|
| | bicubic_interp_mod.F90 |
| | Bicubic interpolation routines for scalars and vectors.
|
| |
| | bilinear_interp_mod.F90 |
| | Bilinear interpolation routines for scalars and vectors.
|
| |
| | budget_interp_mod.F90 |
| | Budget interpolation routines for scalars and vectors.
|
| |
| | earth_radius_mod.F90 |
| | Determine earth radius and shape.
|
| |
| | fftpack.F |
| | A concatenation of several subroutines from the FFTPACK collection.
|
| |
| | gdswzd_c.F90 |
| | C wrapper for routine gdswzd().
|
| |
| | gdswzd_mod.F90 |
| | Driver module for gdswzd routines.
|
| |
| | ip_constants_mod.F90 |
| | Constants for use in NCEPLIBS-ip.
|
| |
| | ip_equid_cylind_grid_mod.F90 |
| | Equidistant cylindrical grib decoder and grid coordinate transformations.
|
| |
| | ip_gaussian_grid_mod.F90 |
| | Gaussian grid coordinate transformations.
|
| |
| | ip_grid_descriptor_mod.F90 |
| | Users derived type grid descriptor objects to abstract away the raw GRIB1 and GRIB2 grid definitions.
|
| |
| | ip_grid_factory_mod.F90 |
| | Routines for creating an ip_grid given a Grib descriptor.
|
| |
| | ip_grid_mod.F90 |
| | Abstract ip_grid type.
|
| |
| | ip_grids_mod.F90 |
| | Re-export the individual grids.
|
| |
| | ip_interpolators_mod.F90 |
| | Top-level module to export interpolation routines and constants.
|
| |
| | ip_lambert_conf_grid_mod.F90 |
| | GDS wizard for lambert conformal conical.
|
| |
| | ip_mercator_grid_mod.F90 |
| | GDS wizard for mercator cylindrical.
|
| |
| | ip_mod.F90 |
| | Top-level module for the ip library.
|
| |
| | ip_polar_stereo_grid_mod.F90 |
| | GDS wizard for polar stereographic azimuthal.
|
| |
| | ip_rot_equid_cylind_egrid_mod.F90 |
| | Rotated equidistant cylindrical GRIB decoder and grid coordinate transformations for Arakawa grid E.
|
| |
| | ip_rot_equid_cylind_grid_mod.F90 |
| | Rotated equidistant cylindrical GRIB decoder and grid coordinate transformations for Arakawa grids A through D.
|
| |
| | ip_station_points_grid_mod.F90 |
| | Interpolate gridded data to a series of station points.
|
| |
| | iplib_4.h |
| | C interface to gdswzd() and gdswzd_grib1() functions for '4' library build.
|
| |
| | iplib_8.h |
| | C interface to gdswzd() and gdswzd_grib1() functions for '8' library build.
|
| |
| | iplib_d.h |
| | C interface to gdswzd() and gdswzd_grib1() functions for 'd' library build.
|
| |
| | ipolates.F90 |
| | Top-level driver for scalar interpolation routine ipolates().
|
| |
| | ipolatev.F90 |
| | Top-level driver for vector interpolation routine ipolates.
|
| |
| | ipxetas.F90 |
| | Expand or contract eta grids using linear interpolation.
|
| |
| | ipxwafs.F90 |
| | Expand or contract wafs grids.
|
| |
| | ipxwafs2.F90 |
| | Expand or contract wafs grids using linear interpolation and account for bitmapped data.
|
| |
| | ipxwafs3.F90 |
| | Expand or contract wafs grids using neighbor interpolation and accout for bitmapped data.
|
| |
| | movect.F90 |
| | Move a vector along a great circle.
|
| |
| | ncpus.F |
| | Set number of cpus.
|
| |
| | neighbor_budget_interp_mod.F90 |
| | Interpolate scalar and vector fields with neighbor budget interpolation.
|
| |
| | neighbor_interp_mod.F90 |
| | Interpolate scalar and vector fields with neighbor interpolation.
|
| |
| | polfix_mod.F90 |
| | Make multiple pole scalar values consistent.
|
| |
| | sp_mod.F |
| |
| | spanaly.f |
| | Analyze spectral from Fourier.
|
| |
| | spdz2uv.f |
| | Compute winds from divergence and vorticity.
