Files
Jungfraujoch/image_analysis/scale_merge/StillsPartialityRefine.cpp
T
leonarski_fandClaude Opus 5 26fc4b02b3 symmetry: carry the space group as the group, not as its number
The adopted space group travelled the pipeline as a bare int and was rebuilt
downstream with find_spacegroup_by_number, which returns the reference setting.
So every setting a number cannot name was destroyed one line after it was
determined: P 1 1 2 came back as P 1 2 1, I 1 1 2 as C 1 2 1, R 3:R as R 3:H.

DatasetSettings now holds the gemmi::SpaceGroup itself, DiffractionExperiment
exposes it as GetGemmiSpaceGroup() / GetSpaceGroupOrP1(), and everything that
used to take an int - HKLKeyGenerator (its int constructor is gone, so the
compiler finds the callers), the merge, the R-free flags, French-Wilson, the
reindexing ambiguity, the completeness enumeration, the MTZ and mmCIF exports,
the model validation - takes the group. -S keeps the setting the symbol names
rather than reducing it to a number.

The end message carries both spellings and a reader prefers the name, since
only the name keeps the setting while the number is what a reader written
before the name understands. It carries them over CBOR too: the determined
group was never serialised at all, so a group rugnux chose reached the master
file only when the same process wrote it, and an online writer fell back to
whatever the user had supplied at the start. Both keys are optional additions,
so an older reader skips them and a newer one reads an older sender.

On disk the master's /entry/sample/space_group carries the extended
Hermann-Mauguin name and is what the reader takes the group from, so a setting
survives a _process.h5 and the --mode scale that re-reads it; the number stays
beside it and is the fallback for files written before. Every one of the 230
reference settings the old writer could produce reads back as itself, so older
files are unaffected.

Stage A and Stage B of the search still enumerate reference settings only, so
this determines no group differently today - it is what the enumeration needs
before it can be widened.

Co-Authored-By: Claude Opus 5 (1M context) <noreply@anthropic.com>
Claude-Session: https://claude.ai/code/session_01EFEJG6WBQv8th4UJFNe53N
2026-08-31 07:16:43 +02:00

397 lines
18 KiB
C++

// SPDX-FileCopyrightText: 2025 Filip Leonarski, Paul Scherrer Institute <filip.leonarski@psi.ch>
// SPDX-License-Identifier: GPL-3.0-only
#include "StillsPartialityRefine.h"
#include <atomic>
#include <cmath>
#include <future>
#include <thread>
#include <vector>
#include <ceres/ceres.h>
#include <ceres/rotation.h>
#include "Merge.h"
namespace {
constexpr size_t MIN_FIT_REFLECTIONS = 20;
constexpr double kRadToDeg = 180.0 / 3.14159265358979323846;
double SafeInv(double x, double fallback) {
if (!std::isfinite(x) || x == 0.0)
return fallback;
return 1.0 / x;
}
// One accepted reflection reduced to the physical partiality fit: the base reciprocal vector q (crystal
// frame at the stored per-image orientation), the reference full intensity, the measured intensity, the
// Lorentz factor and the weight. dist_ewald / partiality are recomputed from q under the refined tilt.
struct FitObs {
double qx, qy, qz;
double Iref;
double Iobs;
double lp; // 1 / rlp
double weight; // 1 / sigma
};
double VecLen(double x, double y, double z) { return std::sqrt(x * x + y * y + z * z); }
// Analytic partiality for a reflection whose base reciprocal vector is q, tilted by (psi_x, psi_y).
// Mirrors BraggPrediction: dist_ewald = |S| - 1/lambda with S = q_rot + S0, and
// p = exp(-dist_ewald^2 / 2 sigma^2), sigma^2 = gamma0^2 + (gamma_e*d*)^2 + (bw*|q_z|)^2 - three
// independent broadenings added in quadrature: the reciprocal-lattice point's own radius (gamma0,
// ~1/domain size, resolution-INdependent), the mosaic/divergence spread (gamma_e*d*, proportional to
// d*) and the bandwidth smear along the beam. In practice the fit below returns gamma_e ~ 0 and the
// width is essentially gamma0 - see there.
