Provided by: gdal-bin_3.8.4+dfsg-3ubuntu3_amd64 bug

NAME

       gdalwarp - Image reprojection and warping utility.

SYNOPSIS

          gdalwarp [--help] [--help-general] [--formats]
              [-b|-srcband <n>]... [-dstband <n>]...
              [-s_srs <srs_def>] [-t_srs <srs_def>] [-ct <string>]
              [-to <NAME>=<VALUE>]... [-vshift | -novshift]
              [-s_coord_epoch <epoch>] [-t_coord_epoch <epoch>]
              [-order n | -tps | -rpc | -geoloc] [-et <err_threshold>]
              [-refine_gcps <tolerance> [<minimum_gcps>]]
              [-te <xmin> <ymin> <xmax> <ymax>] [-te_srs <srs_def>]
              [-tr <xres> <yres>]|[-tr square] [-tap] [-ts <width> <height>]
              [-ovr <level>|AUTO|AUTO-<n>|NONE] [-wo <NAME>=<VALUE>]... [-ot Byte/Int16/...] [-wt Byte/Int16]
              [-srcnodata "<value>[ <value>...]"][-dstnodata "<value>[ <value>...]"]
              [-srcalpha|-nosrcalpha] [-dstalpha]
              [-r <resampling_method>] [-wm <memory_in_mb>] [-multi] [-q]
              [-cutline <datasource>] [-cl <layer>] [-cwhere <expression>]
              [-csql <statement>] [-cblend <dist_in_pixels>] [-crop_to_cutline]
              [-if <format>]... [-of <format>] [-co <NAME>=<VALUE>]... [-overwrite]
              [-nomd] [-cvmd <meta_conflict_value>] [-setci] [-oo <NAME>=<VALUE>]...
              [-doo <NAME>=<VALUE>]...
              <srcfile>... <dstfile>

DESCRIPTION

       The  gdalwarp  utility is an image mosaicing, reprojection and warping utility. The program can reproject
       to any supported projection, and can also apply GCPs stored with the image if the  image  is  "raw"  with
       control information.

       --help Show this help message and exit

       --help-general
              Gives a brief usage message for the generic GDAL commandline options and exit.

       -b <n>

       -srcband <n>
              New in version 3.7.

              Specify an input band number to warp (between 1 and the number of bands of the source dataset).

              This  option  is used to warp a subset of the input bands. All input bands are used when it is not
              specified.

              This option may be repeated multiple times to select several input  bands.   The  order  in  which
              bands  are specified will be the order in which they appear in the output dataset (unless -dstband
              is specified).

              The alpha band should not be specified in the list, as it will be automatically retrieved  (unless
              -nosrcalpha is specified).

              The  following  invocation  will  warp  an  input datasets with bands ordered as Blue, Green, Red,
              NearInfraRed in an output dataset with bands ordered as Red, Green, Blue.

                 gdalwarp in_bgrn.tif out_rgb.tif -b 3 -b 2 -b 1 -overwrite

       -dstband <n>
              New in version 3.7.

              Specify the output band number in which to warp. In practice, this  option  is  only  useful  when
              updating an existing dataset, e.g to warp one band at at time.

                 gdal_create -if in_red.tif -bands 3 out_rgb.tif
                 gdalwarp in_red.tif out_rgb.tif -srcband 1 -dstband 1
                 gdalwarp in_green.tif out_rgb.tif -srcband 1 -dstband 2
                 gdalwarp in_blue.tif out_rgb.tif -srcband 1 -dstband 3

              If -srcband is specified, there must be as many occurrences of -dstband as there are of -srcband.

              The  output  alpha  band should not be specified, as it will be automatically created if the input
              dataset has an alpha band, or if -dstalpha is specified.

              If -dstband is not specified, then -dstband 1 -dstband 2 ... -dstband N is assumed where N is  the
              number of input bands (specified explicitly either with -srcband or implicitly)

       -s_srs <srs def>
              Set source spatial reference. If not specified the SRS found in the input dataset will be used.

              The   coordinate   reference   systems   that   can  be  passed  are  anything  supported  by  the
              OGRSpatialReference.SetFromUserInput() call, which includes EPSG Projected, Geographic or Compound
              CRS (i.e. EPSG:4296), a well known text (WKT) CRS definition, PROJ.4 declarations, or the name  of
              a .prj file containing a WKT CRS definition.

              Starting  with  GDAL  2.2,  if  the  SRS  has  an  explicit vertical datum that points to a PROJ.4
              geoidgrids, and the input dataset is a single band dataset, a vertical correction will be  applied
              to the values of the dataset.