|
| |
| | spectral_interp_mod.F90 |
| | Interpolate spectral.
|
| |
| | speps.f |
| | Compute utility spectral fields.
|
| |
| | spfft.f |
| | Perform multiple fast fourier transforms.
|
| |
| | spfft1.f |
| | Perform multiple fast Fourier transforms.
|
| |
| | spffte.f |
| | Perform multiple fast Fourier transforms.
|
| |
| | spfftpt.f |
| | Compute fourier transform to gridpoints.
|
| |
| | spgradq.f |
| | Compute gradient in spectral space.
|
| |
| | spgradx.f |
| | Compute x-gradient in Fourier space.
|
| |
| | spgrady.f |
| | Compute y-gradient in spectral space.
|
| |
| | splaplac.f |
| | Compute laplacian in spectral space.
|
| |
| | splat.F |
| | Computes cosines of colatitude and Gaussian weights for sets of latitudes.
|
| |
| | splegend.f |
| | Compute Legendre polynomials.
|
| |
| | sppad.f |
| | Pad or truncate a spectral field.
|
| |
| | spsynth.f |
| | Synthesize Fourier coefficients from spectral coefficients.
|
| |
| | sptez.f |
| | Perform a simple scalar spherical transform.
|
| |
| | sptezd.f |
| | Perform a simple gradient spherical transform.
|
| |
| | sptezm.f |
| | Perform simple scalar spherical transforms.
|
| |
| | sptezmd.f |
| | Perform simple gradient spherical transforms.
|
| |
| | sptezmv.f |
| | Perform simple vector spherical transforms.
|
| |
| | sptezv.f |
| | Perform a simple vector spherical transform.
|
| |
| | sptgpm.f |
| | Transform spectral scalar to Mercator.
|
| |
| | sptgpmd.f |
| | Transform spectral to Mercator gradients.
|
| |
| | sptgpmv.f |
| | Transform spectral vector to Mercator.
|
| |
| | sptgps.f |
| | Transform spectral scalar to polar stereo.
|
| |
| | sptgpsd.f |
| | Transform spectral to polar stereographic gradients.
|
| |
| | sptgpsv.f |
| | Transform spectral vector to polar stereo.
|
| |
| | sptgpt.f |
| | Transform spectral scalar to station points.
|
| |
| | sptgptd.f |
| | Transform spectral to station point gradients.
|
| |
| | sptgptsd.f |
| | Transform spectral scalar to station points.
|
| |
| | sptgptv.f |
| | Transform spectral vector to station points.
|
| |
| | sptgptvd.f |
| | Transform spectral vector to station points.
|
| |
| | sptran.f |
| | Perform a scalar spherical transform.
|
| |
| | sptrand.f |
| | Perform a gradient spherical transform.
|
| |
| | sptranf.f |
| | Perform a scalar spherical transform.
|
| |
| | sptranf0.f |
| | Sptranf spectral initialization.
|
| |
| | sptranf1.f |
| | Sptranf spectral transform.
|
| |
| | sptranfv.f |
| | Perform a vector spherical transform.
|
| |
| | sptranv.f |
| | Perform a vector spherical transform.
|
| |
| | sptrun.f |
| | Truncate gridded scalar fields.
|
| |
| | sptrund.f |
| | Spectrally truncate to gradients.
|
| |
| | sptrung.f |
| | Spectrally interpolate scalars to stations.
|
| |
| | sptrungv.f |
| | Spectrally interpolate vectors to stations.
|
| |
| | sptrunl.f |
| | Spectrally truncate to laplacian.
|
| |
| | sptrunm.f |
| | Spectrally interpolate scalars to Mercator.
|
| |
| | sptrunmv.f |
| | Spectrally interpolate vectors to Mercator.
|
| |
| | sptruns.f |
| | Spectrally interpolate scalars to polar stereo.
|
| |
| | sptrunsv.f |
| | Spectrally interpolate vectors to polar stereo.
|
| |
| | sptrunv.f |
| | Spectrally truncate gridded vector fields.
|
| |
| | spuv2dz.f |
| | Compute divergence and vorticity from winds.
|
| |
| | spvar.f |
| | Compute variance by total wavenumber.
|
| |
| | spwget.f |
| | Get wave-space constants.
|
| |
1.13.2 
