PLUTO
4.4-patch2
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#include <structs.h>
Data Fields | |
double ** | v |
double ** | u |
double ** | flux |
double ** | fluxCR |
double ** | lambda |
double ** | Bbck |
double * | prs |
double * | a2 |
double * | cw |
double * | h |
double ** | J |
double ** | cCR |
double ** | Fcr |
double *** | Lp |
double *** | Rp |
The State structure contains one-dimensional vectors of fluid quantities, often used during 1D computations (Riemann solver, sound speed, etc..),
double* a2 |
Array of sound speeds squared
double** Bbck |
Array of background field components
double** cCR |
Cosmic ray velocity times R: cCR = R*u_.
double* cw |
Array of whistler wave speeds
double** Fcr |
Cosmic Rays force (used to copy d->Fcr during directional sweeps)
double** flux |
Array of fluxes
double** fluxCR |
Array of fluxes incudling CR contribution alone
double* h |
Array of enthalpies
double** J |
Array of currents (e.g. Hall-MHD, RRMHD)
double** lambda |
Array of eigenvalues associated to Lp, Rp
double*** Lp |
Left eigenvectors (primitive formulation).
double* prs |
Array of total pressure (see, flux)
double*** Rp |
Right eigenvectors (primitive formulation).
double** u |
Array of conservative variables
double** v |
Array of primitive variables