       -s_coord_epoch <epoch>
              New in version 3.4.

              Assign  a  coordinate  epoch,  linked with the source SRS. Useful when the source SRS is a dynamic
              CRS. Only taken into account if -s_srs is used.

              Before PROJ 9.4, -s_coord_epoch and -t_coord_epoch are mutually exclusive, due to lack of  support
              for transformations between two dynamic CRS.

       -t_srs <srs_def>
              Set target spatial reference.

              A  source  SRS  must be available for reprojection to occur. The source SRS will be by default the
              one found in the input dataset when it is available, or as overridden by the user with -s_srs

              The  coordinate  reference  systems  that  can  be  passed   are   anything   supported   by   the
              OGRSpatialReference.SetFromUserInput() call, which includes EPSG Projected, Geographic or Compound
              CRS  (i.e. EPSG:4296), a well known text (WKT) CRS definition, PROJ.4 declarations, or the name of
              a .prj file containing a WKT CRS definition.

              Starting with GDAL 2.2, if the SRS has  an  explicit  vertical  datum  that  points  to  a  PROJ.4
              geoidgrids,  and the input dataset is a single band dataset, a vertical correction will be applied
              to the values of the dataset.

       -t_coord_epoch <epoch>
              New in version 3.4.

              Assign a coordinate epoch, linked with the target SRS. Useful when the target  SRS  is  a  dynamic
              CRS. Only taken into account if -t_srs is used.

              Before  PROJ 9.4, -s_coord_epoch and -t_coord_epoch are mutually exclusive, due to lack of support
              for transformations between two dynamic CRS.

       -ct <string>
              A PROJ string (single step operation or multiple step string starting with +proj=pipeline), a WKT2
              string describing  a  CoordinateOperation,  or  a  urn:ogc:def:coordinateOperation:EPSG::XXXX  URN
              overriding the default transformation from the source to the target CRS. It must take into account
              the  axis  order  of  the source and target CRS.  When creating a new output file, using -t_srs is
              still necessary to have the target CRS written in  the  metadata  of  the  output  file,  but  the
              parameters of the CoordinateOperation will override those of the standard transformation.

              New in version 3.0.

       -to <NAME>=<VALUE>
              Set   a   transformer   option   suitable  to  pass  to  GDALCreateGenImgProjTransformer2().   See
              GDALCreateRPCTransformerV2() for RPC specific options.

       -vshift
              Force the use of vertical shift. This option is generally not  necessary,  except  when  using  an
              explicit coordinate transformation (-ct), and not specifying an explicit source and target SRS.

              New in version 3.4.

       -novshift
              Disable  the  use  of vertical shift when one of the source or target SRS has an explicit vertical
              datum, and the input dataset is a single band dataset.

              NOTE:
                 this option was named -novshiftgrid in GDAL 2.2 to 3.3.

              New in version 3.4.

       -order <n>
              order of polynomial used for warping (1 to 3). The default is to select a polynomial  order  based
              on the number of GCPs.

       -tps   Force use of thin plate spline transformer based on available GCPs.

       -rpc   Force use of RPCs.

       -geoloc
              Force use of Geolocation Arrays.

       -et <err_threshold>
              Error  threshold  for  transformation  approximation  (in pixel units - defaults to 0.125, unless,
              starting with GDAL 2.1, the RPC_DEM transformer option is  specified,  in  which  case,  an  exact
              transformer, i.e.  err_threshold=0, will be used).

       -refine_gcps <tolerance> [<minimum_gcps>]
              Refines  the  GCPs  by  automatically  eliminating  outliers.   Outliers  will be eliminated until
              minimum_gcps are left or when no outliers can be detected.  The tolerance is passed to adjust when
              a GCP will be eliminated.  Not that GCP refinement only works with polynomial interpolation.   The
              tolerance  is  in  pixel  units  if  no projection is available, otherwise it is in SRS units.  If
              minimum_gcps is not provided, the minimum GCPs according to the polynomial model is used.

       -te <xmin> <ymin> <xmax> <ymax>
              Set georeferenced extents of output file to be created (in target SRS by default, or  in  the  SRS
              specified with -te_srs)

       -te_srs <srs_def>
              Specifies  the  SRS in which to interpret the coordinates given with -te. The <srs_def> may be any
              of the usual GDAL/OGR forms, complete WKT, PROJ.4, EPSG:n or a file containing the WKT.  This must
              not be confused with -t_srs which  is  the  target  SRS  of  the  output  dataset.  -te_srs  is  a
              convenience e.g. when knowing the output coordinates in a geodetic long/lat SRS, but still wanting
              a result in a projected coordinate system.

