NCEPLIBS-ip 5.2.0
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Spectrally interpolate scalars to Mercator. More...
Go to the source code of this file.
Functions/Subroutines | |
subroutine | sptrunm (iromb, maxwv, idrti, imaxi, jmaxi, kmax, mi, mj, iprime, iskipi, jskipi, kskipi, kgskip, niskip, njskip, jcpu, rlat1, rlon1, dlat, dlon, gridi, gm) |
This subprogram spectrally truncates scalar fields on a global cylindrical grid, returning the fields to a Mercator grid. | |
subroutine sptrunm | ( | iromb, | |
maxwv, | |||
idrti, | |||
imaxi, | |||
jmaxi, | |||
kmax, | |||
mi, | |||
mj, | |||
iprime, | |||
iskipi, | |||
jskipi, | |||
kskipi, | |||
kgskip, | |||
niskip, | |||
njskip, | |||
jcpu, | |||
rlat1, | |||
rlon1, | |||
dlat, | |||
dlon, | |||
real, dimension(*) | gridi, | ||
real, dimension(*) | gm | ||
) |
This subprogram spectrally truncates scalar fields on a global cylindrical grid, returning the fields to a Mercator grid.
The wave-space can be either triangular or rhomboidal. The grid-space can be either an equally-spaced grid (with or without pole points) or a Gaussian grid. The grid fields may have general indexing. The transforms are all multiprocessed. Transform several fields at a time to improve vectorization. Subprogram can be called from a multiprocessing environment.
IROMB | - INTEGER SPECTRAL DOMAIN SHAPE (0 FOR TRIANGULAR, 1 FOR RHOMBOIDAL) |
MAXWV | - INTEGER SPECTRAL TRUNCATION |
IDRTI | - INTEGER INPUT GRID IDENTIFIER (IDRTI=4 FOR GAUSSIAN GRID, IDRTI=0 FOR EQUALLY-SPACED GRID INCLUDING POLES, IDRTI=256 FOR EQUALLY-SPACED GRID EXCLUDING POLES) |
IMAXI | - INTEGER EVEN NUMBER OF INPUT LONGITUDES. |
JMAXI | - INTEGER NUMBER OF INPUT LATITUDES. |
KMAX | - INTEGER NUMBER OF FIELDS TO TRANSFORM. |
MI | - INTEGER NUMBER OF POINTS IN THE FASTER ZONAL DIRECTION |
MJ | - INTEGER NUMBER OF POINTS IN THE SLOWER MERID DIRECTION |
IPRIME | - INTEGER INPUT LONGITUDE INDEX FOR THE PRIME MERIDIAN. (DEFAULTS TO 1 IF IPRIME=0) (OUTPUT LONGITUDE INDEX FOR PRIME MERIDIAN ASSUMED 1.) |
ISKIPI | - INTEGER SKIP NUMBER BETWEEN INPUT LONGITUDES (DEFAULTS TO 1 IF ISKIPI=0) |
JSKIPI | - INTEGER SKIP NUMBER BETWEEN INPUT LATITUDES FROM SOUTH (DEFAULTS TO -IMAXI IF JSKIPI=0) |
KSKIPI | - INTEGER SKIP NUMBER BETWEEN INPUT GRID FIELDS (DEFAULTS TO IMAXI*JMAXI IF KSKIPI=0) |
KGSKIP | - INTEGER SKIP NUMBER BETWEEN GRID FIELDS (DEFAULTS TO NPS*NPS IF KGSKIP=0) |
NISKIP | - INTEGER SKIP NUMBER BETWEEN GRID I-POINTS (DEFAULTS TO 1 IF NISKIP=0) |
NJSKIP | - INTEGER SKIP NUMBER BETWEEN GRID J-POINTS (DEFAULTS TO NPS IF NJSKIP=0) |
JCPU | - INTEGER NUMBER OF CPUS OVER WHICH TO MULTIPROCESS (DEFAULTS TO ENVIRONMENT NCPUS IF JCPU=0) |
RLAT1 | - REAL LATITUDE OF THE FIRST GRID POINT IN DEGREES |
RLON1 | - REAL LONGITUDE OF THE FIRST GRID POINT IN DEGREES |
DLAT | - REAL LATITUDE INCREMENT IN DEGREES SUCH THAT D(PHI)/D(J)=DLAT*COS(PHI) WHERE J IS MERIDIONAL INDEX. DLAT IS NEGATIVE FOR GRIDS INDEXED SOUTHWARD. (IN TERMS OF GRID INCREMENT DY VALID AT LATITUDE RLATI, THE LATITUDE INCREMENT DLAT IS DETERMINED AS DLAT=DPR*DY/(RERTH*COS(RLATI/DPR)) WHERE DPR=180/PI AND RERTH IS EARTH'S RADIUS) |
DLON | - REAL LONGITUDE INCREMENT IN DEGREES SUCH THAT D(LAMBDA)/D(I)=DLON WHERE I IS ZONAL INDEX. DLON IS NEGATIVE FOR GRIDS INDEXED WESTWARD. |
GRIDI | - REAL (*) INPUT GRID FIELDS |
GM | - REAL (*) MERCATOR FIELDS |
SUBPROGRAMS CALLED:
MINIMUM GRID DIMENSIONS FOR UNALIASED TRANSFORMS TO SPECTRAL:
DIMENSION | LINEAR | QUADRATIC |
---|---|---|
IMAX | 2*MAXWV+2 | 3*MAXWV/2*2+2 |
JMAX (IDRT=4,IROMB=0) | 1*MAXWV+1 | 3*MAXWV/2+1 |
JMAX (IDRT=4,IROMB=1) | 2*MAXWV+1 | 5*MAXWV/2+1 |
JMAX (IDRT=0,IROMB=0) | 2*MAXWV+3 | 3*MAXWV/2*2+3 |
JMAX (IDRT=0,IROMB=1) | 4*MAXWV+3 | 5*MAXWV/2*2+3 |
JMAX (IDRT=256,IROMB=0) | 2*MAXWV+1 | 3*MAXWV/2*2+1 |
JMAX (IDRT=256,IROMB=1) | 4*MAXWV+1 | 5*MAXWV/2*2+1 |
Definition at line 76 of file sptrunm.f.
References ncpus(), sptgpm(), and sptran().
Referenced by spectral_interp_mod::polates4::polates4_grib1(), and spectral_interp_mod::polates4::polates4_grib2().