double ComputeP(double qx, double qy, double qz,
double psi_x, double psi_y,
double s0x, double s0y, double s0z, double inv_lambda,
double gamma0, double gamma_e, double bw) {
double aa[3] = {psi_x, psi_y, 0.0};
double q[3] = {qx, qy, qz};
double qr[3];
ceres::AngleAxisRotatePoint(aa, q, qr);
const double Sx = qr[0] + s0x, Sy = qr[1] + s0y, Sz = qr[2] + s0z;
const double de = std::sqrt(Sx * Sx + Sy * Sy + Sz * Sz) - inv_lambda;
const double dstar = std::sqrt(qr[0] * qr[0] + qr[1] * qr[1] + qr[2] * qr[2]);
const double sig_ang = gamma_e * dstar;
const double sbw = bw * std::fabs(qr[2]);
const double sig2 = gamma0 * gamma0 + sig_ang * sig_ang + sbw * sbw;
if (!(sig2 > 0.0))
return 1.0;
return std::exp(-0.5 * de * de / sig2);
}
// Robust per-crystal scale G (linear in G given the model coefficients), identical objective to
// ScaleOnTheFly::SolveScaleIRLS: minimise sum Cauchy_k( w (G*coeff - Iobs) ) over G >= 0.
double SolveScaleIRLS(const std::vector<double> &coeff, const std::vector<double> &Iobs,
const std::vector<double> &weight, double robust_k) {
auto weighted_scale = [&](auto robust_weight) {
double num = 0.0, den = 0.0;
for (size_t i = 0; i < coeff.size(); ++i) {
const double rw = robust_weight(i);
const double w2 = weight[i] * weight[i];
num += rw * w2 * coeff[i] * Iobs[i];
den += rw * w2 * coeff[i] * coeff[i];
}
return den > 0.0 ? num / den : NAN;
};
double G = weighted_scale([](size_t) { 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([&](size_t i) {
const double res = weight[i] * (G * coeff[i] - Iobs[i]);
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;
}
// Ceres residual: refine the orientation tilt (psi_x, psi_y) holding the scale G fixed. The tilt
// rotates the base reciprocal vector q; partiality follows analytically. Residual is the intensity
// mismatch weighted by 1/sigma, exactly matching ScaleOnTheFly's intensity-space objective.
struct PsiResidual {
double qx, qy, qz;
double s0x, s0y, s0z, inv_lambda;
double gamma0, gamma_e, bw;
double G, lp, Iref, Iobs, weight;
template<typename T>
bool operator()(const T *const psi, T *residual) const {
T q[3] = {T(qx), T(qy), T(qz)};
T aa[3] = {psi[0], psi[1], T(0.0)};
T qr[3];
ceres::AngleAxisRotatePoint(aa, q, qr);
const T Sx = qr[0] + T(s0x), Sy = qr[1] + T(s0y), Sz = qr[2] + T(s0z);
const T de = ceres::sqrt(Sx * Sx + Sy * Sy + Sz * Sz) - T(inv_lambda);
const T dstar = ceres::sqrt(qr[0] * qr[0] + qr[1] * qr[1] + qr[2] * qr[2]);
const T sig_ang = T(gamma_e) * dstar;
const T sbw = T(bw) * ceres::abs(qr[2]);
const T sig2 = T(gamma0) * T(gamma0) + sig_ang * sig_ang + sbw * sbw;
const T p = ceres::exp(T(-0.5) * de * de / sig2);
residual[0] = T(weight) * (T(G) * p * T(lp) * T(Iref) - T(Iobs));
return true;
}
};
// Gaussian prior N(0, sigma_prior^2) on the tilt. The data residuals above are (model-obs)/sigma, a
// proper chi^2, so the MAP prior residual is simply dpsi/sigma_prior - no scale calibration needed.