       -tr <xres> <yres> | -tr square
              Set output file resolution (in target georeferenced units).

              If  not  specified (or not deduced from -te and -ts), gdalwarp will, in the general case, generate
              an output raster with xres=yres.

              Starting with GDAL 3.7, if neither -tr nor -ts are specified, that  no  reprojection  is  involved
              (including  taking  into  account geolocation arrays or RPC), the resolution of the source file(s)
              will be preserved (in previous version, an output raster with xres=yres was always generated).  It
              is possible to ask square pixels to still be generated, by specifying square as the value for -tr.

       -tap   (target aligned pixels) align the coordinates of the extent of the output file to  the  values  of
              the  -tr,  such  that the aligned extent includes the minimum extent (edges lines/columns that are
              detected as blank, before actual warping, will be removed  starting  with  GDAL  3.8).   Alignment
              means that xmin / resx, ymin / resy, xmax / resx and ymax / resy are integer values.

       -ts <width> <height>
              Set output file size in pixels and lines. If width or height is set to 0, the other dimension will
              be guessed from the computed resolution. Note that -ts cannot be used with -tr

       -ovr <level>|AUTO|AUTO-<n>|NONE
              To  specify  which  overview  level  of  source files must be used. The default choice, AUTO, will
              select the overview level whose resolution is the closest to the  target  resolution.  Specify  an
              integer  value  (0-based,  i.e. 0=1st overview level) to select a particular level. Specify AUTO-n
              where n is an integer greater or equal to 1, to select an overview level below the  AUTO  one.  Or
              specify  NONE  to  force  the  base  resolution  to  be used (can be useful if overviews have been
              generated with a low quality resampling method, and the warping is done  using  a  higher  quality
              resampling method).

       -wo <NAME>=<VALUE>
              Set  a  warp  option.   The GDALWarpOptions::papszWarpOptions docs show all options.  Multiple -wo
              options may be listed.

       -ot <type>
              Force the output image bands to have a specific data type supported by the driver,  which  may  be
              one  of  the following: Byte, Int8, UInt16, Int16, UInt32, Int32, UInt64, Int64, Float32, Float64,
              CInt16, CInt32, CFloat32 or CFloat64.

       -wt <type>
              Working pixel data type. The data type of  pixels  in  the  source  image  and  destination  image
              buffers.

       -r <resampling_method>
              Resampling method to use. Available methods are:

              near: nearest neighbour resampling (default, fastest algorithm, worst interpolation quality).

              bilinear: bilinear resampling.

              cubic: cubic resampling.

              cubicspline: cubic spline resampling.

              lanczos: Lanczos windowed sinc resampling.

              average: average resampling, computes the weighted average of all non-NODATA contributing pixels.

              rms root mean square / quadratic mean of all non-NODATA contributing pixels (GDAL >= 3.3)

              mode:  mode  resampling,  selects the value which appears most often of all the sampled points. In
              the case of ties, the first value identified as the mode will be selected.

              max: maximum resampling, selects the maximum value from all non-NODATA contributing pixels.

              min: minimum resampling, selects the minimum value from all non-NODATA contributing pixels.

              med: median resampling, selects the median value of all non-NODATA contributing pixels.

              q1: first quartile resampling, selects the first quartile value  of  all  non-NODATA  contributing
              pixels.

              q3:  third  quartile  resampling,  selects the third quartile value of all non-NODATA contributing
              pixels.

              sum: compute the weighted sum of all non-NODATA contributing pixels (since GDAL 3.1)

              NOTE:
                 When  downsampling  is  performed  (use  of   -tr   or   -ts),   existing   overviews   (either
                 internal/implicit  or  external  ones) on the source image will be used by default by selecting
                 the closest overview to the desired output resolution.  The resampling method  used  to  create
                 those  overviews is generally not the one you specify through the -r option. Some formats, like
                 JPEG2000, can contain significant outliers due to wavelet compression works. It might  thus  be
                 useful  in  those  situations  to  use the -ovr NONE option to prevent existing overviews to be
                 used.

       -srcnodata "<value>[ <value>]..."
              Set nodata masking values for input bands (different values can be supplied  for  each  band).  If
              more  than  one  value  is  supplied all values should be quoted to keep them together as a single
              operating system argument.  Masked values will not be used  in  interpolation  (details  given  in
              Nodata / source validity mask handling)

              Use a value of None to ignore intrinsic nodata settings on the source dataset.

