Files
Jungfraujoch/image_analysis/scale_merge/ScaleOnTheFly.cpp
T
leonarski_fandFilip Leonarski 19b135186d
Build Packages / Create release (push) Successful in 7s
Build Packages / build:portable:macos-arm64:nocuda (push) Successful in 4m56s
Build Packages / build:rugnux:linux-aarch64:cuda (push) Successful in 9m10s
Build Packages / build:portable:linux-x86_64:nocuda (push) Successful in 13m51s
Build Packages / build:portable:linux-x86_64:cuda (push) Successful in 16m56s
Build Packages / build:jfjoch:rocky8:nocuda (push) Successful in 20m59s
Build Packages / build:portable:windows-x86_64:nocuda (push) Successful in 21m25s
Build Packages / build:jfjoch:rocky9:nocuda (push) Successful in 21m17s
Build Packages / build:jfjoch:ubuntu2204:nocuda (push) Successful in 14m14s
Build Packages / HDF5 consumer tests (DIALS, XDS) (push) Successful in 25m59s
Build Packages / build:portable:windows-x86_64:cuda (push) Successful in 25m48s
Build Packages / build:jfjoch:ubuntu2404:nocuda (push) Successful in 15m52s
Build Packages / build:jfjoch:rocky8:cuda-sls9 (push) Successful in 19m33s
Build Packages / Generate python client (push) Successful in 29s
Build Packages / Build documentation (push) Successful in 1m19s
Build Packages / build:jfjoch:ubuntu2204:cuda (push) Successful in 20m49s
Build Packages / build:jfjoch:rocky9:cuda-sls9 (push) Successful in 25m31s
Build Packages / build:jfjoch:rocky8:cuda (push) Successful in 25m24s
Build Packages / build:jfjoch:rocky9:cuda (push) Successful in 26m5s
Build Packages / build:jfjoch:ubuntu2404:cuda (push) Successful in 22m19s
Build Packages / Unit tests (push) Failing after 2h28m24s
Build Packages / Validation Battery (push) Successful in 40m33s
v1.0.0-rc.175 (#85)
* Rugnux: Processes a collection live while jfjoch_broker writes it (`rugnux <master.h5> <broker URL>`).
* Rugnux: Processing starts on the first images and confirms its choices once all are in, so analysis can begin during collection.
* Rugnux: Faster processing, especially on servers with several GPUs and CPU sockets and on computers without a GPU (`--no-gpu`, macOS).
* Rugnux: Uses much less GPU memory, so large data sets stay on the GPU of smaller cards, and a data set too large for the card is processed on the CPU instead.
* Rugnux: On macOS, Bragg integration runs on the Apple GPU.
* Rugnux: Better handling of twinning and pseudo-symmetry, with the twin hypothesis written as `<prefix>_twin_<SG>.mtz`, and a wrong `--model` no longer confirms the data or decides the hand.
* Rugnux: `--model` accepts predicted (AlphaFold) models and falls back to molecular replacement when the model is not placed as a rigid body (experimental `--mr` forces it), settling space group, hand and twinning and writing a different answer as `<prefix>_mr.mtz`.
* Rugnux: Molecular replacement is faster and settles the space group in more cases with several copies in the asymmetric unit.
* Rugnux: Deposition-ready mmCIF, a richer report, and numbered steps on the terminal with the full log in `<prefix>_log.txt`; `_P1.mtz`, `--estimate-beam-center` and `--beam-center-search` are removed.
* Rugnux: The beam-stop shadow is found correctly on tilted detectors.
* Rugnux: Stills files that record a stationary goniometer axis get the default stills geometry refinement.
* jfjoch_viewer: "Analyze dataset" uses the same defaults as a bare `rugnux <file>`, and shows the results of processed CBF, marCCD and SMV sweeps.
* jfjoch_viewer: The Files panel refreshes on F5 and every few seconds, and the plot type and other selections stay put during live collection.
* jfjoch_writer: Memory stays bounded and old data files are closed efficiently on long runs, any failure ends the run in an error state the broker is told about, and the master file appears only after its data files; the ZeroMQ pusher logs when a stalled writer makes it drop images.
* Fixes: The TCP image pusher no longer blocks the broker's receiver, GPU out-of-memory failures stop with a clear message, and the XDS plugin masks module and chip edges.

