <img alt="musrview.png" src="../pub/MUSR/MusrGui/musrview.png" /> View (Alt+v): <pre class="bash">musrview &#60;msr&#95;file&#62;</pre> is called for the <strong>&lt;msr_file&gt;</strong> selected in the editor. For further information refer to the <a href="MusrFit.html#MusrView">manual</a> of <code>musrfit</code>.
<p></p>
$ <img alt="musrt0.png" src="../pub/MUSR/MusrGui/musrt0.png" /> T0 (Alt+t): <pre class="bash">musrt0 &#60;msr&#95;file&#62;</pre> is called for the <strong>&lt;msr_file&gt;</strong> selected in the editor. For further information refer to the <a href="MusrFit.html#MusrT0">manual</a> of <code>musrfit</code>.
<p></p>
$ <img alt="musrFT.png" src="../pub/MUSR/MusrGui/musrFT.png" /> Raw Fourier: <code>musrFT &lt;with-many-options&gt;</code> is called. For a proper documentation of it, check the <a href="MusrFit.html#MusrFT">manual</a> of <code>musrFT</code>.
<p></p>
<span id="MusrPrefs"></span>
$ <img alt="musrprefs.png" src="../pub/MUSR/MusrGui/musrprefs.png" /> Preferences (Alt+p): Opens a window in which the optional parameters that should be passed to <code>musrfit</code> can be chosen. These options are <code><b>--keep-mn2-output</b></code>, <code><b>--dump ascii</b></code>, <code><b>--dump root</b></code>, and <code><b>--title-from-data-file</b></code>. For further information refer to the <a href="MusrFit.html#MusrFit">manual</a> of <code>musrfit</code>. Additionally, the access to <code>musrt0</code> can be enabled temporarily.
<p></p>
$ <img alt="musrdump.png" src="../pub/MUSR/MusrGui/musrdump.png" /> Dump Header: Opens a file dialog which allows to select a &mu;SR data file. When this file can be read, the run header info is dumped into a dialog window. Essentially this calls <code><b>dump_header</b></code> internally.
<p></p>
<span id="EditorFeatures"></span>
<h1 id="A_4_Editor_Features"> 4 Editor Features </h1>
Besides the functions described above and which are mostly interfacing <code>musrfit/msr2data</code> the editors of <code>musrgui</code> / <code>musredit</code> offer various functions for manipulating especially <code>musrfit</code> msr files:
<img src="../pub/MUSR/MusrGui/musrgui-editor-v0.png" alt="musrgui editor features" width='415' height='566' align="right" /> <ul>
<img class='imagePlain imagePlain_right ' src='../pub/MUSR/MusrGui/igp_4e5811420d6b5b31cac70e88b8477a14_musrgui-editor-v0.png' alt='musrgui editor features' title='musrgui-editor-v0.png' width='415' height='566' style='' /> <ul>
<li> Upon right-clicking an open msr file a menu as shown to the right is displayed which offers the addition of any valid msr file block or theory function. In case a simple theory function is chosen, the function will be inserted into the THEORY block using the <a href="MusrFit.html#TheoryTable">correct syntax</a>. If one chooses to add a whole block to the file a dialog opens in which the necessary information for each block as described in the <a href="MusrFit.html#DescriptionOfTheMsrFileFormat">manual</a> of <code>musrfit</code> can be supplied. <span class='foswikiBlueFG'>This feature is available only in <code>musrgui</code>. In <code>musredit</code> the respective functions can be accessed through the <em>Edit</em> menu.</span>
</li> <li> In order to comment or uncomment lines in a msr file select the according lines and apply <strong>Edit &rarr; (Un)Comment</strong> or use the keyboard shortcut <strong>Ctrl+(Shift)+m</strong>.
</li></ul>
<p></p>
<a name="BugTracking"></a>
<h1><a name="A_5_Bugtracking"></a> 5 Bugtracking </h1>
<span id="BugTracking"></span>
<h1 id="A_5_Bugtracking"> 5 Bugtracking </h1>
<p></p>
For reporting bugs or requesting new features and improvements please use the <a href="https://tracker.intranet.psi.ch/jira/browse/MUSR" target="_top">PSI Tracker</a> or send an e-mail to A. Suter.
For reporting bugs or requesting new features and improvements please use the <a href="https://bitbucket.org/muonspin/musrfit/issues">Bitbucket Tracker</a>, <a href="https://tracker.psi.ch/jira/browse/MUSR/">PSI Tracker</a> (PSI account needed) or send an e-mail to A. Suter.
<p></p>
-- <a href="http://www.fsf.org/register_form?referrer=8369" target="_top">BMW</a> &amp; <a href="http://lmu.web.psi.ch/lem/group.html" target="_top">AS</a> </div>
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<td class="foswikiTableCol3 foswikiLast" style="text-align:right"> 37 K </td>
<td class="foswikiTableCol4 foswikiLast"> <span class="foswikiNoBreak">10 Apr 2009 - 14:53</span> </td>
<td class="foswikiTableCol5 foswikiLast"> <a href="https://intranet.psi.ch/Main/UnknownUser">UnknownUser</a> </td>
<td class="foswikiTableCol6 foswikiLastCol foswikiLast"> musrgui options available upon right clicking a open msr-file </td>
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</div><div class="patternContent"><div class="foswikiTopic"><h1><a name="Quickstart_for_61_61WKM_61_61_users"></a> Quickstart for <code><b>WKM</b></code> users </h1>
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<h2><a name="Introduction"></a> Introduction </h2>
<h2 id="Introduction"> Introduction </h2>
<p></p>
<code>musrfit</code> is a program suite for analyzing &mu;SR data. It is implemented in <code>C++/<a href="http://root.cern.ch/" target="_top">ROOT</a></code> and uses the <a href="http://www.cern.ch/minuit/" target="_top">MINUIT2</a> libraries developed at <a href="http://www.cern.ch/" target="_top">CERN</a> for fitting data.
<code>musrfit</code> is a program suite for analyzing &mu;SR data. It is implemented in <code>C++/<a href="http://root.cern.ch/">ROOT</a></code> and uses the <a href="http://www.cern.ch/minuit/">MINUIT2</a> libraries developed at <a href="http://www.cern.ch/">CERN</a> for fitting data.
Installation instructions for Linux, MS Windows, and Mac OS X can be found <a href="MusrFitSetup.html">here</a>. The full user manual is available <a href="MusrFit.html">here</a>.<br>
In principle the programs can be used in the same fashion as <code>WKM</code> (<code>wkmfit, wkmview</code>).
E.g., for fitting data as defined in the input file <code><b>8472.msr</b></code> one types:<pre>musrfit 8472.msr</pre> for plotting data and the corresponding
fit one calls:<pre>musrview 8472.msr</pre>
Additionally, there are editors called <code><a href="MusrGui.html">musrgui/musredit</a></code> available which can do everything the <code>emacs</code> plug-in for <code>WKM</code> is capable of and even more. <strong><span class='foswikiRedFG'>However, before going to use only <code>musrgui</code> / <code>musredit</code> it is strongly recommended to read at least this "Quickstart" since there are a few differences between the programs as well as new features which are partially described in the following.</span></strong>
<p></p>
<h2><a name="Differences_between_61WKM_61_and_61musrfit_61_msr_files"></a> Differences between <code>WKM</code> and <code>musrfit</code> msr files </h2>
<h2 id="Differences_between_61WKM_61_and_61musrfit_61_msr_files"> Differences between <code>WKM</code> and <code>musrfit</code> msr files </h2>
<p></p>
The msr file format of <code>WKM</code> has some weaknesses and has therefore been extended for the use with <code>musrfit</code>. Existing <code>WKM</code> files can be converted using the <a href="MusrFit.html#Msr2Msr">small utility</a> <code>msr2msr</code>. The changes are: <ul>
<li> The <code>musrfit</code> msr and mlog files contain an additional column in the FITPARAMETER block for the representation of positive uncertainties if <code>MINOS</code> was called during fitting. In that case the <strong>Step</strong> column holds the negative uncertainties. If there has not been performed an error analysis using <code>MINOS</code>, the symmetric error can be found in the <strong>Step</strong> column, whereas the <strong>Pos_Error</strong> column contains only <strong>none</strong> entries. The beginning of the FITPARAMETER block then might look like this <pre>
@ -170,7 +174,7 @@ RUN 2008/lem08&#95;his&#95;8472 MUE4 PSI ROOT-NPP (name beamline institute dat
</li> <li> The commands <strong>SET BATCH</strong> and <strong>END RETURN</strong> may be omitted in the COMMANDS block.
