|2-D binary grid file to be transformed. (See GRID FILE FORMATS below.)|
|-G||Specify the name of the output grid file. (See GRID FILE FORMATS below.)|
Selects the map projection. Scale is UNIT/degree, 1:xxxxx, or width in UNIT (upper case modifier).
UNIT is cm, inch, or m, depending on the MEASURE_UNIT setting in .gmtdefaults4, but this can be
overridden on the command line by appending c, i, or m to the scale/width value.
When central meridian is optional, default is center of longitude range on -R option.
Default standard parallel is the equator.
For map height, max dimension, or min dimension, append h, +, or - to the width,
More details can be found in the psbasemap man pages.
-Jalon0/lat0[/horizon]/scale (Lambert Azimuthal Equal-Area)
-Jp[a]scale[/origin][r|z] (Polar coordinates (theta,r))
No space between the option flag and the associated arguments.
-A Force 1:1 scaling, i.e., output (or input, see -I) data are in actual projected meters. To specify other units, append k (km), m (mile),n (nautical mile), i (inch), c (cm), or p (points). Without -A, the output (or input, see -I) are in the units specified by MEASURE_UNIT (but see -M). -C Let projected coordinates be relative to projection center [Default is relative to lower left corner]. Optionally, add offsets in the projected units to be added (or subtracted when -I is set) to (from) the projected coordinates, such as false eastings and northings for particular projection zones [0/0]. -D x_inc [and optionally y_inc] is the grid spacing. Optionally, append a suffix modifier. Geographical (degrees) coordinates: Append m to indicate arc minutes or c to indicate arc seconds. If one of the units e, k, i, or n is appended instead, the increment is assumed to be given in meter, km, miles, or nautical miles, respectively, and will be converted to the equivalent degrees longitude at the middle latitude of the region (the conversion depends on ELLIPSOID). If /y_inc is given but set to 0 it will be reset equal to x_inc; otherwise it will be converted to degrees latitude. All coordinates: If = is appended then the corresponding max x (east) or y (north) may be slightly adjusted to fit exactly the given increment [by default the increment may be adjusted slightly to fit the given domain]. Finally, instead of giving an increment you may specify the number of nodes desired by appending + to the supplied integer argument; the increment is then recalculated from the number of nodes and the domain. The resulting increment value depends on whether you have selected a gridline-registered or pixel-registered grid; see Appendix B for details. Note: if -Rgrdfile is used then grid spacing has already been initialized; use -D to override the values. -E Set the resolution for the new grid in dots per inch. -F Toggle between pixel and gridline node registration [Default is same as input]. -I Do the Inverse transformation, from rectangular to geographical. -M Append c, i, or m to indicate that cm, inch, or meter should be the projected measure unit [Default is set by MEASURE_UNIT in .gmtdefaults4]. Cannot be used with -A. -N Set the number of grid nodes in the new grid. -R xmin, xmax, ymin, and ymax specify the Region of interest. For geographic regions, these limits correspond to west, east, south, and north and you may specify them in decimal degrees or in [+-]dd:mm[:ss.xxx][W|E|S|N] format. Append r if lower left and upper right map coordinates are given instead of w/e/s/n. The two shorthands -Rg and -Rd stand for global domain (0/360 and -180/+180 in longitude respectively, with -90/+90 in latitude). Alternatively, specify the name of an existing grid file and the -R settings (and grid spacing, if applicable) are copied from the grid. For calendar time coordinates you may either give (a) relative time (relative to the selected TIME_EPOCH and in the selected TIME_UNIT; append t to -JX|x), or (b) absolute time of the form [date]T[clock] (append T to -JX|x). At least one of date and clock must be present; the T is always required. The date string must be of the form [-]yyyy[-mm[-dd]] (Gregorian calendar) or yyyy[-Www[-d]] (ISO week calendar), while the clock string must be of the form hh:mm:ss[.xxx]. The use of delimiters and their type and positions must be exactly as indicated (however, input, output and plot formats are customizable; see gmtdefaults). You may ask to project only a subset of the grid by specifying a smaller input w/e/s/n region [Default is the region given by the grid file]. Special case for the UTM projection: If -C and -I are used and -R is not given then the region is set to coincide with the given UTM zone so as to preserve the full ellipsoidal solution (See RESTRICTIONS for more information). -S Select the interpolation mode by adding b for B-spline smoothing, c for bicubic interpolation, l for bilinear interpolation, or n for nearest-neighbor value (for example to plot categorical data). Optionally, prepend - to switch off antialiasing. Add /threshold to control how close to nodes with NaNs the interpolation will go. A threshold of 1.0 requires all (4 or 16) nodes involved in interpolation to be non-NaN. 0.5 will interpolate about half way from a non-NaN value; 0.1 will go about 90% of the way, etc. [Default is bicubic interpolation with antialiasing and a threshold of 0.5]. -V Selects verbose mode, which will send progress reports to stderr [Default runs "silently"].
