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#include "MantidAlgorithms/CalMuonDetectorPhases.h"
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#include "MantidAPI/Axis.h"
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#include "MantidAPI/FunctionFactory.h"
#include "MantidAPI/GroupingLoader.h"
#include "MantidAPI/ITableWorkspace.h"
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#include "MantidAPI/IFunction.h"
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#include "MantidAPI/MatrixWorkspace.h"
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#include "MantidAPI/MultiDomainFunction.h"
#include "MantidAPI/Run.h"
#include "MantidAPI/TableRow.h"
#include "MantidIndexing/IndexInfo.h"
#include "MantidKernel/ArrayProperty.h"
#include "MantidKernel/PhysicalConstants.h"
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#include "MantidAPI/WorkspaceFactory.h"
#include "MantidAPI/WorkspaceGroup.h"
namespace Mantid {
namespace Algorithms {
using namespace Kernel;
using API::Progress;
// Register the algorithm into the AlgorithmFactory
DECLARE_ALGORITHM(CalMuonDetectorPhases)
/** Initializes the algorithm's properties.
*/
void CalMuonDetectorPhases::init() {
declareProperty(make_unique<API::WorkspaceProperty<>>("InputWorkspace", "",
Direction::Input),
"Name of the reference input workspace");
declareProperty("FirstGoodData", EMPTY_DBL(),
"First good data point in units of micro-seconds",
Direction::Input);
declareProperty("LastGoodData", EMPTY_DBL(),
"Last good data point in units of micro-seconds",
declareProperty("Frequency", EMPTY_DBL(),
"Starting hint for the frequency in MHz", Direction::Input);
declareProperty(make_unique<API::WorkspaceProperty<API::ITableWorkspace>>(
"DetectorTable", "", Direction::Output),
"Name of the TableWorkspace in which to store the list "
"of phases and asymmetries");
declareProperty(make_unique<API::WorkspaceProperty<API::WorkspaceGroup>>(
"DataFitted", "", Direction::Output),
"Name of the output workspace holding fitting results");
declareProperty(
make_unique<ArrayProperty<int>>("ForwardSpectra", Direction::Input),
"The spectra numbers of the forward group. If not specified "
"will read from file.");
declareProperty(
make_unique<ArrayProperty<int>>("BackwardSpectra", Direction::Input),
"The spectra numbers of the backward group. If not specified "
"will read from file.");
/** Validates the inputs.
*/
std::map<std::string, std::string> CalMuonDetectorPhases::validateInputs() {
std::map<std::string, std::string> result;
API::MatrixWorkspace_const_sptr inputWS = getProperty("InputWorkspace");
if (inputWS) {
// Check units, should be microseconds
Unit_const_sptr unit = inputWS->getAxis(0)->unit();
if ((unit->label().ascii() != "Microseconds") &&
(unit->label().ascii() != "microsecond")) {
result["InputWorkspace"] = "InputWorkspace units must be microseconds";
}
// Check spectra numbers are valid, if specified
int nspec = static_cast<int>(inputWS->getNumberHistograms());
std::vector<int> forward = getProperty("ForwardSpectra");
std::vector<int> backward = getProperty("BackwardSpectra");
for (int spec : forward) {
if (spec < 1 || spec > nspec) {
result["ForwardSpectra"] = "Invalid spectrum numbers in ForwardSpectra";
}
for (int spec : backward) {
if (spec < 1 || spec > nspec) {
result["BackwardSpectra"] =
"Invalid spectrum numbers in BackwardSpectra";
}
}
}
return result;
}
//----------------------------------------------------------------------------------------------
/** Executes the algorithm.