</li></ul>
<p></p>
<h2><a name="Selected_new_features_in_61musrfit_61"></a> Selected new features in <code>musrfit</code> </h2> <ul>
<h2 id="Selected_new_features_in_61musrfit_61"> Selected new features in <code>musrfit</code> </h2> <ul>
<li> If single-histogram fits are done, the normalization and background constants are given either "per nanosecond" or "per rebinned bin". The nanosecond normalization allows to change the binning without the need of re-doing the fit to the data.
</li> <li> The use of functions in the RUN block is now possible for the normalization parameter, e.g. for the definition of an &alpha; parameter in simultaneous single-histogram fits of two histograms.
</li> <li> Apart from the default &chi;<sup>2</sup> minimization, when doing single-histogram fits (fit type <strong>0</strong>) in <code>musrfit</code> there is also the possibility to do a log-likelihood maximization instead. For switching, just put <strong>MAX_LIKELIHOOD</strong> in the COMMANDS block.
@ -200,7 +204,7 @@ RUN 2008/lem08&#95;his&#95;8472 MUE4 PSI ROOT-NPP (name beamline institute dat
<li> <strong>gamma_mu</strong> = &gamma;<sub>&mu;</sub>/2&pi; = 0.0135538817 MHz/G
</li> <li> <strong>pi</strong> = &pi; = 3.14159265358979323846
</li></ul>
</li> <li> As theory function also the so called skewed Gaussian can be chosen. The properties of this function are summarized in <a href="http://nemu.web.psi.ch/doc/LEM_Memo/skewedGaussian/skewedGaussian.pdf" target="_top">a memo</a> <span class="foswikiIcon"><img src="../pub/System/DocumentGraphics/pdf.png" width="16" height="16" alt="pdf" /></span>. The function is called in the THEORY block as follows: <pre>
</li> <li> As theory function also the so called skewed Gaussian can be chosen. The properties of this function are summarized in <a href="http://nemu.web.psi.ch/doc/LEM_Memo/skewedGaussian/skewedGaussian.pdf">a memo</a> <span class='foswikiIcon'><img src='../pub/System/DocumentGraphics/pdf.png' width='16' height='16' alt='pdf' /></span>. The function is called in the THEORY block as follows: <pre>
skewedGss 1 2 3 4 (phase frequency rate&#95;m rate&#95;p)
</pre>
</li> <li> After fitting it is possible to keep the <code>MINUIT2</code> output including the correlation matrix of the parameters. Calling <code>musrfit</code> with the <strong>--keep-mn2-ouput</strong> or <strong>-k</strong> option will provide you an ASCII and a ROOT file with the complete output, e.g. <pre>musrfit 8472.msr --keep-mn2-ouput</pre> generates <code><b>8472-mn2.output</b></code> and <code><b>8472-mn2.root</b></code> (and of course <code><b>8472.mlog</b></code>).
@ -258,83 +262,29 @@ RUN 2008/lem08&#95;his&#95;8472 MUE4 PSI ROOT-NPP (name beamline institute dat
</pre> In the above example <code>musrfit</code> reads the data from the file <code><b>superconductor-data.db</b></code>; the <i>x</i> and <i>y</i> data are specified by the <strong>DB</strong> parameter names <code><b>range</b></code> and <code><b>field</b></code>. An alternative specification of the <i>x</i> and <i>y</i> data by the parameter number in the <strong>DB</strong> file is also possible!
</li></ul>
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</div><div class="patternContent"><div class="foswikiTopic"><h1><a name="A_61_61musrfit_61_61_Single_45Histogram_45Fit_Tutorial"></a> <code><b>musrfit</b></code> Single-Histogram-Fit Tutorial </h1>
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<div class="patternContent"><div class="foswikiTopic"> <h1 id="A_61_61musrfit_61_61_Single_45Histogram_45Fit_Tutorial"> <code><b>musrfit</b></code> Single-Histogram-Fit Tutorial </h1>
<p></p>
The &mu;SR-data-analysis process using <code>musrfit</code> is based on so-called <code>msr</code> files. These files contain all information needed for the analysis such as names of the data files, a theory function, fit and plot parameters, and so on. It is the idea of this page to explain the basic use of an <code>msr</code> file and the different programs of the <code>musrfit</code> suite using the example of a single-histogram fit to time-differential transverse-field &mu;SR data. For a complete description of all options please refer to the <a href="MusrFit.html">manual</a>.
<p></p>
The example deals with a diamagnetic sample that has been measured in an applied field of approximately 150 G in the <a href="http://lmu.web.psi.ch/facilities/gps/gps.html" target="_top">GPS spectrometer</a> at <a href="http://www.psi.ch/" target="_top">PSI</a> using the "transverse geometry". In this geometry the muon spin is rotated about 50&#176; up and the field is applied parallel to the muon momentum. Hence, the relevant positron counters (to detect the spin precession) are placed above (histogram 3), below (histogram 4) and right of (histogram 5) the sample. The run numbers start from 3110.
The example deals with a diamagnetic sample that has been measured in an applied field of approximately 150 G in the <a href="http://lmu.web.psi.ch/facilities/gps/gps.html">GPS spectrometer</a> at <a href="http://www.psi.ch/">PSI</a> using the "transverse geometry". In this geometry the muon spin is rotated about 50&#176; up and the field is applied parallel to the muon momentum. Hence, the relevant positron counters (to detect the spin precession) are placed above (histogram 3), below (histogram 4) and right of (histogram 5) the sample. The run numbers start from 3110.
<p></p>
To analyze these data (in a simple way) one starts out from the <code>msr</code> file <strong>3110_tutorial.msr</strong> provided together with the source-code distribution in the sub-directory <strong>doc/examples/</strong>. This ASCII file can be edited using any text editor. For convenience the editors <code>musredit</code>/<code>musrgui</code> are provided which offer some <code>msr</code>-file-specific functionalities and additionally serve as front ends to the underlying programs. In the following it is assumed that the file is open within <code>musredit</code>.
<p></p>
<h1><a name="A_1_The_61msr_61_file"></a> 1 The <code>msr</code> file </h1>
<h1 id="A_1_The_61msr_61_file"> 1 The <code>msr</code> file </h1>
<p></p>
The <code>msr</code> file itself is divided into different blocks&mdash;a full description of the format can be found <a href="MusrFit.html#DescriptionOfTheMsrFileFormat">here</a>.
In the file <strong>3110_tutorial.msr</strong> these blocks are successively: <ul>
@ -230,134 +269,138 @@ STATISTIC --- 2011-07-09 10:58:44
</pre> This block is the last block of a <code>msr</code> file. It contains some information on the fit: the date and time as well as the absolute and normalized values of &#967;<sup>2</sup> and the number of degrees of freedom in the fit.<br> These information only have a meaning if the fitting procedure has been executed at least once and the fit has converged!
</li></ul>
<p></p>
<h1><a name="A_2_Determine_t0_and_the_data_range_using_61musrt0_61"></a> 2 Determine <i>t</i><sub>0</sub> and the data range using <code>musrt0</code> </h1>
<h1 id="A_2_Determine_t0_and_the_data_range_using_61musrt0_61"> 2 Determine <i>t</i><sub>0</sub> and the data range using <code>musrt0</code> </h1>
Before the given model can be fitted to the data, the data ranges and time zeros of the different RUN blocks have to be set correctly. This can be achieved using <code><a href="MusrFit.html#MusrT0">musrt0</a></code>. Starting this program by selecting the <img alt="musrt0.png" src="../pub/MUSR/MusrGui/musrt0.png" /> button in <code>musredit</code> or calling from a terminal <pre>musrt0 3110&#95;tutorial.msr</pre> opens an interactive window plotting the data of the first RUN block:<br />
<img src="../pub/MUSR/TutorialSingleHisto/musrt0-1.png" alt="musrt0-1" align="center" /><br />
<img class='imagePlain imagePlain_center ' src='../pub/MUSR/TutorialSingleHisto/musrt0-1.png' alt='musrt0-1' title='musrt0-1.png' width='708' height='529' style='' /><br />
The green line (at bin 1) represents time zero, the blue lines the start (at bin 1) and end (at bin 8000) of the data range and the optional red lines give the limits of the background range (if the background shall not be determined by the fit). All lines can be either dragged to reasonable locations or set by pressing the corresponding keyboard shortcuts. In the example the time zero can be set by pressing <strong>T</strong> (which moves the green line to the bin containing the maximum number of counts), the start of the data range should be set to about five bins later by zooming into the graph around bin 250 and pressing <strong>d</strong> when the cursor is found at a suitable location:<br />
<img src="../pub/MUSR/TutorialSingleHisto/musrt0-2.png" alt="musrt0-2" width='708' height='529' align="center" /><br />
<img class='imagePlain imagePlain_center ' src='../pub/MUSR/TutorialSingleHisto/igp_9c0f9b31d4414f37be0d3d171836fe63_musrt0-2.png' alt='musrt0-2' title='musrt0-2.png' width='688' height='529' style='' /><br />
After all lines have been adjusted for the first histogram, one can go on to the second by pressing <strong>q</strong>. This procedure is repeated until all ranges have been set correctly. When finished with the last histogram the new <i>t</i><sub>0</sub> and data-range values will be written to the <code>msr</code> file.
