PLUTO
4.4-patch2
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Compute the flux for the (M1) radiation transport equations. More...
#include "pluto.h"
Compute the flux of the conservative radiation transport equations in the direction given by g_dir. This function defines the component of the hyperbolic flux tensor of the standard RHD equations.
In what follows:
VXn
, MXn
are the velocity, momentum components in the direction given by g_dir (normal, "n"
)VXt
, MXt
and VXb
, MXb
are the transverse components (tangent "t"
and bi-tangent "b"
).