NCEPLIBS-ip
5.1.0
|
Files | |
file | bicubic_interp_mod.F90 [code] |
Bicubic interpolation routines for scalars and vectors. | |
file | bilinear_interp_mod.F90 [code] |
Bilinear interpolation routines for scalars and vectors. | |
file | budget_interp_mod.F90 [code] |
Budget interpolation routines for scalars and vectors. | |
file | earth_radius_mod.F90 [code] |
Determine earth radius and shape. | |
file | fftpack.F [code] |
A concatination of the (FFTPACK)[https://netlib.org/fftpack/] library code. | |
file | gdswzd_c.F90 [code] |
C wrapper for routine gdswzd(). | |
file | gdswzd_mod.F90 [code] |
Driver module for gdswzd routines. | |
file | ip_constants_mod.F90 [code] |
Constants for use in NCEPLIBS-ip. | |
file | ip_equid_cylind_grid_mod.F90 [code] |
Equidistant cylindrical grib decoder and grid coordinate transformations. | |
file | ip_gaussian_grid_mod.F90 [code] |
Gaussian grid coordinate transformations. | |
file | ip_grid_descriptor_mod.F90 [code] |
Users derived type grid descriptor objects to abstract away the raw GRIB1 and GRIB2 grid definitions. | |
file | ip_grid_factory_mod.F90 [code] |
Routines for creating an ip_grid given a Grib descriptor. | |
file | ip_grid_mod.F90 [code] |
Abstract ip_grid type. | |
file | ip_grids_mod.F90 [code] |
Re-export the individual grids. | |
file | ip_interpolators_mod.F90 [code] |
Top-level module to export interpolation routines and constants. | |
file | ip_lambert_conf_grid_mod.F90 [code] |
GDS wizard for lambert conformal conical. | |
file | ip_mercator_grid_mod.F90 [code] |
GDS wizard for mercator cylindrical. | |
file | ip_mod.F90 [code] |
Top-level module for the ip library. | |
file | ip_polar_stereo_grid_mod.F90 [code] |
GDS wizard for polar stereographic azimuthal. | |
file | ip_rot_equid_cylind_egrid_mod.F90 [code] |
Rotated equidistant cylindrical GRIB decoder and grid coordinate transformations for Arakawa grid E. | |
file | ip_rot_equid_cylind_grid_mod.F90 [code] |
Rotated equidistant cylindrical GRIB decoder and grid coordinate transformations for Arakawa grids A through D. | |
file | ip_station_points_grid_mod.F90 [code] |
Interpolate gridded data to a series of station points. | |
file | iplib_4.h [code] |
C interface to gdswzd() and gdswzd_grib1() functions for '4' library build. | |
file | iplib_8.h [code] |
C interface to gdswzd() and gdswzd_grib1() functions for '8' library build. | |
file | iplib_d.h [code] |
C interface to gdswzd() and gdswzd_grib1() functions for 'd' library build. | |
file | ipolates.F90 [code] |
Top-level driver for scalar interpolation routine ipolates(). | |
file | ipolatev.F90 [code] |
Top-level driver for vector interpolation routine ipolates. | |
file | ipxetas.F90 [code] |
Expand or contract eta grids using linear interpolation. | |
file | ipxwafs.F90 [code] |
Expand or contract wafs grids. | |
file | ipxwafs2.F90 [code] |
Expand or contract wafs grids using linear interpolation and account for bitmapped data. | |
file | ipxwafs3.F90 [code] |
Expand or contract wafs grids using neighbor interpolation and accout for bitmapped data. | |
file | movect.F90 [code] |
Move a vector along a great circle. | |
file | ncpus.F [code] |
Set number of cpus. | |
file | neighbor_budget_interp_mod.F90 [code] |
Interpolate scalar and vector fields with neighbor budget interpolation. | |
file | neighbor_interp_mod.F90 [code] |
Interpolate scalar and vector fields with neighbor interpolation. | |
file | polfix_mod.F90 [code] |
Make multiple pole scalar values consistent. | |
file | spanaly.f [code] |
Analyze spectral from Fourier. | |
file | spdz2uv.f [code] |
Compute winds from divergence and vorticity. | |
