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GDALWARP(1) |
GDAL |
GDALWARP(1) |
gdalwarp - Image reprojection and warping utility.
Usage: gdalwarp [--help] [--long-usage] [--help-general]
[--quiet] [-overwrite] [-of <output_format>]
[-co <NAME>=<VALUE>]... [-s_srs <srs_def>] [-t_srs <srs_def>]
[[-srcalpha]|[-nosrcalpha]]
[-dstalpha] [-tr <xres> <yres>|square] [-ts <width> <height>]
[-te <xmin> <ymin> <xmax> <ymax>] [-te_srs <srs_def>]
[-r near|bilinear|cubic|cubicspline|lanczos|average|rms|mode|min|max|med|q1|q3|sum]
[-ot Byte|Int8|[U]Int{16|32|64}|CInt{16|32}|[C]Float{32|64}]
<src_dataset_name>... <dst_dataset_name>
Advanced options:
[-wo <NAME>=<VALUE>]... [-multi] [-s_coord_epoch <epoch>]
[-t_coord_epoch <epoch>] [-ct <string>]
[[-tps]|[-rpc]|[-geoloc]]
[-order <1|2|3>] [-refine_gcps <tolerance> [<minimum_gcps>]]
[-to <NAME>=<VALUE>]... [-et <err_threshold>]
[-wm <memory_in_mb>] [-srcnodata "<value>[ <value>]..."]
[-dstnodata "<value>[ <value>]..."] [-tap]
[-wt Byte|Int8|[U]Int{16|32|64}|CInt{16|32}|[C]Float{32|64}]
[-cutline <datasource>|<WKT>] [-cutline_srs <srs_def>]
[-cwhere <expression>]
[[-cl <layername>]|[-csql <query>]]
[-cblend <distance>] [-crop_to_cutline] [-nomd]
[-cvmd <meta_conflict_value>] [-setci] [-oo <NAME>=<VALUE>]...
[-doo <NAME>=<VALUE>]... [-ovr <level>|AUTO|AUTO-<n>|NONE]
[[-vshift]|[-novshiftgrid]]
[-if <format>]... [-srcband <band>]... [-dstband <band>]...
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.
- -srcband
<n>
- Added 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>
- Added 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>
- Added 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 were 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>
- Added 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 were 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, that is typically include a step proj=axisswap
order=2,1 at the beginning of the pipeline if the source CRS has
northing/easting axis order, and/or at the end of the pipeline if the
target CRS has northing/easting axis order.
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.
Added 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.
Added 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.
Added 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.
- -geoloc
- Force use of Geolocation Arrays.
- -et
<err_threshold>
- Error threshold for transformation approximation, expressed as a number of
source pixels. Defaults to 0.125 pixels unless 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.
Note 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_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. It does not necessarily mean that the output grid
aligns with the input grid.
- -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 how
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)
Added 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.
Defaults to 64 MB. Since GDAL 3.10, the value can be specified either as a
fixed amount of memory (e.g., -wm 200MB, -wm 1G) or as a
percentage of usable RAM (-wm 10%). In earlier versions, or if a
unit is not specified, the value is interpreted as being in megabytes if
the value is less than 10000. For values >=10000, it 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
- -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.
Added 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 --format 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>|<WKT>
- Enable use of a blend cutline from the name of a vector dataset. Starting
with GDAL 3.9, a WKT geometry string starting with POLYGON or MULTIPOLYGON
can also be specified.
- -csql
<query>
- Select cutline features using an SQL query instead of from a layer with
-cl.
- -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.
- <src_dataset_name>
- The source file name(s).
- <dst_dataset_name>
- The destination file name.
gdalwarp transforms images between different coordinate
reference systems and spatial resolutions.
First, gdalwarp must determine the extent and resolution of
the output, if these have not been specified using -te and
-tr. These are determined by transforming a sample of points from the
source CRS to the destination CRS. Details of the procedure can be found in
the documentation for GDALSuggestedWarpOutput(). If multiple inputs
are provided to gdalwarp, the output extent will be calculated to
cover all of them, at a resolution consistent with the highest-resolution
input.
