wgrib2: new_grid
Introduction
The new_grid option interpolates the fields to a new
grid.
The default interpolation is bilinear but that can be changed using the
new_grid_interpolation option. This option uses
scalar and vector interpolation as appropriate. In order for the vector
interpolation to work, the vector quantities must be in a (U,V) order.
For example: Z200, U200, V200, Z500, U500, V500 is good. If the data
are not in (U,V) order, the inventory can be sorted into (U,V) order
and the inventory can then be used to control the order of processing.
If the vector quanties are not in (U,V) order, the vector quantites will
not be interpolated. (See example 3 for converting the file into a (U,V) order.)
The option is not part of the default configuration but it included with many distributions.
The interpolation code is written
in fortran and combining fortran and C code can require some work. (gcc/gfortran and
clang/gfortran are already handled by the makefile.) Getting the C and Fortran code to cooperate
requires some systemspecific knowledge and may not be possible in all cases. Consequently
you are on your own in getting the new_grid option installed.
Operations often has to use the new_grid option to produce a large number
of user grids. Fortunately the interpolation can be made embarrassingly parallel. A
portable singlenode solution is described in here. A
multinode solution is possible using OpenMPI and the wgrib2 library.
Caution
The new_grid option works in raw scan mode, so data are not
converted to sn:we order. Conequently options that only work in sn:we order cannot
work at the same time as the new_grid option. Any option
that uses geolocation (ex. rpn, lon)
is incompatible with new_grid.
Usage
new_grid_winds W new_grid A B C outfile
W = earth or grid
earth means that the U wind goes eastward, V goes northward
grid means that U wind goes from grid (i,j) to (i+1,j)
which is not eastward in a Lambertconformal or polar stereographic grids
A, B, C are the output grid description
outfile is an output file. The grib2 interpolated records are written in outfile
Examples
wgrib2 IN.grb set_grib_type same new_grid_winds earth new_grid latlon 100:10:1 30:20:1 OUT.grb
Interpolates from IN.grb to OUT.grb
Uses the same grib packing as in the input file
Makes a 10x20, 1x1 degree latlon grid, lower left corner: 100E 30N
wgrib2 IN.grb set_grib_type same new_grid_winds earth new_grid ncep grid 221 OUT.grb
Interpolates from IN.grb to OUT.grb
Uses the same grib packing as in the input file
Interpolates to NCEP grid 221.
In this example, U and V are not in the required order.
wgrib2 201201.A  sed e 's/:UGRD:/:UGRDa:/' e 's/:VGRD:/:UGRDb:/'  \
sort t: k3,3 k5,8 k4,4  \
wgrib2 201201.A i new_grid_winds earth new_grid ncep grid 2 201201.A.grd2
The first line creates an inventory with new variable names: UGRD > UGRDa and VGRD > UGRDb
The second line sorts the inventory so that UGRDb follows UGRDB.
The third line regrids the file, with the order of processing controlled by the inventory.