file | spectral_interp_mod.F90 [code] |
Interpolate spectral. | |
file | speps.f [code] |
Compute utility spectral fields. | |
file | spfft.f [code] |
Perform multiple fast fourier transforms. | |
file | spfft1.f [code] |
Perform multiple fast Fourier transforms. | |
file | spffte.f [code] |
Perform multiple fast Fourier transforms. | |
file | spfftpt.f [code] |
Compute fourier transform to gridpoints. | |
file | spgradq.f [code] |
Compute gradient in spectral space. | |
file | spgradx.f [code] |
Compute x-gradient in Fourier space. | |
file | spgrady.f [code] |
Compute y-gradient in spectral space. | |
file | splaplac.f [code] |
Compute laplacian in spectral space. | |
file | splat.F [code] |
Computes cosines of colatitude and Gaussian weights for sets of latitudes. | |
file | splegend.f [code] |
Compute Legendre polynomials. | |
file | sppad.f [code] |
Pad or truncate a spectral field. | |
file | spsynth.f [code] |
Synthesize Fourier coefficients from spectral coefficients. | |
file | sptez.f [code] |
Perform a simple scalar spherical transform. | |
file | sptezd.f [code] |
Perform a simple gradient spherical transform. | |
file | sptezm.f [code] |
Perform simple scalar spherical transforms. | |
file | sptezmd.f [code] |
Perform simple gradient spherical transforms. | |
file | sptezmv.f [code] |
Perform simple vector spherical transforms. | |
file | sptezv.f [code] |
Perform a simple vector spherical transform. | |
file | sptgpm.f [code] |
Transform spectral scalar to Mercator. | |
file | sptgpmd.f [code] |
Transform spectral to Mercator gradients. | |
file | sptgpmv.f [code] |
Transform spectral vector to Mercator. | |
file | sptgps.f [code] |
Transform spectral scalar to polar stereo. | |
file | sptgpsd.f [code] |
Transform spectral to polar stereographic gradients. | |
file | sptgpsv.f [code] |
Transform spectral vector to polar stereo. | |
file | sptgpt.f [code] |
Transform spectral scalar to station points. | |
file | sptgptd.f [code] |
Transform spectral to station point gradients. | |
file | sptgptsd.f [code] |
Transform spectral scalar to station points. | |
file | sptgptv.f [code] |
Transform spectral vector to station points. | |
file | sptgptvd.f [code] |
Transform spectral vector to station points. | |
file | sptran.f [code] |
Perform a scalar spherical transform. | |
file | sptrand.f [code] |
Perform a gradient spherical transform. | |
file | sptranf.f [code] |
Perform a scalar spherical transform. | |
file | sptranf0.f [code] |
Sptranf spectral initialization. | |
file | sptranf1.f [code] |
Sptranf spectral transform. | |
file | sptranfv.f [code] |
Perform a vector spherical transform. | |
file | sptranv.f [code] |
Perform a vector spherical transform. | |
file | sptrun.f [code] |
Truncate gridded scalar fields. | |
file | sptrund.f [code] |
Spectrally truncate to gradients. | |
file | sptrung.f [code] |
Spectrally interpolate scalars to stations. | |
file | sptrungv.f [code] |
Spectrally interpolate vectors to stations. | |
file | sptrunl.f [code] |
Spectrally truncate to laplacian. | |
file | sptrunm.f [code] |
Spectrally interpolate scalars to Mercator. | |
file | sptrunmv.f [code] |
Spectrally interpolate vectors to Mercator. | |
file | sptruns.f [code] |
Spectrally interpolate scalars to polar stereo. | |
file | sptrunsv.f [code] |
Spectrally interpolate vectors to polar stereo. | |
file | sptrunv.f [code] |
Spectrally truncate gridded vector fields. | |
file | spuv2dz.f [code] |
Compute divergence and vorticity from winds. | |
file | spvar.f [code] |
Compute variance by total wavenumber. | |
file | spwget.f [code] |
Get wave-space constants. | |