A full description of <code>musrt0</code> can be found <a href="MusrFit.html#MusrT0">here</a>.
<p></p>
<h1><a name="A_3_Fit_the_model_to_the_data_using_61musrfit_61"></a> 3 Fit the model to the data using <code>musrfit</code> </h1>
<h1 id="A_3_Fit_the_model_to_the_data_using_61musrfit_61"> 3 Fit the model to the data using <code>musrfit</code> </h1>
Now that the basics of the <code>msr</code> file have been introduced and the necessary adjustments have been done one can proceed with fitting the specified model to the data. This is done by selecting the <img alt="musrfit.png" src="../pub/MUSR/MusrGui/musrfit.png" /> button in <code>musredit</code> or calling from a terminal <pre>musrfit 3110&#95;tutorial.msr</pre>
<p></p>
After the fitting procedure has finished the <code>msr</code> file is updated and contains the newly determined values of the fit parameters.
<p></p>
<h1><a name="A_4_View_the_data_and_the_fit_using_61musrview_61"></a> 4 View the data and the fit using <code>musrview</code> </h1>
<h1 id="A_4_View_the_data_and_the_fit_using_61musrview_61"> 4 View the data and the fit using <code>musrview</code> </h1>
The data and the corresponding fit can be visualized by choosing <img alt="musrview.png" src="../pub/MUSR/MusrGui/musrview.png" /> in <code>musredit</code> or calling from a terminal <pre>musrview 3110&#95;tutorial.msr</pre> This creates the windows according to the given PLOT blocks in the <code>msr</code> file:<br />
<img src="../pub/MUSR/TutorialSingleHisto/musrview-1.png" alt="musrview-1" align="center" /><br />
<img src="../pub/MUSR/TutorialSingleHisto/musrview-2.png" alt="musrview-2" align="center" /><br />
<img class='imagePlain imagePlain_center ' src='../pub/MUSR/TutorialSingleHisto/musrview-1.png' alt='musrview-1' title='musrview-1.png' width='808' height='629' style='' /><br />
<img class='imagePlain imagePlain_center ' src='../pub/MUSR/TutorialSingleHisto/musrview-2.png' alt='musrview-2' title='musrview-2.png' width='808' height='629' style='' /><br />
The basic features of <code>musrview</code> can be found in the Musrfit menu. They include: <ul>
<li> export the shown data and the model to an ASCII file with comma-separated values
</li> <li> presenting the difference between the shown data and the model (keyboard shortcut: <strong>d</strong>)
</li> <li> calculate and show the Fourier transform of the shown data (keyboard shortcut: <strong>f</strong>), e.g. for the asymmetry of the "Up" and "Down" detectors:<br /> <img src="../pub/MUSR/TutorialSingleHisto/musrview-3.png" alt="musrview-3" align="center" /><br />
</li> <li> calculate and show the Fourier transform of the shown data (keyboard shortcut: <strong>f</strong>), e.g. for the asymmetry of the "Up" and "Down" detectors:<br /> <img class='imagePlain imagePlain_center ' src='../pub/MUSR/TutorialSingleHisto/musrview-3.png' alt='musrview-3' title='musrview-3.png' width='808' height='629' style='' /><br />
</li></ul>
<p></p>
<h1><a name="A_5_Process_multiple_61msr_61_files_using_61msr2data_61"></a> 5 Process multiple <code>msr</code> files using <code>msr2data</code> </h1>
<h1 id="A_5_Process_multiple_61msr_61_files_using_61msr2data_61"> 5 Process multiple <code>msr</code> files using <code>msr2data</code> </h1>
This short introduction is concluded by calling attention to the program <code><a href="Msr2Data.html">msr2data</a></code>. As the name indicates the main purpose of this program is to extract the FITPARAMETER-block information from multiple <code>msr</code> files with the same structure and to summarize them in a single ASCII file (either in TRIUMF DB format or simple columns). However, as described in detail in the <code><a href="Msr2Data.html">manual</a></code>, it is not only possible to collect data from <code>msr</code> files but also to create new <code>msr</code> files from a template and to process these files using <code>musrfit</code> on the fly.<br>
Assuming the successive runs <strong>3111</strong> through <strong>3114</strong> can be analyzed using the same model introduced above for run <strong>3110</strong> (e.g. in the case one has done measurements at different temperatures) one can use the file <strong>3110_tutorial.msr</strong> as template, generate the files <strong>3111_tutorial.msr</strong> through <strong>3114_tutorial.msr</strong> with the corresponding updates in the RUN blocks, call for each one <code>musrfit</code> and finally summarize the FITPARAMETER-block information of all processed files in an ASCII output file <strong>tutorial-T-dependence.dat</strong> (simple columns). If further information on the temperature or the applied field is available in the data files these will be included as well in the resulting ASCII file.<br>
From the terminal this would be done as follows:<pre>
msr2data 3110 3114 &#95;tutorial fit-3110 -o tutorial-T-dependence.dat data
</pre>
To achieve the same in <code>musredit</code> one selects <img alt="musrmsr2data.png" src="../pub/MUSR/MusrGui/musrmsr2data.png" /> and fills the form accordingly:<br />
<img src="../pub/MUSR/TutorialSingleHisto/msr2data.png" alt="msr2data" align="center" />
<img class='imagePlain imagePlain_center ' src='../pub/MUSR/TutorialSingleHisto/msr2data.png' alt='msr2data' title='msr2data.png' width='612' height='605' style='' />
<p></p>
<h1><a name="A_6_Further_reading"></a> 6 Further reading </h1>
<h1 id="A_6_Further_reading"> 6 Further reading </h1>
This page only summarizes the very basic features and options of the programs contained in the <code>musrfit</code> suite. For a complete description please refer to the manuals of <ul>
<li> <code><a href="MusrFit.html">musrfit</a></code> (including <code><a href="MusrFit.html#MusrFit">musrfit</a></code>, <code><a href="MusrFit.html#MusrView">musrview</a></code>, <code><a href="MusrFit.html#MusrT0">musrt0</a></code> and the full description of the <a href="MusrFit.html#DescriptionOfTheMsrFileFormat"><code>msr</code>-file format</a>)
</li> <li> <code><a href="MusrGui.html">musredit</a></code>
</li> <li> <code><a href="Msr2Data.html">msr2data</a></code>.
