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BornAgain
1.19.0
Simulate and fit neutron and x-ray scattering at grazing incidence
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Scan type with inclination angles as coordinate values and a unique wavelength. More...
Inheritance diagram for AngularSpecScan:Public Member Functions | |
| AngularSpecScan (double wl, const IAxis &inc_angle) | |
| AngularSpecScan (double wl, int nbins, double alpha_i_min, double alpha_i_max) | |
| Sets angle-defined specular scan. More... | |
| AngularSpecScan (double wl, std::vector< double > inc_angle) | |
| AngularSpecScan * | clone () const override |
| void | setAbsoluteAngularResolution (const IRangedDistribution &distr, const std::vector< double > &std_dev) |
| Sets angular resolution values via IRangedDistribution and values of standard deviations. More... | |
| void | setAbsoluteAngularResolution (const IRangedDistribution &distr, double std_dev) |
| void | setAbsoluteWavelengthResolution (const IRangedDistribution &distr, const std::vector< double > &std_dev) |
| Sets wavelength resolution values via IRangedDistribution and values of standard deviations. More... | |
| void | setAbsoluteWavelengthResolution (const IRangedDistribution &distr, double std_dev) |
| void | setAngleResolution (const ScanResolution &resolution) |
| Sets angle resolution values via ScanResolution object. | |
| void | setFootprintFactor (const IFootprintFactor *f_factor) |
| Sets footprint correction factor. | |
| void | setRelativeAngularResolution (const IRangedDistribution &distr, const std::vector< double > &rel_dev) |
| Sets angular resolution values via IRangedDistribution and values of relative deviations (that is, rel_dev equals standard deviation divided by the mean value). More... | |
| void | setRelativeAngularResolution (const IRangedDistribution &distr, double rel_dev) |
| void | setRelativeWavelengthResolution (const IRangedDistribution &distr, const std::vector< double > &rel_dev) |
| Sets wavelength resolution values via IRangedDistribution and values of relative deviations (that is, rel_dev equals standard deviation divided by the mean value). More... | |
| void | setRelativeWavelengthResolution (const IRangedDistribution &distr, double rel_dev) |
| void | setWavelengthResolution (const ScanResolution &resolution) |
| Sets wavelength resolution values via ScanResolution object. | |
Scan type with inclination angles as coordinate values and a unique wavelength.
Features footprint correction.
| AngularSpecScan::AngularSpecScan | ( | double | wl, |
| int | nbins, | ||
| double | alpha_i_min, | ||
| double | alpha_i_max | ||
| ) |
Sets angle-defined specular scan.
The first parameter is always a wavelength in nm. Second parameter is either a numpy array of incident angles in radians or an IAxis object with angle values. Alternatively an axis can be defined in-place, then the second passed parameter is the number of bins, third - minimum on-axis angle value, fourth - maximum on-axis angle value.
| void AngularSpecScan::setAbsoluteAngularResolution | ( | const IRangedDistribution & | distr, |
| const std::vector< double > & | std_dev | ||
| ) |
Sets angular resolution values via IRangedDistribution and values of standard deviations.
std_dev can be either single-valued or a numpy array. In the latter case the length of the array should coinside with the length of the inclination angle axis.
| void AngularSpecScan::setAbsoluteWavelengthResolution | ( | const IRangedDistribution & | distr, |
| const std::vector< double > & | std_dev | ||
| ) |
Sets wavelength resolution values via IRangedDistribution and values of standard deviations.
std_dev can be either single-valued or a numpy array. In the latter case the length of the array should coinside with the length of the inclination angle axis.
| void AngularSpecScan::setRelativeAngularResolution | ( | const IRangedDistribution & | distr, |
| const std::vector< double > & | rel_dev | ||
| ) |
Sets angular resolution values via IRangedDistribution and values of relative deviations (that is, rel_dev equals standard deviation divided by the mean value).
rel_dev can be either single-valued or a numpy array. In the latter case the length of the array should coinside with the length of the inclination angle axis.
| void AngularSpecScan::setRelativeWavelengthResolution | ( | const IRangedDistribution & | distr, |
| const std::vector< double > & | rel_dev | ||
| ) |
Sets wavelength resolution values via IRangedDistribution and values of relative deviations (that is, rel_dev equals standard deviation divided by the mean value).
rel_dev can be either single-valued or a numpy array. In the latter case the length of the array should coinside with the length of the inclination angle axis.