cloudy trunk
|
Data Fields | |
string | name |
bool | lgIsTeffLoggGrid |
access_scheme | scheme |
FILE * | ioIN |
const char * | ident |
const char * | command |
IntMode | imode |
int32 | ndim |
int32 | npar |
int32 | nmods |
int32 | ngrid |
uint32 | nOffset |
uint32 | nBlocksize |
mpp * | telg |
double ** | val |
long * | nval |
long * | jlo |
long * | jhi |
char | names [MDIM][MNAM+1] |
long * | trackLen |
long | nTracks |
long * | jval |
- why was it necessary to change stars_tlusty.in? (change from r43 to r50?)
- check all interpolation modes of CoStar
- compare models with original code, dump atmospheres!
- check all Edges arrays...
- update Doxygen documentation
store all the relevant information on a binary atmosphere file
const char* stellar_grid::command |
const char* stellar_grid::ident |
IntMode stellar_grid::imode |
long* stellar_grid::jlo |
jlo/jhi will hold indices into the binary model file: jlo/jhi(i,...,n) will point to the model with parameters val[0][i],...,val[ndim-1][n], or its closest approximation in log(g) in case the model doesn't exist and lgIsTeffLoggGrid is true. jlo will hold the model with the highest log(g) <= than requested jhi will hold the model with the lowest log(g) >= than requested in case no suitable model could be found either array will hold -2
long* stellar_grid::jval |
jval will hold indices into the CoStar grid: jval(nModels,nTracks)
bool stellar_grid::lgIsTeffLoggGrid |
string stellar_grid::name |
uint32 stellar_grid::nBlocksize |
int32 stellar_grid::ndim |
int32 stellar_grid::ngrid |
int32 stellar_grid::nmods |
uint32 stellar_grid::nOffset |
int32 stellar_grid::npar |
long stellar_grid::nTracks |
long* stellar_grid::nval |
access_scheme stellar_grid::scheme |
mpp* stellar_grid::telg |
long* stellar_grid::trackLen |
double** stellar_grid::val |