</li></ul>
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<div class="patternInfo">This topic: MUSR<span class='foswikiSeparator'>&nbsp;&gt;&nbsp;</span>TutorialSingleHisto <br />
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<div class="patternContent"><div class="foswikiTopic"> <h1 id="Welcome_to_the_MUSR_web"> Welcome to the MUSR web </h1>
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<h2><a name="Documentation_of_the_SR_data_analysis_suite_61musrfit_61"></a> Documentation of the &#956;SR data analysis suite <code>musrfit</code> </h2> <ul>
<li> <a href="CiteMusrFit.html">How to cite <code>musrfit</code>? <img src="../pub/Main/SmiliesPluginPSI/yes.gif" alt="yes" title="yes" border="0" /> </a>
<h2 id="Documentation_of_the_SR_data_analysis_suite_61musrfit_61"> Documentation of the &#956;SR data analysis suite <code>musrfit</code> </h2> <ul>
<li> <a href="CiteMusrFit.html">How to cite <code>musrfit</code>? <img class='smily' src='../pub/Main/SmiliesPluginPSI_/yes.gif' alt='yes' title='yes' /> </a>
</li> <li> <a href="TutorialSingleHisto.html">Single-histogram-fit tutorial for <code>musrfit</code> introducing the basic features of the programs and <code>msr</code> files</a>
</li> <li> <a href="MusrFit.html">User manual of the &#956;SR data analysis software <code>musrfit</code> </a>
</li> <li> <a href="MusrFitSetup.html">Setting up <code>musrfit</code> on Different Platforms</a>
@ -126,7 +130,7 @@ pre {
</li> <li> <a href="MusrGui.html">Documentation of <code>musrgui</code>/<code>musredit</code>&mdash;editors interfacing <code>musrfit</code> </a>
</li> <li> <a href="Msr2Data.html">Documentation of <code>msr2data</code>&mdash;a program for automatically processing multiple musrfit <code>msr</code> files</a>
</li> <li> <a href="MusrFit.html#Any2Many"><code>any2many</code>&mdash;a universal &#956;SR-file-format converter</a>
</li> <li> <a href="MusrRoot.html"><code>MusrRoot</code>: an extensible open file format for &#956;SR</a> <img src="../pub/System/DocumentGraphics/new.png" width="30" height="16" alt="New" border="0" />
</li> <li> <a href="MusrRoot.html"><code>MusrRoot</code>: an extensible open file format for &#956;SR</a>
</li> <li> Documentation of user libs (user functions) <ul>
<li> <a href="BmwLibs.html">Meissner-Profiles / Vortex-Lattice related functions (BMW libs)</a>
</li> <li> Nonlocal superconductivity related Meissner screening functions (AS libs)
@ -134,83 +138,29 @@ pre {
</li> <li> <a href="MusrFitAcknowledgements.html">Acknowledgements</a>
</li></ul>
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-- <a href="http://lmu.web.psi.ch/lem/group.html" target="_top">AS</a> &amp; (<a href="http://www.fsf.org/register_form?referrer=8369" target="_top">BMW</a>) - last update Dec 18, 2014 </div>
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#---------------------------------------------------
# get compilation flags from root-config
ROOTCFLAGS = $(shell $(ROOTSYS)/bin/root-config --cflags)
#---------------------------------------------------
OS = LINUX
CXX = g++
CXXFLAGS = -O3 -Wall -Wno-trigraphs -fPIC
LOCALINCLUDE = .
ROOTINCLUDE = $(ROOTSYS)/include
INCLUDES = -I$(LOCALINCLUDE) -I$(ROOTINCLUDE)
LD = g++
LDFLAGS =
SOFLAGS = -O -shared
# the output from the root-config script:
CXXFLAGS += $(ROOTCFLAGS)
LDFLAGS +=
# some definitions: headers (used to generate *Dict* stuff), sources, objects,...
OBJS =
OBJS += TMyFunction.o TMyLibraryDict.o
SHLIB = libTMyLibrary.so
# make the shared lib:
#
all: $(SHLIB)
$(SHLIB): $(OBJS)
@echo "---> Building shared library $(SHLIB) ..."
/bin/rm -f $(SHLIB)
$(LD) $(OBJS) $(SOFLAGS) -o $(SHLIB)
@echo "done"
# clean up: remove all object file (and core files)
# semicolon needed to tell make there is no source
# for this target!
#
clean:; @rm -f $(OBJS) *Dict* core*
@echo "---> removing $(OBJS)"
#
$(OBJS): %.o: %.cpp
$(CXX) $(INCLUDES) $(CXXFLAGS) -c $<
# Generate the ROOT CINT dictionary
TMyLibraryDict.cpp: TMyFunction.h TMyLibraryLinkDef.h
@echo "Generating dictionary $@..."
rootcint -f $@ -c -p -I$(ROOTINCLUDE) $^
install: all
@echo "Installing shared lib: libTApproximation.so"
ifeq ($(OS),LINUX)
cp -pv $(SHLIB) $(ROOTSYS)/lib
cp -pv $(LOCALINCLUDE)/*.h $(ROOTSYS)/include
endif

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places the side bar at the left
depends on global settings in layout.css
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\documentclass[twoside]{article}
\usepackage[english]{babel}
\usepackage{a4}
\usepackage{amssymb}
\usepackage{graphicx}
\usepackage{fancyhdr}
\usepackage{array}
\usepackage{float}
\usepackage{hyperref}
\usepackage{xspace}
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% \setlength{\evensidemargin}{0cm}
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\def\mathbi#1{\textbf{\em #1}}
\pagestyle{fancyplain}
\addtolength{\headwidth}{0.6cm}
\fancyhead{}%
\fancyhead[RE,LO]{\bf RRF Fits}%
\fancyhead[LE,RO]{\thepage}
\cfoot{--- Andreas Suter -- \today ---}
\rfoot{\includegraphics[width=6.4cm]{PSI_Logo_wide_blau.pdf}}
\DeclareMathAlphabet{\bi}{OML}{cmm}{b}{it}
\newcommand{\mean}[1]{\langle #1 \rangle}
\newcommand{\lem}{LE-$\mu$SR\xspace}
\newcommand{\musr}{$\mu$SR\xspace}
\newcommand{\etal}{\emph{et al.\xspace}}
\newcommand{\ie}{\emph{i.e.\xspace}}
\newcommand{\eg}{\emph{e.g.\xspace}}
\newcolumntype{d}[1]{D{.}{.}{#1}}
\begin{document}
% Header info --------------------------------------------------
\thispagestyle{empty}
\noindent
\begin{tabular}{@{\hspace{-0.7cm}}l@{\hspace{6cm}}r}
\noindent\includegraphics[width=3.4cm]{PSI_Logo_narrow_blau.jpg} &
{\Huge\sf Memorandum}
\end{tabular}
%
\vskip 1cm
%
\begin{tabular}{@{\hspace{-0.5cm}}ll@{\hspace{4cm}}ll}
Datum: & \today & & \\[3ex]
Von: & Andreas Suter & An: & \\
Telefon: & +41\, (0)56\, 310\, 4238 & & \\
Raum: & WLGA / 119 & cc: & \\
e-mail: & \verb?andreas.suter@psi.ch? & & \\
\end{tabular}
%
\vskip 0.3cm
\noindent\hrulefill
\vskip 1cm
%
\section{Rotating Reference Frame Fits}
High transverse field \musr (HTF-\musr) experiments will typically lead to
rather large data sets since it is necessary to follow the high frequencies
present in the positron decay histograms. Currently the HAL-9500 instrument
at PSI \cite{HAL9500} is operated with $2\time 8$ positron detector, with a
typical number of $\sim 4\times 10^5$ histogram bins. To analyze HTF-\musr
data on rather slugish computer hardware is a challenge. In the last millennium
the people invented the rotating reference frame transformation (RRF) \cite{Riseman90}
to reduce to data sets to be handled.
Here I will shortly describe the ways how it is implemented in \textsc{Musrfit},
and why it should be avoided to be used altogether. The starting point of all
is given by the positron decay spectrum which formally takes the form
\begin{equation}\label{eq:positron_decay_spectrum}
N^{(j)}(t) = N_0^{(j)} \exp(-t / \tau_\mu) \, \left[ 1 + A^{(j)}(t) \right] + N_{\rm bkg}^{(j)},
\end{equation}
\noindent where $(j)$ is the index of the positron counter, $N_0$ gives the scale
of recorded positrons, $\tau_\mu$ is the muon lifetime, $A(t)$ the asymmetry, and $N_{\rm bkg}$
describes the background due to uncorrelated events.
The idea behind the RRF is twofolded: (i) try to extract $A(t)$, and (ii) shift the high frequency
data set $A(t)$ to lower frequencies such that the number of necessary bins needed can be
reduced (packing / rebinning), and hence the overall number of bins is much smaller.
As I will try to explain, this is not for free, and there are problems arising from
this kind of data treatment.
\subsection{Single Histogram RRF Implementation}
In a first step the asymmetry needs to be determined. This is done the following way:
\begin{enumerate}
\item Determine the background, $N_{\rm bkg}$, at times before $t_0$ ($t_0$ is the time of the muon
implantation). Hopefully the background before and after $t_0$ is equal, which is not always
the case.
\item Multiple the background corrected histogram with $\exp(+t / \tau_\mu)$, this is leading to
\end{enumerate}
\begin{equation}\label{eq:Mt}
M(t) \equiv \left[ N(t) - N_{\rm bkg} \right]\,\exp(+t / \tau_\mu) = N_0 \left[ 1 + A(t) \right].