Grid description format
new_grid ncep grid I outfile I = 2,3,98,126129,170,173,221,230,241,249
(NCEP grid defintions)
T62,T126,T170,T190,T254,T382,T574,T1148,T1534
(NCEP Gaussian grids definitions)
Want more ncep grids? Modify ncep_grids.c
new_grid latlon lon0:nlon:dlon lat0:nlat:dlat outfile latlon grid
lat0, lon0 = degrees of lat/lon for 1st grid point
nlon = number of longitudes
nlat = number of latitudes
dlon = grid cell size in degrees of longitude
dlat = grid cell size in degrees of latitude
new_grid lambert:lov:latin1:latin2:lad lon0:nx:dx lat0:ny:dy outfile Lambert conic conformal
new_grid lambert:lov:latin1:latin2 lon0:nx:dx lat0:ny:dy outfile lad = latin2
new_grid lambert:lov:latin1 lon0:nx:dx lat0:ny:dy outfile latin2 = latini lad = latin1
lov = longitude (degrees) where y axis is parallel to meridian
latin1 = first latitude from pole which cuts the secant cone
latin2 = second latitude from pole which cuts the secant cone
lad = latitude (degrees) where dx and dy are specified
lat0, lon0 = degrees of lat/lon for 1st grid point
nx = number of grid points in X direction
ny = number of grid points in Y direction
dx = grid cell size in meters in x direction
dy = grid cell size in meters in y direction
note: if latin2 >= 0, the north pole is on proj plane
if latin2 < 0, the south pole is on proj plane
new_grid lambertc:lov:latin1:latin2:lad lonc:nx:dx latc:ny:dy outfile Lambert conic conformal with centered position
new_grid lambertc:lov:latin1:latin2 lonc:nx:dx latc:ny:dy outfile like lambert except lonc and latc replace lon0 and lat0
new_grid lambertc:lov:latin1 lonc:nx:dx latc:ny:dy outfile latc, lonc = degrees of lat/lon for center of the grid
new_grid nps:lov:lad lon0:nx:dx lat0:ny:dy outfile north polar stereographic
new_grid sps:lov:lad lon0:nx:dx lat0:ny:dy outfile south polar stereographic
lov = longitude (degrees) where y axis is parallel to meridian
lad = latitude (degrees) where dx and dy are specified
note: grib1 uses lad = 60N (nps) or 60S (sps)
lad must be 60 (nps) or 60 (sps) (library limitation)
lat0, lon0 = degrees of lat/lon for 1st grid point
nx = number of grid points in X direction
ny = number of grid points in Y direction
dx = grid cell distance meters in x direction at lad
dy = grid cell distance meters in y direction at lad
new_grid gaussian lon0:nx:dlon lat0:ny outfile global Gaussian grids
lat0, lon0 = degrees of lat/lon for 1st grid point
note: lon1 = lon0, lat1 = lat0 + (nx1)*dlon;
nx = number of grid points in X direction
ny = number of grid points in Y direction
ny must be even
dlon = degrees of longitude between adjacent grid points
new_grid mercator:lad lon0:nx:dx:lonn lat0:ny:dy:latn outfile lad = latitude (degrees) where dx and dy are specified
lat0, lon0 = degrees of lat/lon for 1st grid point
latn, lonn = degrees of lat/lon for last grid point
nx = number of grid points in X direction
ny = number of grid points in Y direction
dx = grid cell distance in meters in x direction at lad
dy = grid cell distance in meters in y direction at lad
note: the mercator grid description is over specified
User must make sure (nx,dy) is consistent with lonn
as well as (ny,dy) is consistent with latn
lambert, nps, sps, mercator only support we:sn ordering
latlon, gaussian only support we:sn and we:ns ordering
Type of Interpolation
The IPOLATES library supports a number of interpolation schemes including bilinear (default),
bicubic, neighbor and budget. The wgrib2 was tested with the spectral interpolation but
that option was removed because it greatly increased the code size for a minor option.
The interpolation method can be selected by using the new_grid_interpolation
option before the new_grid option. Some of the interpolation
options need numeric parameters which are set by the
new_grid_ipopt option. IPOPT is defined in the IPOLATES library documentation.
You can use different interpolations for different variables. For example, a
bilinear interpolation of soil or vegetation type is meaningless. So
nearest neighbor interpolation is used instead.
wgrib2 IN.grb new_grid_winds earth \
new_grid_interpolation bilinear \
if ":(VGTYPSOTYP):" new_grid_interpolation neighbor fi \
new_grid latlon 0:360:1 90:181:1 OUT.grb
line 2: set default interpolation to bilinear
line 3: if VGTYP or SOTYP then set the interpolation to nearest neighbor
line 4: do the interpolation
Winds
Before you do an interpolation, you need to define the wind directions.
Most people want the the V winds to be in the direction of the North Pole.
With a verbose wgrib2 inventory, you will seee winds(N/S). However, some
meteorologists want the V winds to go from grid point (i,j) to (i,j+1).
The corresponding wgrib2 notation is "winds(grid)". See the
new_grid_winds option for more details.
