本文整理汇总了C++中dataobjects::Workspace2D_sptr::mutableY方法的典型用法代码示例。如果您正苦于以下问题：C++ Workspace2D_sptr::mutableY方法的具体用法？C++ Workspace2D_sptr::mutableY怎么用？C++ Workspace2D_sptr::mutableY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dataobjects::Workspace2D_sptr的用法示例。
在下文中一共展示了Workspace2D_sptr::mutableY方法的1个代码示例，这些例子默认根据受欢迎程度排序。您可以为喜欢或者感觉有用的代码点赞，您的评价将有助于系统推荐出更棒的C++代码示例。
示例1: store_value
/**
* Convenience function to store a detector value into a given spectrum.
* Note that this type of data doesn't use TOD, so that we use a single dummy
* bin in X. Each detector is defined as a spectrum of length 1.
* @param ws: workspace
* @param specID: ID of the spectrum to store the value in
* @param value: value to store [count]
* @param error: error on the value [count]
* @param wavelength: wavelength value [Angstrom]
* @param dwavelength: error on the wavelength [Angstrom]
*/
void store_value(DataObjects::Workspace2D_sptr ws, int specID, double value,
double error, double wavelength, double dwavelength) {
auto &X = ws->mutableX(specID);
auto &Y = ws->mutableY(specID);
auto &E = ws->mutableE(specID);
// The following is mostly to make Mantid happy by defining a histogram with
// a single bin around the neutron wavelength
X[0] = wavelength - dwavelength / 2.0;
X[1] = wavelength + dwavelength / 2.0;
Y[0] = value;
E[0] = error;
ws->getSpectrum(specID).setSpectrumNo(specID);
}