*/
void CalMuonDetectorPhases::exec() {
m_inputWS = getProperty("InputWorkspace");
double startTime = getStartTime();
double endTime = getEndTime();
// Prepares the workspaces: extracts data from [startTime, endTime]
API::MatrixWorkspace_sptr tempWS =
extractDataFromWorkspace(startTime, endTime);
// Get the frequency
double freq = getFrequency(tempWS);
// Create the output workspaces
auto tab = API::WorkspaceFactory::Instance().createTable("TableWorkspace");
auto group = boost::make_shared<API::WorkspaceGroup>();
// Get the name of 'DataFitted'
std::string groupName = getPropertyValue("DataFitted");
// Remove exponential decay and fit the workspace
auto wsToFit = removeExpDecay(tempWS);
fitWorkspace(wsToFit, freq, groupName, tab, group);
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// Set the table
setProperty("DetectorTable", tab);
// Set the group
setProperty("DataFitted", group);
/** Fits each spectrum in the workspace to f(x) = A * sin( w * x + p)
* @param ws :: [input] The workspace to fit
* @param freq :: [input] Hint for the frequency (w)
* @param groupName :: [input] The name of the output workspace group
* @param resTab :: [output] Table workspace storing the asymmetries and phases
* @param resGroup :: [output] Workspace group storing the fitting results
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*/
void CalMuonDetectorPhases::fitWorkspace(const API::MatrixWorkspace_sptr &ws,
double freq, std::string groupName,
API::ITableWorkspace_sptr &resTab,
API::WorkspaceGroup_sptr &resGroup) {
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int nhist = static_cast<int>(ws->getNumberHistograms());
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// Create the fitting function f(x) = A * sin ( w * x + p )
// The same function and initial parameters are used for each fit
std::string funcStr = createFittingFunction(freq, true);
// Set up results table
resTab->addColumn("int", "Spectrum number");
resTab->addColumn("double", "Asymmetry");
resTab->addColumn("double", "Phase");
const auto &indexInfo = ws->indexInfo();
// Loop through fitting all spectra individually
const static std::string success = "success";
for (int wsIndex = 0; wsIndex < nhist; wsIndex++) {
reportProgress(wsIndex, nhist);
auto fit = createChildAlgorithm("Fit");
fit->initialize();
fit->setPropertyValue("Function", funcStr);
fit->setProperty("InputWorkspace", ws);
fit->setProperty("WorkspaceIndex", wsIndex);
fit->setProperty("CreateOutput", true);
fit->setPropertyValue("Output", groupName);
fit->execute();
std::string status = fit->getProperty("OutputStatus");
if (!fit->isExecuted() || status != success) {
error << "Fit failed for spectrum at workspace index " << wsIndex;
error << ": " << status;
throw std::runtime_error(error.str());
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API::MatrixWorkspace_sptr fitOut = fit->getProperty("OutputWorkspace");
resGroup->addWorkspace(fitOut);
API::ITableWorkspace_sptr tab = fit->getProperty("OutputParameters");
// Now we have our fitting results stored in tab
// but we need to extract the relevant information, i.e.
// the detector phases (parameter 'p') and asymmetries ('A')
extractDetectorInfo(tab, resTab, indexInfo.spectrumNumber(wsIndex));
}
/** Extracts detector asymmetries and phases from fitting results
* and adds a new row to the results table with them
* @param paramTab :: [input] Output parameter table resulting from the fit
* @param resultsTab :: [input] Results table to update with a new row
* @param spectrumNumber :: [input] Spectrum number
void CalMuonDetectorPhases::extractDetectorInfo(
const API::ITableWorkspace_sptr ¶mTab,
const API::ITableWorkspace_sptr &resultsTab,
const Indexing::SpectrumNumber spectrumNumber) {
double asym = paramTab->Double(0, 1);
double phase = paramTab->Double(2, 1);
// If asym<0, take the absolute value and add \pi to phase
// f(x) = A * sin( w * x + p) = -A * sin( w * x + p + PI)
if (asym < 0) {
asym = -asym;
phase = phase + M_PI;
// Now convert phases to interval [0, 2PI)
int factor = static_cast<int>(floor(phase / 2 / M_PI));
if (factor) {
phase = phase - factor * 2 * M_PI;
// Copy parameters to new row in results table
API::TableRow row = resultsTab->appendRow();
row << static_cast<int>(spectrumNumber) << asym << phase;
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}
/** Creates the fitting function f(x) = A * sin( w*x + p) + B as string
* Two modes:
* 1) Fixed frequency, no background - for main sequential fit
* 2) Varying frequency, flat background - for finding frequency from asymmetry
* @param freq :: [input] Value for the frequency (w)
* @param fixFreq :: [input] True: fixed frequency, no background. False: varying
* frequency with flat background.
