mxlib
c++ tools for analyzing astronomical data and other tasks by Jared R. Males. [git repo]
aoConstants.hpp File Reference

Calculate and provide constants related to adaptive optics. More...

Calculate and provide constants related to adaptive optics.

Author
Jared R. Males (jared.nosp@m.male.nosp@m.s@gma.nosp@m.il.c.nosp@m.om)

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...
 

Function Documentation

◆ calcConstants()

template<typename floatT >
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().