---------

Co-authored-by: Filip Leonarski <jungfrau@filips-mac-mini.home>
Reviewed-on: #85
Co-authored-by: Filip Leonarski <filip.leonarski@psi.ch>
2026-10-16 15:34:43 +02:00

225 lines
9.2 KiB
C++

// SPDX-FileCopyrightText: 2025 Filip Leonarski, Paul Scherrer Institute <filip.leonarski@psi.ch>
// SPDX-License-Identifier: GPL-3.0-only
#include "ScaleOnTheFly.h"
#include "../../common/Logger.h"
#include "../../common/ThreadAffinity.h"
#include <algorithm>
#include <atomic>
#include <chrono>
#include <cmath>
#include <future>
#include <thread>
#include <vector>
namespace {
// Robust loss scale (in sigma units) for the per-image scale fit: a few outlier reflections
// (zingers, overlaps, a mis-predicted spot) must not drag a frame's G/B into a bad optimum -
// that is the stochastic per-frame mis-scaling that elevates R-meas and collapses CC1/2 at low
// symmetry. Cauchy down-weights residuals beyond ~this many sigma without a hard cut.
constexpr double SCALE_ROBUST_K = 3.0;
// Smallest per-image scale, relative to the run's median, that is still believable as a scale
// rather than a failed fit. The same ratio guards the rotation path's per-frame scales.
constexpr double MIN_CREDIBLE_SCALE_RATIO = 0.02;
double SafeInv(double x, double fallback) {
if (!std::isfinite(x) || x == 0.0)
return fallback;
return 1.0 / x;
}
// One reflection reduced to the 1-D scale fit: predicted intensity is G * coeff (coeff is constant
// while B is fixed), measured is Iobs, weighted by 1/sigma.
struct ScaleObs {
double coeff;
double Iobs;
double weight;
};
// Robust per-image scale: minimise sum_i Cauchy_k( weight_i (G*coeff_i - Iobs_i) ) over G >= 0. The
// model is linear in G, so this M-estimate is a few reweighted-least-squares steps (each a closed-form
// weighted ratio) - the same objective the Ceres path solves, without a per-image problem/autodiff/
// trust-region. Seeded from the plain weighted-LS solution; Cauchy weight is 1/(1 + (res/k)^2).
double SolveScaleIRLS(const std::vector<ScaleObs> &obs, double robust_k) {
auto weighted_scale = [&obs](auto robust_weight) {
double num = 0.0, den = 0.0;
for (const auto &o: obs) {
const double rw = robust_weight(o);
const double w2 = o.weight * o.weight;
num += rw * w2 * o.coeff * o.Iobs;
den += rw * w2 * o.coeff * o.coeff;
}
return den > 0.0 ? num / den : NAN;
};
double G = weighted_scale([](const ScaleObs &) { return 1.0; });
if (!std::isfinite(G))
return 1.0;
G = std::max(0.0, G);
const double k2 = robust_k * robust_k;
for (int iter = 0; iter < 30; ++iter) {
const double G_prev = G;
const double G_next = weighted_scale([&](const ScaleObs &o) {
const double res = o.weight * (G * o.coeff - o.Iobs);
return 1.0 / (1.0 + res * res / k2);
});
if (!std::isfinite(G_next))
break;
G = std::max(0.0, G_next);
if (std::abs(G - G_prev) <= 1e-7 * std::max(G, 1.0))
break;
}
return G;
}
}
ScaleOnTheFly::ScaleOnTheFly(const DiffractionExperiment &x, const std::vector<MergedReflection> &ref)
: s(x.GetScalingSettings()),
hkl_key_generator(s.GetMergeFriedel(), x.GetSpaceGroupOrP1()) {
for (const auto &r: ref) {
const auto key = hkl_key_generator(r);
reference_data[key] = r.I;
}
}
bool ScaleOnTheFly::Accept(const Reflection &r) const {
if (r.on_ice_ring) // ice-contaminated intensity would drag the per-image scale; keep it out of the fit
return false;
return AcceptReflection(r, s.GetHighResolutionLimit_A(), s.GetLowResolutionLimit_A());
}
void ScaleOnTheFly::Scale(IntegrationOutcome &integration_outcome) const {
if (integration_outcome.reflections.empty())
return;
ScaleOnTheFlyResult result{ .G = 1.0 };
auto clear_scale = [&]() {
integration_outcome.image_scale_cc.reset();
integration_outcome.image_scale_cc_n.reset();
integration_outcome.image_scale_g.reset();
};
// The fixed-partiality model G * coeff is linear in G, so the robust per-image scale is a 1-D
// M-estimate solved directly (IRLS) rather than a Ceres problem per image.