* @returns :: The fitting function as a string
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*/
std::string CalMuonDetectorPhases::createFittingFunction(double freq,
bool fixFreq) {
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// The fitting function is:
// f(x) = A * sin ( w * x + p ) [+ B]
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std::ostringstream ss;
ss << "name=UserFunction,";
if (fixFreq) {
// no background
ss << "Formula=A*sin(w*x+p),";
} else {
// flat background
ss << "Formula=A*sin(w*x+p)+B,";
ss << "B=0.5,";
}
ss << "A=0.5,";
ss << "w=" << freq << ",";
ss << "p=0.5;";
if (fixFreq) {
// w is shared across workspaces
ss << "ties=(f0.w=" << freq << ")";
}
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return ss.str();
}
/** Extracts relevant data from a workspace
* @param startTime :: [input] First X value to consider
* @param endTime :: [input] Last X value to consider
* @return :: Pre-processed workspace to fit
*/
API::MatrixWorkspace_sptr
CalMuonDetectorPhases::extractDataFromWorkspace(double startTime,
double endTime) {
// Extract counts from startTime to endTime
API::IAlgorithm_sptr crop = createChildAlgorithm("CropWorkspace");
crop->setProperty("InputWorkspace", m_inputWS);
crop->setProperty("XMin", startTime);
crop->setProperty("XMax", endTime);
crop->executeAsChildAlg();
boost::shared_ptr<API::MatrixWorkspace> wsCrop =
crop->getProperty("OutputWorkspace");
/**
* Removes exponential decay from a workspace
* @param wsInput :: [input] Workspace to work on
* @return :: Workspace with decay removed
*/
API::MatrixWorkspace_sptr CalMuonDetectorPhases::removeExpDecay(
const API::MatrixWorkspace_sptr &wsInput) {
API::IAlgorithm_sptr remove = createChildAlgorithm("RemoveExpDecay");
remove->setProperty("InputWorkspace", wsInput);
remove->executeAsChildAlg();
API::MatrixWorkspace_sptr wsRem = remove->getProperty("OutputWorkspace");
* Returns the frequency hint to use as a starting point for finding the
* frequency.
* If user has provided a frequency (MHz) as input, use that converted to
* Mrad/s.
* Otherwise, use 2*pi*g_mu*(sample_magn_field).
* (2*pi to convert MHz to Mrad/s)
* @return :: Frequency hint to use in Mrad/s
double CalMuonDetectorPhases::getFrequencyHint() const {
double freq = getProperty("Frequency");
if (freq == EMPTY_DBL()) {
try {
// Read sample_magn_field from workspace logs
freq = m_inputWS->run().getLogAsSingleValue("sample_magn_field");
// Multiply by muon gyromagnetic ratio: 0.01355 MHz/G
freq *= PhysicalConstants::MuonGyromagneticRatio;
} catch (...) {
throw std::runtime_error(
"Couldn't read sample_magn_field. Please provide a value for "
"the frequency");
}
}
// Convert from MHz to Mrad/s
freq *= 2 * M_PI;
return freq;
}
/**
* Returns the frequency to use in the sequential fit.
*
* Finds this by grouping the spectra and calculating the asymmetry, then
* fitting this to get the frequency.
* The starting value for this fit is taken from the frequency hint or logs.
