Run model with mcstas gamme source selene 1
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16
e2-estia.i
16
e2-estia.i
@@ -148,8 +148,8 @@ c read file=tallies/bunker_mesh.i echo
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c read file=tallies/bunker_mesh_p.i echo
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c read file=tallies/bunker_mesh_np.i echo
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c read file=tallies/bunker_mesh_act.i echo
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read file=tallies/full_mesh.i echo
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c read file=tallies/full_mesh_p.i echo
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c read file=tallies/full_mesh.i echo
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read file=tallies/full_mesh_p.i echo
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c read file=tallies/full_mesh_np.i echo
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c read file=tallies/vs_fine_mesh.i echo
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c read file=tallies/boundary_meshes.i echo
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@@ -208,9 +208,9 @@ c --------------- PHYSICS CARDS --------------------------
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c -------------------------------------------------------
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c dbcn 375642321 j j j j j j j j j j j 15291711
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c stop calculation either at XeY histories, 6.5 days or tally 15 error <0.001
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c stop nps 39242646 CTME 4e5 $f31 0.01
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c stop nps 1e9 CTME 4e5 $f31 0.01
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nps 14e10 $ works with rssa file, value is scaled to source particles
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c nps 39242646 $ works with rssa file from McStas, original tracks 39242646
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stop nps 1e7 CTME 4e5 $f31 0.01
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c nps 14e10 $ works with rssa file, value is scaled to source particles
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c write particle tracks
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c ssw 206505 pty=n $ record all neutron tracks crossing outward
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c random number generator options
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@@ -253,7 +253,7 @@ c read file=sources/proton.i echo
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c * Source Term from Valentina for 2m adapted to size
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c read file=sources/e2_2m.i echo
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c read file=sources/e2_2m_mod.i echo
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read file=sources/rssa.i echo
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c read file=sources/rssa.i echo
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c * Estimated source within bunker wall to optimize collimator efficiency
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c read file=sources/bunker_wall.i echo $ approximate, not for official results
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c * McStas source terms for gamma doeses
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@@ -261,10 +261,10 @@ c read file=sources/mcstas_rssa.i echo
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c read file=sources/mcstas_source_vs.i echo
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c read file=sources/mcstas_source_sample.i echo
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c read file=sources/mcstas_source_mf.i echo
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c read file=sources/mcstas_gammas.i echo
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read file=sources/mcstas_gammas.i echo
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c read file=sources/mcstas_gammas_2.i echo
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c read file=sources/mcstas_source_shutter.i echo
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prdmp -120 -30 1 2 -1
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prdmp -120 -30 1 2 5e5
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print 30 32 40
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c 120 $O importance function quality
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c 128 $O universe map
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@@ -1,5 +1,6 @@
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c source definition based on surface source generated from McStas
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cut:n j 0 0 0 $ use analog capture for source from McStas
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cut:n j j -0.2 -0.1 $ put weight cut-off for 0-WW to 10% of source weight
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c cut:n j 0 0 0 $ use analog capture for source from McStas
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c cut all photons that can't produce neutrons
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cut:p 1e+08 0.05
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c adjust weight windows to be essentially ignored
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@@ -1,11 +1,7 @@
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c large and detailed mesh tally covering the beamline from monolith to full cave
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tmesh
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rmesh1:p dose 1
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cora1 500 9i 1000 22i 1460
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corb1 -700 11i -100 9i 100 3i 300
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corc1 -200 1i -100 9i 100 5i 400
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rmesh11:p dose 1
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cora11 1460 151i 4500
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cora11 1300 159i 4500
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corb11 -400 59i 800
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corc11 -200 39i 600
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c Official ESS dose conversion factors from gamma/cm²/s to Sv/h
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