|
PLUTO
4.0
|
|
PLUTO
4.0
|
#include <mod_defs.h>
Data Fields | |
| double | D |
| double | sigma_c |
| double | E |
| double | m2 |
| double | rho |
| double | W |
| double | lor |
| double | prs |
| double | S |
| double | S2 |
| double | B2 |
The Map_param structure is used to pass input/output arguments during the conversion from conservative to primitive variables operated by the ConsToPrim() function. The output parameter, rho, W, lor and p, must be set at the end of every root-finder routine (EnergySolve(), EntropySolve() and PressureFix()). Additionally, some of the input parameters must be re-computed in EntropySolve() and PressureFix().
The Map_param structure is used to pass input/output arguments during the conversion from conservative to primitive variables operated by the ConsToPrim() function in the relativistic modules (RHD and RMHD). The output parameter, rho, W, lor and p, must be set at the end of every root-finder routine (EnergySolve(), EntropySolve() and PressureFix()). Additionally, some of the input parameters must be re-computed in EntropySolve() and PressureFix().
| double B2 |
Square of magnetic field (input).
| double D |
Lab density (input).
| double E |
Total energy (input).
| double lor |
Lorentz factor (output).
| double m2 |
Square of total momentum (input).
| double prs |
Thermal pressure (output).
| double rho |
proper density (output)
| double S |
m<dot>B (input).
| double S2 |
Square of S (input).
| double sigma_c |
Conserved entropy (input).
| double W |
D*h*lor (output).
1.8.2