Changes from copygb
 copygb default vectors: UGRD/VGRD
 wgrib2 default vectors: depends on version of wgrib2. See new_grid_vectors.
 copygb can have vectors in any order
 wgrib2 must have V follow U for vectors pairs
 copygb has bilinear, bicubic, nearest neighbor, budget and spectral interpolations.
 wgrib2 has bilinear, bicubic, nearest neighbor, and budget interpolations.
 copygb uses fixed Earth's radius
 wgrib2 uses Earth's radius based on grib message
 wgrib2 doesn't have merging, mapthreshold or map files
 copygb by default, ignores the binary scaling and preserves decimal scaling
 wgrib2 by default, preserves binary and decimal scaling
 copygb does grib1.
 wgrib2 does grib2.
Speed: Interpolation Weights
The first step of the new_grid interpolation is
to calculate the interpolation weights. (Each grid point on the new grid
is a weighted average of a small set of the old grid points.)
To save time for future interpolations, the last set of weights is saved.
Consequently interpolation is fastest when the input and output grids remain
don't change. While one can have multiple new_grid options on
the command line, it is not recommended because the caching of the weights
wouldn't work and weights would have to be recalculated every time.
Installation
1) set USE_IPOLATES to 1 in the makefile
2) environment variable $FC must be set to the fortran90 compiler, ex. export FC=gfortran
3) If $FC is not gfortran, openf95, or xlf_r, then
modify the makefile for the new fortran compiler
modify New_grid.c for the new fortran compiler
Note: icc and pgc are incompatible with the jasper library and are not supported
4) now you are ready to make
Converting from WE:SN to WE:NS Grids
Many of wgrib2 grib2 writing options will write the grid
in WE:SN order. This natural because geolocation is
only enabled when the internal grids are in WE:SN order.
However, some codes need the grid in WE:NS order. To
convert a grib file from WE:SN order to WE:NS order, the
simplest way is to use new_grid. Lat0 and lon0 need
to be lat/lon of the top left corner of the grid. Dlon
will a positive number and dlat will be negative.
If you want to be tricky, you can do a variation of the
"NDFD work arounds" technique. It will be faster and
more generic.
Quilting tiles  Merging files
Yes, it can be done using new_grid, bin, import_bin rpn, and
the grib_out options. No, I haven't done it.
Limitations of the IPOLATES library
The IPOLATES library has its limitations.
Grids types used by NCEP get supported and others don't. The library has a grib1 interface, so
new features of grib2 are not supported and the precision of the grid parameters
are limited to the grib1 values. For example, latitude and longitude
values are limited to millidegrees instead of microdegrees.
 not all grid types are supported by IPOLATES
 only common grids are supported by the wgrib2 "wrapper" for IPOLATES
 latitude, longitude values are in millidegrees (affects interpolation)
 only grib1 scan order are supported (i.e., WE:SN and WE:NS)
 NDFD/Glahn scan order are not supported (i.e., WEEW:SN)
 Earth is assumed to be spherical
 Lambert conformal: LatD must follow grib1 conventions
 Polar Stereographic: LatD must be 60 latitude (grib1 convention)
 nx, ny, npts must be ≤ 2147483647. (Grib2 standard is 4294967295.)
NDFD work arounds
NDFD files are written in an order which is not supported by the IPOLATES library.
The NDFD files come in (WEEW):SN order. Which means the odd rows are in WE order and
the even rows are EW order. The rows go from south to north. The solution is to
convert the grid to WE:SN order is
Version 0
 for data in input=WEEW:SN scan order (wgrib2 IN scan)
 read data, change order scan order of data, change flag table 3.4, save data
 wgrib2 IN.grb rpn alt_x_scan set table_3.4 64 grib_out OUT.grb
Version 1
 Read trick 55 in wgrib2 tricks
Version 1
A variation of the previous trick can be used to put data in to (WEEW):SN packing.
See also:
new_grid_interpolation,
new_grid_winds,
new_grid_vectors,
lola,
bin,
import_bin,
rpn,
grib_out,
new_grid multicore usage,