              When  this option is set to a non-None value, it causes the UNIFIED_SRC_NODATA warping option (see
              GDALWarpOptions::papszWarpOptions) to be set to YES, if it is not explicitly set.

              If -srcnodata is not explicitly set, but the source dataset has nodata values, they will be  taken
              into account, with UNIFIED_SRC_NODATA at PARTIAL by default.

       -dstnodata "<value>[ <value>]..."
              Set nodata values for output bands (different values can be supplied for each band).  If more than
              one  value  is  supplied  all  values should be quoted to keep them together as a single operating
              system argument.  New files will be initialized to this value and if  possible  the  nodata  value
              will be recorded in the output file. Use a value of None to ensure that nodata is not defined.  If
              this argument is not used then nodata values will be copied from the source dataset.

       -srcalpha
              Force the last band of a source image to be considered as a source alpha band.

       -nosrcalpha
              Prevent  the alpha band of a source image to be considered as such (it will be warped as a regular
              band)

              New in version 2.2.

       -dstalpha
              Create an output alpha band to identify nodata (unset/transparent) pixels.

       -wm <memory_in_mb>
              Set the amount of memory that the warp API is allowed to use for caching. The value is interpreted
              as being in megabytes if the value is less than 10000. For values >=10000, this is interpreted  as
              bytes.

              The  warper  will  total  up the memory required to hold the input and output image arrays and any
              auxiliary masking arrays and if they are larger than the "warp memory" allowed it  will  subdivide
              the chunk into smaller chunks and try again.

              If  the -wm value is very small there is some extra overhead in doing many small chunks so setting
              it larger is better but it is a matter of diminishing returns.

       -multi Use multithreaded warping implementation.  Two threads will be used to process chunks of image and
              perform input/output operation simultaneously. Note that computation is not multithreaded  itself.
              To do that, you can use the -wo NUM_THREADS=val/ALL_CPUS option, which can be combined with -multi

       -q     Be quiet.

       -if <format>
              Format/driver  name  to  be  attempted to open the input file(s). It is generally not necessary to
              specify it, but it can be used to skip automatic driver detection, when it  fails  to  select  the
              appropriate  driver.   This  option  can  be  repeated  several times to specify several candidate
              drivers.  Note that it does not force those drivers to  open  the  dataset.  In  particular,  some
              drivers have requirements on file extensions.

              New in version 3.2.

       -of <format>
              Select the output format. Starting with GDAL 2.3, if not specified, the format is guessed from the
              extension (previously was GTiff). Use the short format name.

       -co <NAME>=<VALUE>
              Many  formats  have  one or more optional creation options that can be used to control particulars
              about the file created. For instance, the GeoTIFF driver  supports  creation  options  to  control
              compression, and whether the file should be tiled.

              The  creation  options  available  vary by format driver, and some simple formats have no creation
              options at all. A list of options supported for a format can be listed with the --formats  command
              line option but the documentation for the format is the definitive source of information on driver
              creation options.  See Raster drivers format specific documentation for legal creation options for
              each format.

       -cutline <datasource>
              Enable use of a blend cutline from the name OGR support datasource.

       -cl <layername>
              Select the named layer from the cutline datasource.

       -cwhere <expression>
              Restrict desired cutline features based on attribute query.

       -csql <query>
              Select cutline features using an SQL query instead of from a layer with -cl.

       -cblend <distance>
              Set a blend distance to use to blend over cutlines (in pixels).

       -crop_to_cutline
              Crop the extent of the target dataset to the extent of the cutline.

       -overwrite
              Overwrite the target dataset if it already exists. Overwriting must be understood here as deleting
              and  recreating  the  file  from scratch. Note that if this option is not specified and the output
              file already exists, it will be updated in place.

       -nomd  Do not copy metadata. Without this option, dataset  and  band  metadata  (as  well  as  some  band
              information)  will  be  copied  from  the  first source dataset.  Items that differ between source
              datasets will be set to * (see -cvmd option).

       -cvmd <meta_conflict_value>
              Value to set metadata items that conflict between source datasets (default  is  "*").  Use  ""  to
              remove conflicting items.

       -setci Set the color interpretation of the bands of the target dataset from the source dataset.

       -oo <NAME>=<VALUE>
              Dataset open option (format specific)

       -doo <NAME>=<VALUE>
              Output dataset open option (format specific)

              New in version 2.1.