Once the dimensions of the output image have been determined,
gdalwarp divides the output image into chunks that can be processed
independently within the amount of memory specified by -wm.
gdalwarp then iterates over scanlines in these chunks, and for each
output pixel determines a rectangular region of source pixels that
contribute to the value of the output pixel. The dimensions of this
rectangular region are typically determined by estimating the relative
scales of the source and destination raster, but can be manually specified
(see documentation of the XSCALE parameter in
GDALWarpOptions::papszWarpOptions). Because the source region is a
simple rectangle, it is not possible for an output pixel to be associated
with source pixels from both sides of the antimeridian or pole (when
transforming from geographic coordinates).
The rectangular region of source pixels is then provided to a
function that performs the resampling algorithm selected with -r.
Depending on the resampling algorithm and relative scales of the source and
destination rasters, source pixels may be weighted either according to the
approximate fraction of the source pixel that is covered by the destination
pixel (e.g., "mean" and "sum" resampling), or by
horizontal and vertical Cartesian distances between the center of the source
pixel and the center of the target pixel (e.g., bilinear or cubic spline
resampling). In the latter case, the relative weight of an individual source
pixel is determined by the product of the weights determined for its row and
column; the diagonal Cartesian distance is not calculated.
When multiple inputs are provided to gdalwarp, they are
processed independently in the order they are listed. This may introduce
edge effects near the boundaries of the input files, because output pixel
values will be derived from the final input only. To avoid this,
non-overlapping input files may first be combined into a VRT file
(e.g., using gdalbuildvrt). This will allow gdalwarp to use
pixels from all inputs when calculating output pixel values.
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
are assumed to 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.
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 (in this case, valid pixels
within the kernel radius would not be considered). 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
By default gdalwarp uses a linear approximator for the
transformations with a permitted error of 0.125 pixels in the source
dataset. The approximator precisely transforms three points per output
scanline (the start, middle, and end) from a row and column in the output
dataset to a row and column in the source dataset. It then compares a linear
approximation of the center point coordinates to the precisely transformed
value. If the sum of the horizontal and vertical errors is less than the
error threshold then the remaining source points are approximated using
linear interpolation between the start and middle point, and between the
middle and end 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 source dataset 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.
While gdalwarp is most commonly used to perform coordinate
transformations in the 2D space, it can also perform vertical
transformations. Vertical transformations are automatically performed when
the following two conditions are met:
- at least one of the source or target CRS has an explicit vertical CRS (as
part of a compound CRS) or is a 3D (generally geographic) CRS, and
- the raster has a single band
This mode can also be forced by using the -vshift (this is
essentially useful when the CRS involved are not explicitly 3D, but a
transformation pipeline is specified with -ct), or disabled with
-novshift.
When a vertical transformation is involved, typically a shift
value read in a geoid grid will be applied. This may require such grid(s) to
be installed, or PROJ networking capabilities to be enabled. Consult
PROJ documentation for more details. In addition to a shift, the
raster values may be multiplied by a factor to take into account vertical
unit changes. In priority, the value returned by
GDALRasterBand::GetUnitType() is used. The following values are
currently recognized: m, metre, metre, ft,
foot, US survey foot. If there is no defined unit type at the
band level, the vertical unit of the source CRS is used. The vertical unit
of the target CRS is also used to determine that conversion factor. The
conversion factor may be overridden by setting the
MULT_FACTOR_VERTICAL_SHIFT warping option with -wo. For
example -wo MULT_FACTOR_VERTICAL_SHIFT=1 to disable any vertical unit
change.
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.
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.
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:
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:
gdalwarp -overwrite in_dem.tif out_dem.tif -s_srs EPSG:4326+5773 -t_srs EPSG:4979
This utility is also callable from C with GDALWarp().
Frank Warmerdam <warmerdam@pobox.com>, Silke Reimer
<silke@intevation.de>
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