struct PsiPrior {
double inv_sigma;
template<typename T>
bool operator()(const T *const psi, T *residual) const {
residual[0] = T(inv_sigma) * psi[0];
residual[1] = T(inv_sigma) * psi[1];
return true;
}
};
}
StillsPartialityRefine::StillsPartialityRefine(const DiffractionExperiment &x)
: experiment_(x),
hkl_key_generator_(x.GetScalingSettings().GetMergeFriedel(), x.GetSpaceGroupOrP1()),
d_min_limit_(x.GetScalingSettings().GetHighResolutionLimit_A()),
d_max_limit_(x.GetScalingSettings().GetLowResolutionLimit_A()),
min_partiality_(x.GetScalingSettings().GetMinPartiality()),
bandwidth_sigma_(x.GetBandwidthFWHM().value_or(0.0f) / 2.3548f) {}
double StillsPartialityRefine::RefineOne(IntegrationOutcome &outcome,
const std::map<HKLKey, double> &reference) const {
if (outcome.reflections.empty())
return 0.0;
const Coord Astar = outcome.latt.Astar();
const Coord Bstar = outcome.latt.Bstar();
const Coord Cstar = outcome.latt.Cstar();
const Coord S0 = outcome.geom.GetScatteringVector();
const double inv_lambda = 1.0 / outcome.geom.GetWavelength_A();
const double bw = bandwidth_sigma_;
auto base_q = [&](const Reflection &r) {
return Astar * static_cast<float>(r.h) + Bstar * static_cast<float>(r.k)
+ Cstar * static_cast<float>(r.l);
};
// Collect the reflections that constrain the fit (accepted, non-ice, finite, present in the reference).
std::vector<FitObs> obs;
obs.reserve(outcome.reflections.size());
// Moments of the excitation error against resolution: de^2 ~ gamma0^2 + gamma_e^2 * d*^2, fitted per
// crystal by ordinary least squares on (d*^2, de^2). Both components come out of the data.
double m_n = 0.0, m_x = 0.0, m_xx = 0.0, m_y = 0.0, m_xy = 0.0;
size_t n_de = 0;
for (const Reflection &r: outcome.reflections) {
if (r.on_ice_ring || !AcceptReflection(r, d_min_limit_, d_max_limit_))
continue;
if (!std::isfinite(r.I) || !std::isfinite(r.sigma) || r.sigma <= 0.0f)
continue;
const auto it = reference.find(hkl_key_generator_(r));
if (it == reference.end() || !std::isfinite(it->second))
continue;
const Coord q = base_q(r);
obs.push_back(FitObs{
.qx = q.x, .qy = q.y, .qz = q.z,
.Iref = it->second,
.Iobs = static_cast<double>(r.I),
.lp = SafeInv(r.rlp, 1.0),
.weight = SafeInv(r.sigma, 1.0),
});
// Excitation error at the stored orientation (psi = 0), collected as the moments of de^2 against
// d*^2, so BOTH width components are fitted rather than one being forced to zero. Forcing the
// width to be purely angular (gamma0 = 0) pins it to the high-resolution edge - it is fitted over
// a d*^2-dense population - and it then collapses at low d*, giving p ~ 0 for reflections that
// were plainly recorded, which inflated the merged low-resolution intensity scale ~3.6x.
const double dstar = VecLen(q.x, q.y, q.z);
const double de0 = VecLen(q.x + S0.x, q.y + S0.y, q.z + S0.z) - inv_lambda;
if (dstar > 1e-9) {
const double x = dstar * dstar, y = de0 * de0;
m_n += 1.0;
m_x += x;
m_xx += x * x;
m_y += y;
m_xy += x * y;
++n_de;
}
}
if (obs.size() < MIN_FIT_REFLECTIONS || n_de == 0)
return 0.0;
// Solve the 2x2 normal equations for de^2 = A + B d*^2. A degenerate spread in d* (all reflections in
// one shell) leaves B undetermined, so fall back to the pure angular width there; a negative fitted
// component is unphysical and is clamped to zero, which reduces to the previous model.