       <srcfile>
              The source file name(s).

       <dstfile>
              The destination file name.

       Mosaicing into an existing output file is supported if the output file already exists. The spatial extent
       of  the  existing file will not be modified to accommodate new data, so you may have to remove it in that
       case, or use the -overwrite option.

       Polygon cutlines may be used as a mask to restrict the area of the destination file that may be  updated,
       including  blending.   If  the OGR layer containing the cutline features has no explicit SRS, the cutline
       features must be in the SRS of the destination file. When writing to a not yet existing  target  dataset,
       its extent will be the one of the original raster unless -te or -crop_to_cutline are specified.

       Starting with GDAL 3.1, it is possible to use as output format a driver that only supports the CreateCopy
       operation. This may internally imply creation of a temporary file.

NODATA / SOURCE VALIDITY MASK HANDLING

       Invalid  values  in  source  pixels,  either identified through a nodata value metadata set on the source
       band, a mask band, an alpha band or the use of -srcnodata will not be used in interpolation.  The details
       of how it is taken into account depends on the resampling kernel:

       • for nearest resampling, for each target pixel, the coordinate of its center is projected back to source
         coordinates and the source pixel containing that coordinate is identified.  If  this  source  pixel  is
         invalid, the target pixel is considered as nodata.

       • for  bilinear,  cubic,  cubicspline and lanczos, for each target pixel, the coordinate of its center is
         projected back to source coordinates and a corresponding source pixel is  identified.  If  this  source
         pixel is invalid, the target pixel is considered as nodata.  Given that those resampling kernels have a
         non-null  kernel  radius, this source pixel is just one among other several source pixels, and it might
         be possible that there are invalid values in those other contributing source pixels.  The weights  used
         to take into account those invalid values will be set to zero to ignore them.

       • for  the  other  resampling  methods,  source  pixels  contributing  to the target pixel are ignored if
         invalid. Only the valid ones are taken into account. If there are none, the target pixel is  considered
         as nodata.

       If using -srcnodata for multiple images with different invalid values, you need to either (a) pre-process
       them  to have the same to-be-ignored value, or (b) set the nodata flag for each file. Use (b) if you need
       to preserve the original values for some reason, for example:

          # for this image we want to ignore black (0)
          gdalwarp -srcnodata 0 -dstnodata 0 orig-ignore-black.tif black-nodata.tif

          # and now we want to ignore white (0)
          gdalwarp -srcnodata 255 -dstnodata 255 orig-ignore-white.tif white-nodata.tif

          # and finally ignore a particular blue-grey (RGB 125 125 150)
          gdalwarp -srcnodata "125 125 150" -dstnodata "125 125 150" orig-ignore-grey.tif grey-nodata.tif

          # now we can mosaic them all and not worry about nodata parameters
          gdalwarp black-nodata.tif grey-nodata.tif white-nodata.tif final-mosaic.tif

APPROXIMATE TRANSFORMATION

       By default gdalwarp uses a linear approximator for the transformations with a permitted  error  of  0.125
       pixels.  The  approximator  basically  transforms  three points on a scanline: the start, end and middle.
       Then it compares the linear approximation of the center based on the end points to  the  real  thing  and
       checks  the  error.  If  the  error  is  less  than  the  error  threshold  then the remaining points are
       approximated (in two chunks utilizing the center point). If the error exceeds the threshold, the scanline
       is split into two sections, and the approximator is recursively applied to each section until  the  error
       is less than the threshold or all points have been exactly computed.

       The  error threshold (in pixels) can be controlled with the gdalwarp -et switch. If you want to compare a
       true pixel-by-pixel reprojection use -et 0 which disables this approximator entirely.

MEMORY USAGE

       Adding RAM will almost certainly increase the speed of gdalwarp.  That's not at all the  same  as  saying
       that  it  is  worth it, or that the speed increase will be significant. Disks are the slowest part of the
       process.  By default gdalwarp won't take much advantage of RAM. Using the flag -wm 500  will  operate  on
       500MB chunks at a time which is better than the default. The warp memory specified by -wm is shared among
       all  threads,  so  it  is  especially  beneficial  to  increase this value when running gdalwarp with -wo
       NUM_THREADS (or its equivalent GDAL_NUM_THREADS) greater than 1.

       Increasing the I/O block cache size may also  help.  This  can  be  done  by  setting  the  GDAL_CACHEMAX
       configuration like:

          gdalwarp --config GDAL_CACHEMAX 500 -wm 500 ...