* @param ws :: [input] Pointer to cropped workspace with exp decay removed
* @return :: Fixed frequency value to use in the sequential fit
*/
double
CalMuonDetectorPhases::getFrequency(const API::MatrixWorkspace_sptr &ws) {
std::vector<int> forward = getProperty("ForwardSpectra");
std::vector<int> backward = getProperty("BackwardSpectra");
// If grouping not provided, read it from the instrument
if (forward.empty() || backward.empty()) {
getGroupingFromInstrument(ws, forward, backward);
}
// Calculate asymmetry
const double alpha = getAlpha(ws, forward, backward);
const API::MatrixWorkspace_sptr wsAsym =
getAsymmetry(ws, forward, backward, alpha);
// Fit an oscillating function, allowing frequency to vary
double frequency = fitFrequencyFromAsymmetry(wsAsym);
return frequency;
}
/**
* If grouping was not provided, find the instrument from the input workspace
* and read the default grouping from its IDF. Returns the forward and backward
* groupings as arrays of integers.
* @param ws :: [input] Workspace to find grouping for
* @param forward :: [output] Forward spectrum indices for given instrument
* @param backward :: [output] Backward spectrum indices for given instrument
*/
void CalMuonDetectorPhases::getGroupingFromInstrument(
const API::MatrixWorkspace_sptr &ws, std::vector<int> &forward,
std::vector<int> &backward) {
// make sure both arrays are empty
forward.clear();
backward.clear();
const auto instrument = ws->getInstrument();
auto loader = Kernel::make_unique<API::GroupingLoader>(instrument);
if (instrument->getName() == "MUSR") {
// Two possibilities for grouping - use workspace log
auto fieldDir = ws->run().getLogData("main_field_direction");
if (fieldDir) {
loader = Kernel::make_unique<API::GroupingLoader>(instrument,
fieldDir->value());
}
if (!fieldDir) {
throw std::invalid_argument(
"Cannot use default instrument grouping for MUSR "
"as main field direction is unknown");
}
}
// Load grouping and find forward, backward groups
std::string fwdRange, bwdRange;
const auto grouping = loader->getGroupingFromIDF();
size_t nGroups = grouping->groups.size();
for (size_t iGroup = 0; iGroup < nGroups; iGroup++) {
const std::string name = grouping->groupNames[iGroup];
if (name == "fwd") {
fwdRange = grouping->groups[iGroup];
} else if (name == "bwd" || name == "bkwd") {
bwdRange = grouping->groups[iGroup];
}
}
// Use ArrayProperty's functionality to convert string ranges to groups
this->setProperty("ForwardSpectra", fwdRange);
this->setProperty("BackwardSpectra", bwdRange);
forward = getProperty("ForwardSpectra");
backward = getProperty("BackwardSpectra");
}
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/**
* Get start time for fit
* If not provided as input, try to read from workspace logs.
* If it's not there either, set to 0 and warn user.
* @return :: Start time for fit
*/
double CalMuonDetectorPhases::getStartTime() const {
double startTime = getProperty("FirstGoodData");
if (startTime == EMPTY_DBL()) {
try {
// Read FirstGoodData from workspace logs if possible
double firstGoodData =
m_inputWS->run().getLogAsSingleValue("FirstGoodData");
startTime = firstGoodData;
} catch (...) {
g_log.warning("Couldn't read FirstGoodData, setting to 0");
startTime = 0.;
}
}
return startTime;
}
/**
* Get end time for fit
* If it's not there, use the last available time in the workspace.
* @return :: End time for fit
*/
double CalMuonDetectorPhases::getEndTime() const {
double endTime = getProperty("LastGoodData");
if (endTime == EMPTY_DBL()) {
// Last available time
endTime = m_inputWS->readX(0).back();
}
return endTime;
}
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/**
* Calculate alpha (detector efficiency) from the given workspace
* If calculation fails, returns default 1.0
* @param ws :: [input] Workspace to calculate alpha from
* @param forward :: [input] Forward group spectra numbers
* @param backward :: [input] Backward group spectra numbers
* @return :: Alpha, or 1.0 if calculation failed
*/
double CalMuonDetectorPhases::getAlpha(const API::MatrixWorkspace_sptr &ws,
const std::vector<int> &forward,
const std::vector<int> &backward) {
double alpha = 1.0;
try {
auto alphaAlg = createChildAlgorithm("AlphaCalc");
alphaAlg->setProperty("InputWorkspace", ws);
alphaAlg->setProperty("ForwardSpectra", forward);
alphaAlg->setProperty("BackwardSpectra", backward);
alphaAlg->executeAsChildAlg();
alpha = alphaAlg->getProperty("Alpha");
} catch (const std::exception &e) {
// Eat the error and return default 1.0 so algorithm can continue.
