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Jungfraujoch/common/Definitions.h
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leonarski_fandClaude Opus 5 64169bb04d rugnux: a measured spot budget below the input floor degrades the run instead of killing it
The rotation first pass measures how deep each image's intensity-ordered spot list
still lies on the lattice and adopts that depth as the spot budget. The measurement
can honestly land below ten - seen where a wrong header detector distance left
indexing a compensating, uniformly scaled cell that matches only the few brightest,
most central spots - but the setter rejects anything under ten, so the run died on
its own measurement, reporting a parameter the user never set.

The floor predates the estimator by a year and was written to guard user input; by
provenance it is the stills fitting bound, one more than a viable cell needs, which a
rotation pass that only tests a lattice already in hand does not owe anything to.
Exempting the measurement entirely would be worse than the crash: the validation gate
still needs that many indexed spots per frame, so a shorter list can never index
anything and the pass would abort one confusing error later.

So the floor gets a name beside its companion, keeps its job for input, and the
measured budget is clamped to it before adoption - with a warning saying what a
sub-floor measurement means: the geometry in the file or the lattice is wrong, not
that the crystal is weak.

The dataset that died now completes like its siblings with the cause named; the same
data at the reference-refined distance indexes 99% of images and measures no budget
cut at all; and runs whose budgets sit at or above the floor are report-identical,
checked at the two lowest in the corpus.

Co-Authored-By: Claude Opus 5 <noreply@anthropic.com>
Claude-Session: https://claude.ai/code/session_01EFEJG6WBQv8th4UJFNe53N
2026-09-05 23:33:43 +02:00

