mxlib
c++ tools for analyzing astronomical data and other tasks by Jared R. Males. [git repo]
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Calculate and provide constants related to adaptive optics. More...
Calculate and provide constants related to adaptive optics.
Definition in file aoConstants.hpp.
Go to the source code of this file.
Namespaces | |
mx | |
The mxlib c++ namespace. | |
Functions | |
template<typename floatT > | |
void | mx::AO::constants::calcConstants (floatT &a_sf, floatT &a_psd) |
Calculate the AO constants. More... | |
template<typename floatT > | |
constexpr floatT | mx::AO::constants::a_SF () |
The scaling constant for the Kolmorogov optical phase structure function. More... | |
template<typename floatT > | |
constexpr floatT | mx::AO::constants::a_PSD () |
The scaling constant for the Kolmorogov optical phase power spectral density. More... | |
void mx::AO::constants::calcConstants | ( | floatT & | a_sf, |
floatT & | a_psd | ||
) |
Calculate the AO constants.
Definition at line 29 of file aoConstants.hpp.
References mx::AO::constants::calcConstants(), and mx::math::pi().
Referenced by mx::AO::constants::calcConstants().