\end{equation}
\begin{enumerate}
\setcounter{enumi}{2}
\item In order to extract $A(t)$ from $M(t)$, $N_0$ needs to be determined, which is almost the
most tricky part here. The idea is simple: since $A(t)$ is dominated by high frequency signals,
proper averaging over $M(t)$ should allow to determine $N_0$, assuming that $\langle A(t) \rangle = 0$.
Is this assumption always true? \emph{No!} For instance it is \emph{not} true if the averaging is preformed
over incomplete periodes of a single assumed signal. Another case where it will fail is if multiple signals
with too far apart frequencies is present, as \eg in the case of muonium. Said all this, let's come
back and try to determine $N_0$:
\end{enumerate}
\begin{equation}\label{eq:N0estimate}
N_0 = \sum_{k=0}^{N_{\rm avg}} w_k M(t_k),
\end{equation}
\noindent where $N_{\rm avg}$ is determined such that $N_{\rm avg} \Delta t \simeq 1 \mu$s ($\Delta t$ being the
time resolution. $1 \mu$s means averaging over many cyles). In order to get a good estimate for $N_{\rm avg}$, $N(t)$ is Fourier
transformed, and from this power spectrum the frequency with the largest amplitude is determined, $\nu_{\rm 0}$. From $\nu_0$,
$\Delta t$, the number of cycles fitting into $1 \mu$s can be determined, and from this and the time resolution $N_{\rm avg}$
can be calculated. The weight $w_k$ is given by:
\begin{equation}
w_k = \frac{\left[\Delta M(t_k)\right]^{-2}}{\sum_{j=0}^{N_{\rm avg}} \left[\Delta M(t_j)\right]^{-2}},
\end{equation}
\noindent where
\begin{equation}
\Delta M(t) = \left[ \left(\frac{\partial M}{\partial N} \Delta N\right)^2 +
\left(\frac{\partial M}{\partial N_{\rm bkg}} \Delta N_{\rm bkg}\right)^2 \right]^{1/2}
\simeq \exp(+t/\tau_\mu) \sqrt{N(t)}.
\end{equation}
\noindent The error estimate on $N_0$ is then
\begin{equation}\label{eq:N0-rrf}
\Delta N_0 = \sigma_{N_0} = \sqrt{\sum_k w_k^2 \Delta M(t_k)^2}.
\end{equation}
\noindent Having estimated $N_0$, the asymmetry can be extracted as:
\begin{equation}
A(t) = M(t) / N_0 - 1.
\end{equation}
\begin{enumerate}
\setcounter{enumi}{3}
\item Now the actual RRF transformation can take place: $A_{\rm rrf}(t) = 2 \times A(t) \cos(\omega_{\rm rrf} t + \phi_{\rm rrf})$.
The factor of 2 is introduced to conserve the asymmetry amplitude. The idea is the following: Fourier transform theory tells as that
\end{enumerate}
\begin{equation}
{\cal F}\left\{2 \times A(t) \cos(\omega_{\rm rrf} t + \phi_{\rm rrf}) \right\} =
{\cal F}\left\{A(t)\right\}(\omega-\omega_{\rm rrf}) + {\cal F}\left\{A(t)\right\}(\omega+\omega_{\rm rrf}),
\end{equation}
\noindent \ie that the Fourier spectrum of $A(t)$ is shifted down and up by $\omega - \omega_{\rm rrf}$ and $\omega + \omega_{\rm rrf}$, respectively.
In order to get rid of the high frequency part (${\cal F}\left\{A(t)\right\}(\omega+\omega_{\rm rrf})$), $A_{\rm rrf}(t)$ will be heavily over-binned,
\ie
\begin{enumerate}
\setcounter{enumi}{4}
\item Do the rrf packing: $A_{\rm rrf}(t) \rightarrow \langle A_{\rm rrf}(t) \rangle_p$. Packing itself is a filtering of data! Especially this
kind of filter is dispersive \cite{King89}, \ie that it potentially is leading to line shape distortions. For symmetric, rather narrow
lines, this is unlikely to be a problem. However, this might be quite different for complex line shapes as in the case of vortex lattices.
\end{enumerate}
\noindent The property $\langle A_{\rm rrf}(t) \rangle_p$ is what is fitted. The error on this property is estimated the following way: (i) the
unpacked error of $A(t)$ is:
\begin{equation}
\Delta A(t) \simeq \frac{\exp(+t/\tau_\mu)}{N_0}\,\left[ N(t) + \left( \frac{N(t)-N_{\rm bkg}}{N_0} \right)^2 \Delta N_0^2 \right]^{1/2},
\end{equation}
\noindent and form this the packed $A_{\rm rrf}(t)$ error can be calculated.
\subsection{Asymmetry RRF Implementation}
\begin{enumerate}
\item In order to circumvent the difficulties to estimate $N_0$ the asymmetry of the starting positron histograms is formed. For details
see \cite{musrfit_userManual15}. For this, positron detectors geometrically under $180^\circ$ are used. However, due the the spiraling
of the positron in sufficiently high magnetic fields, and the uncertainties of the $t_0$'s, the geometrical phase might \emph{not}
correspond to the positron signal phase! At $B=9$T the uncertainty in $t_0$ by one channel leads to a phase shift of
$\gamma_\mu B \Delta t \cdot (180 / \pi) = 1.7^\circ$. Fig.\ref{fig:hal-9500-t0} shows the $t_0$-region of a typical HAL-9500 spectrum.
It shows that it is very hard to get the absolut value of $t_0$ right.
\item Carry out the RRF transformation $A_{\rm rrf}(t) = 2 \times A(t) \cos(\omega_{\rm rrf} t + \phi_{\rm rrf})$.
\item Do the rrf packing.
\end{enumerate}
\begin{figure}[h]
\centering
\includegraphics[width=0.5\textwidth]{HAL-9500-t0.pdf}
\caption{The $t_0$ region of a typical HAL-9500 spectrum. The broad black hump with the green line, is the ``prompt'' peak.
It is \emph{not} straight forward how to define $t_0$.}\label{fig:hal-9500-t0}
\end{figure}
\section{Discussion}
Both RRF transformation sketched above have weak points which makes it hard to estimate systematic errors. Both methods will fail at too
low fields of $\lesssim 1$T. The only and single purpose of the RRF transformation is slughish computer power! We developed GPU based fitting
which overcomes \emph{all} this uncontrolled weaknesses and henceforth RRF could be omitted altogether. I still added it for the time being,
since strong GPU/CPU hardware is still a bit costly and therefore not affordable to everyone.
In order to give a feeling about what might go ``wrong'' with the RRF, I was running a couple of test cases. The chosen asymmetry is
\begin{equation}\label{eq:asymmetry-simulation}
A^{(j)}(t) = A_0^{(j)} \sum_{k=1}^3 f_k \exp\left[-0.5\cdot (\sigma_k t)^2 \right] \cos(\gamma_\mu B_k t + \phi^{(j)}),
\end{equation}
\noindent with values found in Tab.\ref{tab:asymmetry-parameters}. For the simulation 4 positron detector signals were generated with
$A_0^{(j)} = \left\{ 0.2554, 0.2574, 0.2576, 0.2566 \right\}$. The further ingredients were: $N_0^{(j)} = \left\{ 27.0, 25.3, 25.6, 26.9 \right\}$,
$N_{\rm bkg}^{(j)} = \left\{ 0.055, 0.060, 0.069, 0.064 \right\}$, and $ \phi^{(j)} = \left\{ 5.0, 95.0, 185.0, 275.0 \right\}$.
\begin{table}[h]
\centering
\begin{tabular}{c|c|c|c}
$k$ & $f_k$ & $\sigma_k$ & $B_k$ \\
& & ($1/\mu$s) & (T) \\ \hline\hline
1 & 0.5 & 7 & $1$ or $9$ \\
2 & 0.2 & 0.75 & $1.02$ or $9.02$ \\
3 & 0.3 & 0.25 & $1.06$ or $9.06$
\end{tabular}
\caption{Parameters used in Eq.(\ref{eq:asymmetry-simulation}).}\label{tab:asymmetry-parameters}
\end{table}
\begin{figure}[h]
\centering
\includegraphics[width=0.45\textwidth]{08011-Fourier-Averaged.pdf} \quad
\includegraphics[width=0.45\textwidth]{08011-RRF-Histo-Fourier-Averaged-Ghost.pdf} \\
\includegraphics[width=0.45\textwidth]{08011-RRF-Asym-Fourier-Averaged-Ghost.pdf}
\caption{Averaged Fourier power spectra. Top left: from single histogram fit for the 1T data set.
