本文整理汇总了C++中api::MatrixWorkspace_sptr::indexInfo方法的典型用法代码示例。如果您正苦于以下问题：C++ MatrixWorkspace_sptr::indexInfo方法的具体用法？C++ MatrixWorkspace_sptr::indexInfo怎么用？C++ MatrixWorkspace_sptr::indexInfo使用的例子？那么, 这里精选的方法代码示例或许可以为您提供帮助。您也可以进一步了解该方法所在类api::MatrixWorkspace_sptr的用法示例。
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示例1: fitWorkspace
/** 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
*/
void CalMuonDetectorPhases::fitWorkspace(const API::MatrixWorkspace_sptr &ws,
double freq, std::string groupName,
API::ITableWorkspace_sptr resTab,
API::WorkspaceGroup_sptr &resGroup) {
int nhist = static_cast<int>(ws->getNumberHistograms());
// 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);
const auto &yValues = ws->y(wsIndex);
auto emptySpectrum = std::all_of(yValues.begin(), yValues.end(),
[](double value) { return value == 0.; });
if (emptySpectrum) {
g_log.warning("Spectrum " + std::to_string(wsIndex) + " is empty");
TableWorkspace_sptr tab = boost::make_shared<TableWorkspace>();
tab->addColumn("str", "Name");
tab->addColumn("double", "Value");
tab->addColumn("double", "Error");
for (int j = 0; j < 4; j++) {
API::TableRow row = tab->appendRow();
if (j == PHASE_ROW) {
row << "dummy" << 0.0 << 0.0;
} else {
row << "dummy" << ASYMM_ERROR << 0.0;
}
}
extractDetectorInfo(*tab, *resTab, indexInfo.spectrumNumber(wsIndex));
} else {
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()) {
std::ostringstream error;
error << "Fit failed for spectrum at workspace index " << wsIndex;
error << ": " << status;
throw std::runtime_error(error.str());
} else if (status != success) {
g_log.warning("Fit failed for spectrum at workspace index " +
std::to_string(wsIndex) + ": " + status);
}
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));
}
}
}