By default GMT writes out grid as single precision floats in a COARDS-complaint netCDF file format. However, GMT is able to produce grid files in many other commonly used grid file formats and also facilitates so called "packing" of grids, writing out floating point data as 2- or 4-byte integers. To specify the precision, scale and offset, the user should add the suffix =id[/scale/offset[/nan]], where id is a two-letter identifier of the grid type and precision, and scale and offset are optional scale factor and offset to be applied to all grid values, and nan is the value used to indicate missing data. When reading grids, the format is generally automatically recognized. If not, the same suffix can be added to input grid file names. See grdreformat(1) and Section 4.17 of the GMT Technical Reference and Cookbook for more information.
When reading a netCDF file that contains multiple grids, GMT will read, by default, the first 2-dimensional grid that can find in that file. To coax GMT into reading another multi-dimensional variable in the grid file, append ?varname to the file name, where varname is the name of the variable. Note that you may need to escape the special meaning of ? in your shell program by putting a backslash in front of it, or by placing the filename and suffix between quotes or double quotes. The ?varname suffix can also be used for output grids to specify a variable name different from the default: "z". See grdreformat(1) and Section 4.18 of the GMT Technical Reference and Cookbook for more information, particularly on how to read splices of 3-, 4-, or 5-dimensional grids.
To transform the geographical grid dbdb5.grd onto a pixel Mercator grid at 300 dpi, run
grdproject dbdb5.grd -R 20/50/12/25 -Jm 0.25i -E 300 -F -G dbdb5_merc.grd
To inversely transform the file topo_tm.grd back onto a geographical grid, use
grdproject topo_tm.grd -R-80/-70/20/40 -Jt-75/1:500000 -I -D 5m -V -G topo.grd
This assumes, of course, that the coordinates in topo_tm.grd were created with the same projection parameters.
To inversely transform the file topo_utm.grd (which is in UTM meters) back to a geographical grid we specify a one-to-one mapping with meter as the measure unit:
grdproject topo_utm.grd -R 203/205/60/65 -Ju 5/1:1 -I -Mm -G topo.grd -V
The boundaries of a projected (rectangular) data set will not necessarily give rectangular geographical boundaries (Mercator is one exception). In those cases some nodes may be unconstrained (set to NaN). To get a full grid back, your input grid may have to cover a larger area than you are interested in.
For some projections, a spherical solution may be used despite the user having selected an ellipsoid. This occurs when the users -R setting implies a region that exceeds the domain in which the ellipsoidal series expansions are valid. These are the conditions: (1) Lambert Conformal Conic (-JL) and Albers Equal-Area (-JB) will use the spherical solution when the map scale exceeds 1.0E7. (2) Transverse Mercator (-JT) and UTM (-JU) will will use the spherical solution when either the west or east boundary given in -R is more than 10 degrees from the central meridian, and (3) same for Cassini (-JC) but with a limit of only 4 degrees.
|GMT 4.5.14||GRDPROJECT (1)||1 Nov 2015|