{
std::vector<ScaleObs> obs;
obs.reserve(integration_outcome.reflections.size());
for (const auto &r: integration_outcome.reflections) {
if (!Accept(r))
continue;
const auto it = reference_data.find(hkl_key_generator(r));
if (it == reference_data.end())
continue;
const double coeff = r.partiality * SafeInv(r.prescaling_corr * r.qe_corr * r.flight_corr, 1.0) * it->second;
obs.push_back({coeff, static_cast<double>(r.I), SafeInv(r.sigma, 1.0)});
}
if (obs.size() < MIN_REFLECTIONS) {
clear_scale();
return;
}
result.G = SolveScaleIRLS(obs, SCALE_ROBUST_K);
}
for (auto &r: integration_outcome.reflections) {
const float corr = r.prescaling_corr * r.qe_corr * r.flight_corr;
const double denom = r.partiality * result.G;
r.image_scale_corr = (std::isfinite(corr) && std::isfinite(denom) && denom > 0.0)
? static_cast<float>(corr / denom)
: NAN;
}
const auto [cc, cc_n] = ImageReferenceCC(integration_outcome.reflections, reference_data,
hkl_key_generator, s.GetHighResolutionLimit_A(),
s.GetLowResolutionLimit_A(), s.GetMinPartiality());
result.cc = cc;
result.cc_n = cc_n;
integration_outcome.image_scale_cc = cc;
integration_outcome.image_scale_cc_n = cc_n;
integration_outcome.image_scale_g = result.G;
integration_outcome.image_scale_wedge_deg.reset();
}
// A per-image scale that has collapsed toward zero multiplies that image's intensities by 1/G - and its
// sigmas by the same factor, so nothing downstream can recognise it: the merge's n-sigma outlier test
// scales with the very number that is wrong. The rotation path already refuses a per-frame scale this
// far below its neighbours; the stills path had no such guard.
//
// Such an image is DROPPED from the merge, not merged unscaled. Substituting G = 1 looks conservative
// but is the more damaging of the two errors: if the collapsed value was a failed fit, the image goes in
// mis-scaled by an unknown factor, and if it was a real scale (per-crystal scales on serial stills
// genuinely span orders of magnitude, unlike frames of one rotation sweep) then G = 1 divides both its
// intensities AND its sigmas by 1/G, so it enters at 1/G^2 times the weight it deserves - the merge
// cannot down-weight it, because the number that is wrong is the same number the weight is built from.
// An image whose scale is not believable has no usable scale, so it contributes nothing instead.
void ScaleOnTheFly::RejectCollapsedScales(std::vector<IntegrationOutcome> &integration) {
std::vector<double> fitted;
fitted.reserve(integration.size());
for (const auto &i: integration)
if (i.image_scale_g && std::isfinite(*i.image_scale_g) && *i.image_scale_g > 0.0)
fitted.push_back(*i.image_scale_g);
if (fitted.size() < 2)
return;
const size_t mid = fitted.size() / 2;
std::nth_element(fitted.begin(), fitted.begin() + mid, fitted.end());
const double g_floor = fitted[mid] * MIN_CREDIBLE_SCALE_RATIO;
int64_t n_rejected = 0;
for (auto &i: integration) {
if (!i.image_scale_g || !std::isfinite(*i.image_scale_g) || *i.image_scale_g >= g_floor)
continue;
// A non-finite correction is what every merge path already skips on (Merge.cpp), so this drops
// the image consistently from the merged intensities, the error model and the statistics.
for (auto &r: i.reflections)
r.image_scale_corr = NAN;
i.image_scale_cc.reset();
i.image_scale_cc_n.reset();
i.image_scale_g.reset();
++n_rejected;
}
if (n_rejected > 0)
Logger("ScaleOnTheFly").Warning(
"Dropped {} image(s) from the merge: their per-image scale collapsed more than {:.0f}x below "
"the run median, so it is not a scale the intensities can be put on",
n_rejected, 1.0 / MIN_CREDIBLE_SCALE_RATIO);
}
void ScaleOnTheFly::Scale(std::vector<IntegrationOutcome> &integration, size_t nthreads) const {
if (nthreads == 0)
nthreads = AvailableCpus();
if (nthreads <= 1) {
for (auto & i : integration)
Scale(i);
} else {
auto local_nthreads = std::min(nthreads, integration.size());
std::vector<std::future<void>> futures;
futures.reserve(local_nthreads);
std::atomic<size_t> curr_image = 0;
for (size_t t = 0; t < local_nthreads; ++t)
futures.emplace_back(std::async(std::launch::async, [&] {
size_t i = curr_image.fetch_add(1);
while (i < integration.size()) {
Scale(integration[i]);
i = curr_image.fetch_add(1);
}
}));
for (auto &f: futures)
f.get();
}
RejectCollapsedScales(integration);
}