// Warn the user that calculating alpha failed
std::ostringstream message;
message << "Calculating alpha failed, default to 1.0: " << e.what();
g_log.error(message.str());
}
return alpha;
}
/**
* Calculate asymmetry for the given workspace
* @param ws :: [input] Workspace to calculate asymmetry from
* @param forward :: [input] Forward group spectra numbers
* @param backward :: [input] Backward group spectra numbers
* @param alpha :: [input] Detector efficiency
* @return :: Asymmetry for workspace
*/
API::MatrixWorkspace_sptr CalMuonDetectorPhases::getAsymmetry(
const API::MatrixWorkspace_sptr &ws, const std::vector<int> &forward,
const std::vector<int> &backward, const double alpha) {
auto alg = createChildAlgorithm("AsymmetryCalc");
alg->setProperty("InputWorkspace", ws);
alg->setProperty("OutputWorkspace", "__NotUsed");
alg->setProperty("ForwardSpectra", forward);
alg->setProperty("BackwardSpectra", backward);
alg->setProperty("Alpha", alpha);
alg->executeAsChildAlg();
API::MatrixWorkspace_sptr wsAsym = alg->getProperty("OutputWorkspace");
return wsAsym;
}
/**
* Fit the asymmetry and return the frequency found.
* Starting value for the frequency is taken from the hint.
* If the fit fails, return the initial hint.
* @param wsAsym :: [input] Workspace with asymmetry to fit
* @return :: Frequency found from fit
*/
double CalMuonDetectorPhases::fitFrequencyFromAsymmetry(
const API::MatrixWorkspace_sptr &wsAsym) {
// Starting value for frequency is hint
double hint = getFrequencyHint();
std::string funcStr = createFittingFunction(hint, false);
double frequency = hint;
std::string fitStatus = "success";
try {
auto func = API::FunctionFactory::Instance().createInitialized(funcStr);
auto fit = createChildAlgorithm("Fit");
fit->setProperty("Function", func);
fit->setProperty("InputWorkspace", wsAsym);
fit->setProperty("WorkspaceIndex", 0);
fit->setProperty("CreateOutput", true);
fit->setProperty("OutputParametersOnly", true);
fit->setProperty("Output", "__Invisible");
fit->executeAsChildAlg();
fitStatus = fit->getPropertyValue("OutputStatus");
if (fitStatus == "success") {
API::ITableWorkspace_sptr params = fit->getProperty("OutputParameters");
const size_t rows = params->rowCount();
static size_t colName(0), colValue(1);
for (size_t iRow = 0; iRow < rows; iRow++) {
if (params->cell<std::string>(iRow, colName) == "w") {
frequency = params->cell<double>(iRow, colValue);
break;
}
}
}
} catch (const std::exception &e) {
// Report fit failure to user
fitStatus = e.what();
}
if (fitStatus != "success") { // Either failed, or threw an exception
std::ostringstream message;
message << "Fit failed (" << fitStatus << "), using omega hint = " << hint;
g_log.error(message.str());
}
return frequency;
}
* Updates the algorithm progress
* @param thisSpectrum :: [input] Spectrum number currently being fitted
* @param totalSpectra :: [input] Total number of spectra to fit
void CalMuonDetectorPhases::reportProgress(const int thisSpectrum,
const int totalSpectra) {
double proportionDone = (double)thisSpectrum / (double)totalSpectra;
std::ostringstream progMessage;
progMessage << "Fitting " << thisSpectrum + 1 << " of " << totalSpectra;
this->progress(proportionDone, progMessage.str());
} // namespace Algorithms
} // namespace Mantid