Top right: from single histogram RRF fit. Bottom: from asymmetry RRF fit. Both RRF
sets show ghost lines.}\label{fig:08011-Fourier}
\end{figure}
Figure.\ref{fig:08011-Fourier} shows the averaged Fourier power spectra for the simulated data sets at 1T. Both RRF transformation are
showing ghost lines, even for optimally chosen RRF rebinning. At higher fields this is less pronounced. The ghost lines have various origins
such as aliasing effects due to the RRF packing not prefectly suppressing the high frequency part of $A_{\rm rrf}(t)$, leakage of the RRF frequency
for not sufficently precise known $N_0$ (see Eq.(\ref{eq:N0-rrf})) for single histogram RRF fits, etc.
Fits of simulated data as described above (see Eq.(\ref{eq:asymmetry-simulation}), with fields 0.5, 1.0, 3.0, 5.0, 7.0, and 9.0T) show that above
about 1T the model parameters of the RRF fits are acceptable, but the error bars are typically about a factor 3 larger compared to single histogram
fits. The asymmetries of the RRF fits are ``substantially'' too small. The $\chi^2$ values are close to meaningless for the RRF fits, since they
are strongly depending on the RRF packing, time interval chosen, etc.
To summaries: RRF fits can be used for online analysis if no GPU accelerator is available, but \emph{must not} be used for any final analysis!
\bibliographystyle{amsplain}
\bibliography{rrf}
\end{document}

29
doc/memos/rrf/rrf.bib Normal file
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@ -0,0 +1,29 @@
@Article{ Riseman90,
title = {{The Rotating Reference Frame Transformation in $\mu$SR}},
author = "T. M. Riseman and J. H. Brewer",
journal = "Hyperfine Interact.",
volume = "65",
year = "1990",
pages = "1107"
}
@Misc{ HAL9500,
title = {{HAL-9500}},
author = "",
note = {{\verb!https://www.psi.ch/smus/hal-9500!}},
}
@book{ King89,
Address = {New York},
Author = {R. King and M. Ahmadi and R. Gorgui-Naguib and A. Kwabwe and M. Azimi-Sajadi},
Edition = {1st},
Publisher = {Plenum Press},
Title = {Digital Filtering in one and two Dimensions},
Year = 1989
}
@Misc{ musrfit_userManual15,
title = {{Musrfit User Guide}},
author = "",
note = {{\verb!https://intranet.psi.ch/MUSR/MusrFit#A_5.3_Asymmetry_Fit!}},
}

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@ -6,8 +6,6 @@
content: Description of musrfit framework.
$Id$
**********************************************************************************************/
/**
@ -18,18 +16,18 @@
<p>People merely intrested in the handling of the programs should check this link:
\htmlonly
<a href="http://lmu.web.psi.ch/facilities/software/musrfit/user/MUSR/MusrFit.html">musrfit user manual</a>
<a href="http://lmu.web.psi.ch/musrfit/user/MUSR/MusrFit.html">musrfit user manual</a>
\endhtmlonly
\latexonly
musrfit user manual: \texttt{http://lmu.web.psi.ch/facilities/software/musrfit/user/MUSR/MusrFit.html}
musrfit user manual: \texttt{http://lmu.web.psi.ch/musrfit/user/MUSR/MusrFit.html}
\endlatexonly
<p>People which would like to know how to install the musrfit framework, please check this link:
\htmlonly
<a href="http://lmu.web.psi.ch/facilities/software/musrfit/user/MUSR/MusrFitSetup.html">How to setup musrfit on different platforms</a>
<a href="http://lmu.web.psi.ch/musrfit/user/MUSR/MusrFitSetup.html">How to setup musrfit on different platforms</a>
\endhtmlonly
\latexonly
How to setup musrfit on different platforms: \texttt{http://lmu.web.psi.ch/facilities/software/musrfit/user/MUSR/MusrFitSetup.html}
How to setup musrfit on different platforms: \texttt{http://lmu.web.psi.ch/musrfit/user/MUSR/MusrFitSetup.html}
\endlatexonly
//****************************************************************************************************
@ -40,6 +38,7 @@ How to setup musrfit on different platforms: \texttt{http://lmu.web.psi.ch/facil
<p>The musrfit framework provies the following programs:
- \ref musrfit Carries out fits based on a msr-file.
- \ref musrview Is used show the data in a graphical representation.
- \ref musrFT Is used to show Fourier transforms of data without the need of a theory (raw data Fourier transform).
- \ref musrt0 Is used to set graphically t0's, background and data ranges off raw histogram data.
- \ref musrparam Can be used to generate ascii output files with extracted fit-parameters (from msr-files) and independent additional variables like temperature, field, ... The ascii output files can than be used to plot parameters, e.g. by gnuplot.
- \ref msr2data A program (originally written by Bastian M. Wojek). Its purpose is to process/generate multiple musrfit msr-files with the same parameters and summarize the fitting results either in a TRIUMF DB or a column ASCII file.
@ -77,26 +76,31 @@ This two points are somewhat contradictory, and currently it is not clear which
\section bugs How to report bugs
<p>Bugs, unexpected features, can be reported directly to me: \verbatim andreas.suter@psi.ch, \endverbatim or entered in the bug-tracking tool at PSI \verbatim https://tracker.intranet.psi.ch/ \endverbatim (access to within
PSI firewall required).
<p>Bugs, unexpected features, can be reported directly to me: \verbatim andreas.suter@psi.ch, \endverbatim or entered in the bug-tracking tool at bitbkucket \verbatim https://bitbucket.org/muonspin/musrfit/issues \endverbatim.
//****************************************************************************************************
\page musrfitPage
\section musrfit musrfit
<p>Here will eventually follow a more technical description of musrfit. If you looking for a user-manual like description, please check \htmlonly<a href="http://lmu.web.psi.ch/facilities/software/musrfit/user/MUSR/MusrFit.html">musrfit user manual</a>\endhtmlonly \latexonly musrfit user manual: \texttt{http://lmu.web.psi.ch/facilities/software/musrfit/user/MUSR/MusrFit.html} \endlatexonly
<p>Here will eventually follow a more technical description of musrfit. If you looking for a user-manual like description, please check \htmlonly<a href="http://lmu.web.psi.ch/musrfit/user/MUSR/MusrFit.html">musrfit user manual</a>\endhtmlonly \latexonly musrfit user manual: \texttt{http://lmu.web.psi.ch/musrfit/user/MUSR/MusrFit.html} \endlatexonly
//****************************************************************************************************
\page musrviewPage
\section musrview musrview
<p>Here will eventually follow a more technical description of musrview. If you looking for a user-manual like description, please check \htmlonly<a href="http://lmu.web.psi.ch/facilities/software/musrfit/user/MUSR/MusrFit.html">musrfit user manual</a>\endhtmlonly \latexonly musrfit user manual: \texttt{http://lmu.web.psi.ch/facilities/software/musrfit/user/MUSR/MusrFit.html} \endlatexonly
<p>Here will eventually follow a more technical description of musrview. If you looking for a user-manual like description, please check \htmlonly<a href="http://lmu.web.psi.ch/musrfit/user/MUSR/MusrFit.html">musrfit user manual</a>\endhtmlonly \latexonly musrfit user manual: \texttt{http://lmu.web.psi.ch/musrfit/user/MUSR/MusrFit.html} \endlatexonly
//****************************************************************************************************
\page musrFTPage
\section musrFT musrFT
<p>Here will eventually follow a more technical description of musrFT. If you looking for a user-manual like description, please check \htmlonly<a href="http://lmu.web.psi.ch/musrfit/user/MUSR/MusrFit.html">musrfit user manual</a>\endhtmlonly \latexonly musrfit user manual: \texttt{http://lmu.web.psi.ch/musrfit/user/MUSR/MusrFit.html} \endlatexonly
//****************************************************************************************************
\page musrt0Page
\section musrt0 musrt0
<p>Here will eventually follow a more technical description of musrt0. If you looking for a user-manual like description, please check \htmlonly<a href="http://lmu.web.psi.ch/facilities/software/musrfit/user/MUSR/MusrFit.html">musrfit user manual</a>\endhtmlonly \latexonly musrfit user manual: \texttt{http://lmu.web.psi.ch/facilities/software/musrfit/user/MUSR/MusrFit.html} \endlatexonly
<p>Here will eventually follow a more technical description of musrt0. If you looking for a user-manual like description, please check \htmlonly<a href="http://lmu.web.psi.ch/musrfit/user/MUSR/MusrFit.html">musrfit user manual</a>\endhtmlonly \latexonly musrfit user manual: \texttt{http://lmu.web.psi.ch/musrfit/user/MUSR/MusrFit.html} \endlatexonly
//****************************************************************************************************
\page musrparamPage

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@ -23,7 +23,7 @@ PROJECT_NAME = musrfit