//
// Measured outcome, worth knowing before touching this: the fit does NOT split the width between the
// two terms - it returns gamma0 ~ 4e-4 1/A and gamma_e ~ 0 (their cross-over sits at d = 0.3 A, far
// outside any measured range), i.e. a width constant in the LINEAR Ewald distance. That is
// structural, not a fluke: prediction accepts reflections on a fixed linear |dist_ewald| cutoff, so
// the accepted population's de^2 is flat in d*^2 by construction and the slope is genuinely ~0. The
// truncated population cannot constrain an angular term; the resolution-independent one is what the
// data actually support.
const double det = m_n * m_xx - m_x * m_x;
double A = 0.0, B = 0.0;
if (std::fabs(det) > 1e-30) {
A = (m_xx * m_y - m_x * m_xy) / det;
B = (m_n * m_xy - m_x * m_y) / det;
} else {
B = m_x > 0.0 ? m_y / m_x : 0.0;
}
const double gamma0 = std::sqrt(std::max(0.0, A));
const double gamma_e_fit = std::max(std::sqrt(std::max(0.0, B)), 1e-9);
const double gamma_e = settings_.gamma_e > 0.0 ? settings_.gamma_e : gamma_e_fit;
double psi[2] = {0.0, 0.0};
double G = 1.0;
const bool refine_tilt = obs.size() >= settings_.min_reflections;
const int inner = refine_tilt ? settings_.inner_iterations : 1;
for (int it = 0; it < inner; ++it) {
// (1) Solve G given the current partialities.
std::vector<double> coeff(obs.size()), Iobs(obs.size()), weight(obs.size());
for (size_t j = 0; j < obs.size(); ++j) {
const double p = ComputeP(obs[j].qx, obs[j].qy, obs[j].qz, psi[0], psi[1],
S0.x, S0.y, S0.z, inv_lambda, gamma0, gamma_e, bw);
coeff[j] = p * obs[j].lp * obs[j].Iref;
Iobs[j] = obs[j].Iobs;
weight[j] = obs[j].weight;
}
G = SolveScaleIRLS(coeff, Iobs, weight, settings_.robust_k);
if (!(G > 0.0) || !std::isfinite(G))
return 0.0;
if (!refine_tilt)
break;
// (2) Refine the tilt holding G fixed.
ceres::Problem problem;
for (const auto &o: obs) {
auto *cost = new ceres::AutoDiffCostFunction<PsiResidual, 1, 2>(new PsiResidual{
.qx = o.qx, .qy = o.qy, .qz = o.qz,
.s0x = S0.x, .s0y = S0.y, .s0z = S0.z, .inv_lambda = inv_lambda,
.gamma0 = gamma0, .gamma_e = gamma_e, .bw = bw,
.G = G, .lp = o.lp, .Iref = o.Iref, .Iobs = o.Iobs, .weight = o.weight});
problem.AddResidualBlock(cost, new ceres::CauchyLoss(settings_.robust_k), psi);
}
if (settings_.prior_sigma_deg > 0.0) {
const double inv_sigma = kRadToDeg / settings_.prior_sigma_deg; // 1 / sigma_prior (rad)
problem.AddResidualBlock(new ceres::AutoDiffCostFunction<PsiPrior, 2, 2>(
new PsiPrior{inv_sigma}), nullptr, psi);
}
problem.SetParameterLowerBound(psi, 0, -settings_.max_tilt_rad);
problem.SetParameterUpperBound(psi, 0, settings_.max_tilt_rad);
problem.SetParameterLowerBound(psi, 1, -settings_.max_tilt_rad);
problem.SetParameterUpperBound(psi, 1, settings_.max_tilt_rad);
ceres::Solver::Options options;
options.linear_solver_type = ceres::DENSE_QR;
options.minimizer_progress_to_stdout = false;
options.num_threads = 1;
options.max_num_iterations = 25;
ceres::Solver::Summary summary;
const double psi_before[2] = {psi[0], psi[1]};
ceres::Solve(options, &problem, &summary);
// A solve that failed leaves whatever the minimiser last wrote in psi, and that tilt would go
// straight onto every reflection's partiality below. Keep the tilt this crystal came in with
// and stop refining it instead - G alone is still a usable model.
if (!summary.IsSolutionUsable()) {
psi[0] = psi_before[0];
psi[1] = psi_before[1];
break;
}
}
// Keep what the crystal came in with. This refinement is on by default, so a crystal the tilt model
// happens to suit WORSE than the fixed partiality it replaces must not be made worse by it - and
// whether it suits is only known once the corrections are written and the CC re-measured.