       This  uses  500MB  of  RAM  for read/write caching, and 500MB of RAM for working buffers during the warp.
       Beyond that it is doubtful more memory will make a substantial difference.

       Check CPU usage while gdalwarp is running. If it is substantially less than 100% then you know things are
       IO bound. Otherwise they are CPU bound.  The --debug option may  also  provide  useful  information.  For
       instance, after running the following:

          gdalwarp --debug on abc.tif def.tif

       a message like the following will be output:

          GDAL: 224 block reads on 32 block band 1 of utm.tif

       In  this  case  it  is  saying  that band 1 of utm.tif has 32 blocks, but that 224 block reads were done,
       implying that lots of data was having to be re-read, presumably because of a limited IO cache.  You  will
       also see messages like:

          GDAL: GDALWarpKernel()::GWKNearestNoMasksByte()
          Src=0,0,512x512 Dst=0,0,512x512

       The  Src/Dst  windows  show  you  the  "chunk size" being used. In this case my whole image which is very
       small. If you find things are being broken into a lot of chunks increasing -wm may help somewhat.

       But far more important than memory are ensuring you are going through an optimized path in the warper. If
       you ever see it reporting GDALWarpKernel()::GWKGeneralCase() you know things  will  be  relatively  slow.
       Basically,  the  fastest situations are nearest neighbour resampling on 8bit data without nodata or alpha
       masking in effect.

COMPRESSED OUTPUT

       In some cases, the output of gdalwarp may be much larger than the original, even if the same  compression
       algorithm  is  used.  By  default,  gdalwarp operates on chunks that are not necessarily aligned with the
       boundaries  of  the  blocks/tiles/strips  of  the  output  format,   so   this   might   cause   repeated
       compression/decompression of partial blocks, leading to lost space in the output format.

       The situation can be improved by using the OPTIMIZE_SIZE warping option (-wo OPTIMIZE_SIZE=YES), but note
       that  depending  on  the source and target projections, it might also significantly slow down the warping
       process.

       Another possibility is to use gdalwarp without compression and then follow up  with  gdal_translate  with
       compression:

          gdalwarp infile tempfile.tif ...options...
          gdal_translate tempfile.tif outfile.tif -co compress=lzw ...etc.

       Alternatively,  you can use a VRT file as the output format of gdalwarp. The VRT file is just an XML file
       that will be created immediately. The gdal_translate operations will be of course a bit slower as it will
       do the real warping operation.

          gdalwarp -of VRT infile tempfile.vrt ...options...
          gdal_translate tempfile.vrt outfile.tif -co compress=lzw ...etc.

EXAMPLES

       • Basic transformation:

          gdalwarp -t_srs EPSG:4326 input.tif output.tif

       • For instance, an eight bit spot scene stored in GeoTIFF with control  points  mapping  the  corners  to
         lat/long could be warped to a UTM projection with a command like this:

          gdalwarp -t_srs '+proj=utm +zone=11 +datum=WGS84' -overwrite raw_spot.tif utm11.tif

       • For  instance,  the  second  channel  of  an  ASTER image stored in HDF with control points mapping the
         corners to lat/long could be warped to a UTM projection with a command like this:
            New in version 2.2.

          gdalwarp -overwrite HDF4_SDS:ASTER_L1B:"pg-PR1B0000-2002031402_100_001":2 pg-PR1B0000-2002031402_100_001_2.tif

       • To apply a cutline on a un-georeferenced image and clip from pixel (220,60) to pixel (1160,690):

          gdalwarp -overwrite -to SRC_METHOD=NO_GEOTRANSFORM -to DST_METHOD=NO_GEOTRANSFORM -te 220 60 1160 690 -cutline cutline.csv in.png out.tif

       where cutline.csv content is like:

          id,WKT
          1,"POLYGON((....))"

       • To transform a DEM from geoid elevations (using EGM96) to WGS84 ellipsoidal heights:
            New in version 2.2.

          gdalwarp -overwrite in_dem.tif out_dem.tif -s_srs EPSG:4326+5773 -t_srs EPSG:4979

C API

       This utility is also callable from C with GDALWarp().

SEE ALSO

       Wiki page discussing options and behaviours of gdalwarp

AUTHOR

       Frank Warmerdam <warmerdam@pobox.com>, Silke Reimer <silke@intevation.de>

COPYRIGHT

       1998-2024

                                                  Feb 08, 2024                                       GDALWARP(1)