# This could be handy for archiving the generated documentation or
# if some version control system is used.
PROJECT_NUMBER = 0.11.0
PROJECT_NUMBER = 0.14.0
# The OUTPUT_DIRECTORY tag is used to specify the (relative or absolute)
# base path where the generated documentation will be put.
@ -462,17 +462,19 @@ WARN_LOGFILE =
INPUT = musrfit.dox \
../src/include/PFitterFcn.h \
../src/include/PFitter.h \
../src/include/PFourier.h \
../src/include/PFourier.h \
../src/include/PFourierCanvas.h \
../src/include/PFunctionGrammar.h \
../src/include/PFunction.h \
../src/include/PFunctionHandler.h \
../src/include/PMsr2Data.h \
../src/include/PMsr2Data.h \
../src/include/PMsrHandler.h \
../src/include/PMusrCanvas.h \
../src/include/PMusrCanvasLinkDef.h \
../src/include/PMusr.h \
../src/include/PMusrT0.h \
../src/include/PMusrT0LinkDef.h \
../src/include/PMusrT0.h \
../src/include/PMusrT0LinkDef.h \
../src/include/PPrepFourier.h \
../src/include/PRunAsymmetry.h \
../src/include/PRunBase.h \
../src/include/PRunDataHandler.h \
@ -488,7 +490,8 @@ INPUT = musrfit.dox \
../src/include/PUserFcn.h \
../src/classes/PFitter.cpp \
../src/classes/PFitterFcn.cpp \
../src/classes/PFourier.cpp \
../src/classes/PFourier.cpp \
../src/classes/PFourierCanvas.cpp \
../src/classes/PFunction.cpp \
../src/classes/PFunctionHandler.cpp \
../src/classes/PMsr2Data.cpp \
@ -496,6 +499,7 @@ INPUT = musrfit.dox \
../src/classes/PMusrCanvas.cpp \
../src/classes/PMusr.cpp \
../src/classes/PMusrT0.cpp \
../src/classes/PPrepFourier.cpp \
../src/classes/PRunAsymmetry.cpp \
../src/classes/PRunBase.cpp \
../src/classes/PRunDataHandler.cpp \

View File

@ -16,31 +16,43 @@ if BUILD_MUSREDIT
EDITORDIR = musredit
endif
if BUILD_MUSREDIT_QT5
EDITORDIR = musredit_qt5
endif
SUBDIRS = external/MusrRoot \
external/TLemRunHeader \
external/MuSR_software \
external/mud \
$(PNEXUSDIRS) \
classes \
external
external \
musredit_qt5 \
musredit \
musrgui
if BUILD_MUSRGUI
SUBDIRS += $(EDITORDIR)
#SUBDIRS += $(EDITORDIR)
EXTRA_DIST = $(EDITORDIR)/Makefile
endif
if BUILD_MUSREDIT
SUBDIRS += $(EDITORDIR)
#SUBDIRS += $(EDITORDIR)
EXTRA_DIST = $(EDITORDIR)/Makefile
endif
bin_PROGRAMS = musrfit musrview musrt0 msr2msr msr2data any2many
if BUILD_MUSREDIT_QT5
EXTRA_DIST = $(EDITORDIR)/Makefile
endif
bin_PROGRAMS = musrfit musrview musrt0 musrFT msr2msr msr2data any2many
bin_PROGRAMS += write_musrRoot_runHeader musrRootValidation
bin_PROGRAMS += dump_header
musrfit_SOURCES = musrfit.cpp
musrview_SOURCES = musrview.cpp
musrt0_SOURCES = musrt0.cpp
musrFT_SOURCES = musrFT.cpp
msr2msr_SOURCES = msr2msr.cpp
msr2data_SOURCES = msr2data.cpp
any2many_SOURCES = any2many.cpp
@ -48,7 +60,7 @@ write_musrRoot_runHeader_SOURCES = write_musrRoot_runHeader.cpp
musrRootValidation_SOURCES = musrRootValidation.cpp
dump_header_SOURCES = dump_header.cpp
xmldir = $(bindir)
xmldir = $(HOME)/.musrfit
xml_DATA = musrfit_startup.xml
LIBADD = $(PMUSR_LIBS) $(MUSR_ROOT_LIBS) $(LEM_LIBS) $(PSIBIN_LIBS) $(MUD_LIBS) $(PNEXUS_LIBS)
@ -70,7 +82,7 @@ install-xmlDATA: $(xml_DATA)
DIFF="$$(diff "$(DESTDIR)$(xmldir)/$(xml_DATA)" "$(xml_DATA)" 2>&1)"; \
if test "x$$DIFF" != "x"; then \
echo " " && \
echo " musrfit_startup.xml in $(bindir)" && \
echo " musrfit_startup.xml in $(xmldir)" && \
echo " is different from the distribution's version." && \
echo " Do you want to overwrite it? [y/N]" && \
read OVERWRITE && \
@ -89,7 +101,7 @@ uninstall-xmlDATA:
DIFF="$$(diff "$(DESTDIR)$(xmldir)/$(xml_DATA)" "$(xml_DATA)" 2>&1)"; \
if test "x$$DIFF" != "x"; then \
echo " " && \
echo " musrfit_startup.xml in $(bindir)" && \
echo " musrfit_startup.xml in $(xmldir)" && \
echo " is different from the distribution's version." && \
echo " Do you want to remove it? [y/N]" && \
read REMOVE && \

View File

@ -54,7 +54,7 @@ using namespace std;
void any2many_syntax()
{
cout << endl << "usage: any2many [--help] : will show this help.";
cout << endl << " any2many --version : will show the svn version.";
cout << endl << " any2many --version : will show the git version.";
cout << endl << " any2many -f <filenameList-input> | -r <runList-input>";
cout << endl << " -c <convert-options> [-p <output-path>] [-y <year>]";
cout << endl << " [-o <outputFileName> | -t <in-template> <out-template>] [-s]";
@ -83,6 +83,10 @@ void any2many_syntax()
cout << endl << " NeXus2-HDF4, NeXus2-HDF5, NeXus2-XML, WKM, ASCII";
cout << endl << " Comment: ROOT is superseeded by MusrRoot. If there is not a very good";
cout << endl << " reason, avoid it!";
cout << endl << " -h <histo-group-list> : This option is for MusrRoot input files only!";
cout << endl << " Select the the histo groups to be exported. <histo-group-list> is a space";
cout << endl << " separated list of the histo group, e.g. -h 0, 20 will try to export the histo";
cout << endl << " 0 (NPP) and 20 (PPC).";
cout << endl << " -p <output-path> : where <output-path> is the output path for the";
cout << endl << " converted files. If nothing is given, the current directory";
cout << endl << " will be used, unless the option '-s' is used.";
@ -190,7 +194,7 @@ int main(int argc, char *argv[])
// call any2many --help or any2many --version
if (argc == 2) {
if (strstr(argv[1], "--h"))
if (!strncmp(argv[1], "--help", 128))
any2many_syntax();
else if (strstr(argv[1], "--v")) {
#ifdef HAVE_CONFIG_H
@ -344,6 +348,21 @@ int main(int argc, char *argv[])
show_syntax = true;
break;
}
} else if (!strcmp(argv[i], "-h")) { // filter histo group list (for MusrRoot and ROOT (LEM) only!)