const auto cc_before = outcome.image_scale_cc;
const auto g_before = outcome.image_scale_g;
std::vector<std::pair<float, float>> before; // partiality, image_scale_corr
before.reserve(outcome.reflections.size());
for (const auto &r: outcome.reflections)
before.emplace_back(r.partiality, r.image_scale_corr);
// Write the refined partiality + scale correction onto every reflection of the crystal (not only the
// fit subset), so the merge sees a consistent model. image_scale_corr = rlp / (partiality * G), the
// same composition ScaleOnTheFly writes.
for (auto &r: outcome.reflections) {
const Coord q = base_q(r);
const double p = ComputeP(q.x, q.y, q.z, psi[0], psi[1], S0.x, S0.y, S0.z, inv_lambda,
gamma0, gamma_e, bw);
r.partiality = static_cast<float>(p);
const double denom = p * G;
r.image_scale_corr = (std::isfinite(r.rlp) && std::isfinite(denom) && denom > 0.0)
? static_cast<float>(r.rlp / denom)
: NAN;
}
outcome.image_scale_g = static_cast<float>(G);
// The corrections just changed, so the CC that ScaleOnTheFly measured no longer describes them.
// Refresh it here: it is reported per image and --min-image-cc drops images by it, so it has to be
// the CC of the data that is actually merged.
const auto [cc, cc_n] = ImageReferenceCC(outcome.reflections, reference, hkl_key_generator_,
d_min_limit_, d_max_limit_, min_partiality_);
// Adopt the refined model only if it correlates with the reference at least as well as the model it
// replaces. Rejecting puts the crystal back exactly as it arrived, which is the same state a
// crystal with too few reflections to fit ends in. A CC that cannot be measured at all counts as
// worse, not as no opinion: ImageReferenceCC returns NaN when too few reflections clear the
// partiality cut, which is precisely what a refinement that collapsed the partialities produces -
// and adopting it would leave image_scale_cc NaN, on which --min-image-cc drops the image outright.
if (cc_before.has_value() && std::isfinite(*cc_before) && !(std::isfinite(cc) && cc >= *cc_before)) {
for (size_t i = 0; i < outcome.reflections.size(); ++i) {
outcome.reflections[i].partiality = before[i].first;
outcome.reflections[i].image_scale_corr = before[i].second;
}
outcome.image_scale_g = g_before;
return 0.0; // nothing adopted, so no tilt to report
}
outcome.image_scale_cc = cc;
outcome.image_scale_cc_n = cc_n;
const double tilt_deg = std::sqrt(psi[0] * psi[0] + psi[1] * psi[1]) * kRadToDeg;
return tilt_deg;
}
double StillsPartialityRefine::Run(std::vector<IntegrationOutcome> &outcomes, size_t nthreads) const {
if (nthreads == 0)
nthreads = std::thread::hardware_concurrency();
nthreads = std::max<size_t>(1, nthreads);
double last_mean_tilt = 0.0;
for (int outer = 0; outer < settings_.outer_iterations; ++outer) {
// Reference full intensities from the current corrections.
const std::vector<MergedReflection> merged = MergeAll(experiment_, outcomes);
std::map<HKLKey, double> reference;
for (const auto &m: merged)
reference[hkl_key_generator_(m)] = m.I;
std::atomic<double> tilt_sum{0.0};
std::atomic<size_t> tilt_n{0};
std::atomic<size_t> next{0};
auto worker = [&]() {
size_t i = next.fetch_add(1);
while (i < outcomes.size()) {
const double t = RefineOne(outcomes[i], reference);
if (t > 0.0) {
double prev = tilt_sum.load();
while (!tilt_sum.compare_exchange_weak(prev, prev + t)) {}
tilt_n.fetch_add(1);
}
i = next.fetch_add(1);
}
};
const size_t nt = std::min(nthreads, std::max<size_t>(1, outcomes.size()));
if (nt <= 1) {
worker();
} else {
std::vector<std::future<void>> futures;
futures.reserve(nt);
for (size_t t = 0; t < nt; ++t)
futures.emplace_back(std::async(std::launch::async, worker));
for (auto &f: futures)
f.get();
}
last_mean_tilt = tilt_n > 0 ? tilt_sum.load() / static_cast<double>(tilt_n.load()) : 0.0;
}
return last_mean_tilt;
}