105 lines
5.5 KiB
C++

// SPDX-FileCopyrightText: 2024 Filip Leonarski, Paul Scherrer Institute <filip.leonarski@psi.ch>
// SPDX-License-Identifier: GPL-3.0-only
#pragma once
#include "../fpga/pcie_driver/jfjoch_fpga.h"
#include <cstdint>
#include <cstddef>
#include <chrono>
#include <array>
#include <cmath>
constexpr float WVL_1A_IN_KEV = 12.39854f;
constexpr size_t CONVERTED_MODULE_LINES = 514;
constexpr size_t CONVERTED_MODULE_COLS = 1030;
constexpr size_t CONVERTED_MODULE_SIZE = CONVERTED_MODULE_LINES * CONVERTED_MODULE_COLS;
constexpr size_t JUNGFRAU_PACKET_SIZE_BYTES = 8192;
constexpr int MAX_IMAGE_NUMBER = 2*1024*1024;
// Defaults for images_per_file when the acquisition does not ask for a particular number; see
// DiffractionExperiment::GetImagesPerFile.
constexpr int64_t DEFAULT_IMAGES_PER_FILE = 1000;
// Above this, a rotation sweep is split rather than written to one file.
constexpr int64_t ROTATION_SINGLE_FILE_IMAGE_LIMIT = 20000;
constexpr std::chrono::nanoseconds MIN_COUNT_TIME = std::chrono::microseconds(3);
constexpr std::chrono::nanoseconds MIN_STORAGE_CELL_DELAY = std::chrono::nanoseconds(2100);
constexpr std::chrono::nanoseconds MIN_FRAME_TIME_JUNGFRAU_HALF_SPEED = std::chrono::microseconds(1000);
constexpr std::chrono::nanoseconds MIN_FRAME_TIME_JUNGFRAU_FULL_SPEED = std::chrono::microseconds(470);
constexpr std::chrono::nanoseconds MIN_FRAME_TIME_EIGER = std::chrono::microseconds(250);
constexpr std::chrono::nanoseconds MAX_COUNT_TIME_JUNGFRAU = std::chrono::microseconds(2000);
constexpr std::chrono::nanoseconds FRAME_TIME_PEDE_G1G2 = std::chrono::microseconds(10*1000);
constexpr std::chrono::nanoseconds PSI_JUNGFRAU_READOUT_TIME = std::chrono::microseconds(20);
constexpr std::chrono::nanoseconds PSI_EIGER_READOUT_TIME = std::chrono::microseconds(20);
constexpr std::chrono::nanoseconds DARK_MASK_FRAME_TIME = std::chrono::milliseconds(10);
constexpr float MIN_ENERGY_KEV = 0.001;
constexpr float MAX_ENERGY_KEV = 500.0;
constexpr float DEFAULT_G0_FACTOR = 41.0f;
constexpr float DEFAULT_G1_FACTOR = -1.439f;
constexpr float DEFAULT_G2_FACTOR = -0.1145f;
constexpr float DEFAULT_HG0_FACTOR = 100.0f;
constexpr int MAX_SPOT_COUNT = 64 * 1024;
// Three spots fit any lattice at all; one short of ViableCellMinSpots (default 9) is where a fitted
// lattice stops being distinguishable from a random one, so a spot list shorter than this is never
// worth handing to indexing - and the frame gate needs the same count to validate a frame
// (AnalyzeIndexing), so a shorter list could never index anything anyway.
constexpr int MIN_SPOT_COUNT = 10;
constexpr uint32_t MASK_PEDESTAL_G0_RMS_LIMIT = (1U<<4);
constexpr size_t PEDESTAL_MIN_IMAGE_COUNT = 128;
constexpr uint16_t PEDESTAL_WRONG = (UINT16_MAX);
constexpr size_t PEDESTAL_G0_WRONG_GAIN_ALLOWED_COUNT = 2;
constexpr size_t MESSAGE_SIZE_FOR_START_END = (256*1024*1024); // pessimistic highest value
constexpr float LAB6_CELL_A = 4.156468f;
// Hexagonal-ice ring positions. The first eleven are the measured ones from:
// Moreau, Atakisi, Thorne, Acta Cryst D77, 2021, 540,554
// https://journals.iucr.org/d/issues/2021/04/00/tz5104/index.html
// That paper's Table 1 stops at 1.522 A because it says so in its own words - "pure hexagonal ice has
// 11 diffraction rings between 4 and 1.5 A resolution" - and its subject was detecting ice in the PDB,
// not masking it. Ice does not stop there, and on a detector that reaches past 1.5 A the rings it does
// not list are the ones left in the data: one strongly diffracting set had 44% of every frame's spots
// in ice bands, and beyond 1.5 A its spots were ice and nothing else.
//
// The rest are calculated, because past that paper there is nothing measured to copy. Ice Ih is
// P6_3/mmc with O on 4f, so enumerating hkl is not enough - most of what it emits is extinguished by
// the oxygen sublattice rather than by the space group, which is why (004) at 1.830 A and (104) at
// 1.657 A are absent from the measured list although they lie inside its range and its reflection
// conditions allow them. Structure factors were computed instead (oxygen only - the hydrogens are
// half-occupancy disordered and scatter X-rays weakly) and the lines kept are those reaching 3% of the
// strongest. That reproduces the measured eleven exactly, and every line it drops in their range
// computes to zero, which is what makes the same rule trustworthy below 1.522 A.
// Following Roettger, Endriss, Ihringer, Doyle & Kuhs (1994) Acta Cryst. B50, 644-648 for the cell.
//
// It stops at 1.170 A: below that the calculated real lines fall to 2-3% while the extinct ones rise
// to about 1%, and an oxygen-only calculation cannot separate them honestly any further.
constexpr std::array<float, 19> ICE_RING_RES_A = {3.895, 3.661, 3.438, 2.667, 2.249, 2.068, 1.947,
1.916, 1.882, 1.719, 1.522,
1.472, 1.443, 1.371, 1.366, 1.298, 1.261, 1.224,
1.170};
// True when resolution d (Angstrom) sits within half_width of a hexagonal-ice powder ring, in the
// q = 2*pi/d units the spot-finder uses (ice_ring_width_Q_recipA). Used to drop ice-contaminated
// reflections from scaling/merging when ice-ring handling is enabled.
inline bool IsOnIceRing(float d_A, float half_width_q_recipA) {
if (!(d_A > 0.0f))
return false;
constexpr float two_pi = 6.283185307f;
const float q = two_pi / d_A;
for (const float ice_d : ICE_RING_RES_A)
if (std::fabs(q - two_pi / ice_d) < half_width_q_recipA)
return true;
return false;
}