Function lupnt::DensityHarrisPriester¶

Defined in File forces.h

Function Documentation¶

Real lupnt::DensityHarrisPriester(Real mjd_tt, const Vec3 &r_tod)¶

Computes the atmospheric density using the Harris-Priester model.

Parameters:

mjd_tt – Modified Julian Date (Terrestrial Time).
r_tod – Position vector in the true of date frame.

Returns:

Real Atmospheric density.