bool done = false;
int j = i+1;
do {
status = sscanf(argv[j], "%d", &ival);
if (status == 1) {
info.groupHistoList.push_back(ival);
j++;
} else {
done = true;
}
} while (!done && (j<argc));
i = j-1;
if (j >= argc) // make sure that counter is still in range
break;
} else if (!strcmp(argv[i], "-p")) { // filter output path name flag
if (i+1 < argc) {
info.outPath = argv[i+1];

View File

@ -4,6 +4,7 @@ h_sources = \
../include/PFitterFcn.h \
../include/PFitter.h \
../include/PFourier.h \
../include/PFourierCanvas.h \
../include/PFunctionGrammar.h \
../include/PFunction.h \
../include/PFunctionHandler.h \
@ -12,13 +13,16 @@ h_sources = \
../include/PMusrCanvas.h \
../include/PMusr.h \
../include/PMusrT0.h \
../include/PPrepFourier.h \
../include/PRunAsymmetry.h \
../include/PRunAsymmetryRRF.h \
../include/PRunBase.h \
../include/PRunDataHandler.h \
../include/PRunListCollection.h \
../include/PRunNonMusr.h \
../include/PRunMuMinus.h \
../include/PRunSingleHisto.h \
../include/PRunSingleHistoRRF.h \
../include/PStartupHandler.h \
../include/PTheory.h
@ -26,6 +30,7 @@ h_sources_userFcn = \
../include/PUserFcnBase.h
h_linkdef = \
../include/PFourierCanvasLinkDef.h \
../include/PMusrCanvasLinkDef.h \
../include/PMusrT0LinkDef.h \
../include/PStartupHandlerLinkDef.h
@ -34,6 +39,7 @@ h_linkdef_userFcn = \
../include/PUserFcnBaseLinkDef.h
dict_h_sources = \
PFourierCanvasDict.h \
PMusrCanvasDict.h \
PMusrT0Dict.h \
PStartupHandlerDict.h
@ -45,6 +51,7 @@ cpp_sources = \
PFitter.cpp \
PFitterFcn.cpp \
PFourier.cpp \
PFourierCanvas.cpp \
PFunction.cpp \
PFunctionHandler.cpp \
PMsr2Data.cpp \
@ -52,13 +59,16 @@ cpp_sources = \
PMusrCanvas.cpp \
PMusr.cpp \
PMusrT0.cpp \
PPrepFourier.cpp \
PRunAsymmetry.cpp \
PRunAsymmetryRRF.cpp \
PRunBase.cpp \
PRunDataHandler.cpp \
PRunListCollection.cpp \
PRunNonMusr.cpp \
PRunMuMinus.cpp \
PRunSingleHisto.cpp \
PRunSingleHistoRRF.cpp \
PStartupHandler.cpp \
PTheory.cpp
@ -66,6 +76,7 @@ cpp_sources_userFcn = \
PUserFcnBase.cpp
dict_cpp_sources = \
PFourierCanvasDict.cpp \
PMusrCanvasDict.cpp \
PMusrT0Dict.cpp \
PStartupHandlerDict.cpp
@ -84,7 +95,7 @@ AM_LDFLAGS = $(LOCAL_LIB_LDFLAGS) -L@ROOTLIBDIR@
CLEANFILES = *Dict.cpp *Dict.h *~ core
%Dict.cpp %Dict.h: ../include/%.h ../include/%LinkDef.h
@ROOTCINT@ -v -f $*Dict.cpp -c -p $(INCLUDES) $^
@ROOTCINT@ -v -f $*Dict.cpp -c -p $(AM_CPPFLAGS) $^
lib_LTLIBRARIES = libPUserFcnBase.la libPMusr.la

View File

@ -8,7 +8,7 @@
***************************************************************************/
/***************************************************************************
* Copyright (C) 2007-2014 by Andreas Suter *
* Copyright (C) 2007-2016 by Andreas Suter *
* andreas.suter@psi.ch *
* *
* This program is free software; you can redistribute it and/or modify *
@ -1564,64 +1564,66 @@ Bool_t PFitter::ExecuteSave(Bool_t firstSave)
}
// handle expected chisq if applicable
if (fUseChi2) {
fParams = *(fRunInfo->GetMsrParamList()); // get the update parameters back
fParams = *(fRunInfo->GetMsrParamList()); // get the update parameters back
// calculate expected chisq
std::vector<Double_t> param;
Double_t totalExpectedChisq = 0.0;
std::vector<Double_t> expectedChisqPerHisto;
std::vector<UInt_t> ndfPerHisto;
// calculate expected chisq
std::vector<Double_t> param;
Double_t totalExpectedChisq = 0.0;
std::vector<Double_t> expectedChisqPerHisto;
std::vector<UInt_t> ndfPerHisto;
for (UInt_t i=0; i<fParams.size(); i++)
param.push_back(fParams[i].fValue);
for (UInt_t i=0; i<fParams.size(); i++)
param.push_back(fParams[i].fValue);
fFitterFcn->CalcExpectedChiSquare(param, totalExpectedChisq, expectedChisqPerHisto);
// CalcExpectedChiSquare handles both, chisq and mlh
fFitterFcn->CalcExpectedChiSquare(param, totalExpectedChisq, expectedChisqPerHisto);
// calculate chisq per run
std::vector<Double_t> chisqPerHisto;
for (UInt_t i=0; i<fRunInfo->GetMsrRunList()->size(); i++) {
// calculate chisq per run
std::vector<Double_t> chisqPerHisto;
for (UInt_t i=0; i<fRunInfo->GetMsrRunList()->size(); i++) {
if (fUseChi2)
chisqPerHisto.push_back(fRunListCollection->GetSingleRunChisq(param, i));
}
if (totalExpectedChisq != 0.0) { // i.e. applicable for single histogram fits only
// get the ndf's of the histos
UInt_t ndf_histo;
for (UInt_t i=0; i<expectedChisqPerHisto.size(); i++) {
ndf_histo = fFitterFcn->GetNoOfFittedBins(i) - fRunInfo->GetNoOfFitParameters(i);
ndfPerHisto.push_back(ndf_histo);
}
// feed the msr-file handler
PMsrStatisticStructure *statistics = fRunInfo->GetMsrStatistic();
if (statistics) {
statistics->fMinPerHisto = chisqPerHisto;
statistics->fMinExpected = totalExpectedChisq;
statistics->fMinExpectedPerHisto = expectedChisqPerHisto;
statistics->fNdfPerHisto = ndfPerHisto;
}
} else if (chisqPerHisto.size() > 1) { // in case expected chisq is not applicable like for asymmetry fits
UInt_t ndf_histo = 0;
for (UInt_t i=0; i<chisqPerHisto.size(); i++) {
ndf_histo = fFitterFcn->GetNoOfFittedBins(i) - fRunInfo->GetNoOfFitParameters(i);
ndfPerHisto.push_back(ndf_histo);
}
// feed the msr-file handler
PMsrStatisticStructure *statistics = fRunInfo->GetMsrStatistic();
if (statistics) {
statistics->fMinPerHisto = chisqPerHisto;
statistics->fNdfPerHisto = ndfPerHisto;
}
}
// clean up
param.clear();
expectedChisqPerHisto.clear();
ndfPerHisto.clear();
chisqPerHisto.clear();
else
chisqPerHisto.push_back(fRunListCollection->GetSingleRunMaximumLikelihood(param, i));
}
if (totalExpectedChisq != 0.0) { // i.e. applicable for single histogram fits only
// get the ndf's of the histos
UInt_t ndf_histo;
for (UInt_t i=0; i<expectedChisqPerHisto.size(); i++) {
ndf_histo = fFitterFcn->GetNoOfFittedBins(i) - fRunInfo->GetNoOfFitParameters(i);
ndfPerHisto.push_back(ndf_histo);
}
// feed the msr-file handler
PMsrStatisticStructure *statistics = fRunInfo->GetMsrStatistic();
if (statistics) {
statistics->fMinPerHisto = chisqPerHisto;
statistics->fMinExpected = totalExpectedChisq;
statistics->fMinExpectedPerHisto = expectedChisqPerHisto;
statistics->fNdfPerHisto = ndfPerHisto;
}
} else if (chisqPerHisto.size() > 1) { // in case expected chisq is not applicable like for asymmetry fits
UInt_t ndf_histo = 0;
for (UInt_t i=0; i<chisqPerHisto.size(); i++) {
ndf_histo = fFitterFcn->GetNoOfFittedBins(i) - fRunInfo->GetNoOfFitParameters(i);
ndfPerHisto.push_back(ndf_histo);
}
// feed the msr-file handler
PMsrStatisticStructure *statistics = fRunInfo->GetMsrStatistic();
if (statistics) {
statistics->fMinPerHisto = chisqPerHisto;
statistics->fNdfPerHisto = ndfPerHisto;
}
}
// clean up
param.clear();
expectedChisqPerHisto.clear();
ndfPerHisto.clear();
chisqPerHisto.clear();
cout << ">> PFitter::ExecuteSave(): will write minuit2 output file ..." << endl;
ofstream fout;

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