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GDAL_VIEWSHED(1) GDAL GDAL_VIEWSHED(1) NAME gdal_viewshed - Calculates a viewshed raster from an input raster DEM for a user defined point SYNOPSIS gdal_viewshed [--help] [--help-general] [-b <band>] [-a_nodata <value>] [-f <formatname>] [-oz <observer_height>] [-tz <target_height>] [-md <max_distance>] -ox <observer_x> -oy <observer_y> [-vv <visibility>] [-iv <invisibility>] [-ov <out_of_range>] [-cc <curvature_coef>] [-os <observer_spacing>] [-j <relative job count>] [-co <NAME>=<VALUE>]... [-q] [-om <output mode>] <src_filename> <dst_filename> DESCRIPTION By default the gdal_viewshed generates a binary visibility raster from one band of the input raster elevation model (DEM). The output raster will be of type Byte. With the -mode flag can also return a minimum visible height raster of type Float64. NOTE: The algorithm as implemented currently will only output meaningful results if the georeferencing is in a projected coordinate reference system. --help Show this help message and exit --help-general Gives a brief usage message for the generic GDAL commandline op- tions and exit. -co <NAME>=<VALUE> Many formats have one or more optional creation options that can be used to control particulars about the file created. For in- stance, 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 op- tions 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 cre- ation options for each format. -b <band> Select an input band band containing the DEM data. Bands are numbered from 1. Only a single band can be used. Only the part of the raster within the specified maximum distance around the observer point is processed. -a_nodata <value> The value to be set for the cells in the output raster that have no data. NOTE: Currently, no special processing of input cells at a nodata value is done (which may result in erroneous results). -ox <value> The X position of the observer (in SRS units). If the coordi- nate is outside of the raster, all space between the observer and the raster is assumed not to occlude visibility of the raster. (Not supported in cumulative mode.) -oy <value> The Y position of the observer (in SRS units). If the coordi- nate is outside of the raster, all space between the observer and the raster is assumed not to occlude visibility of the raster. (Not supported in cumulative mode.) -oz <value> The height of the observer above the DEM surface in the height unit of the DEM. Default: 2 -tz <value> The height of the target above the DEM surface in the height unit of the DEM. Default: 0 -md <value> Maximum distance from observer to compute visibility. It is also used to clamp the extent of the output raster. (Not sup- ported in cumulative mode) -cc <value> Coefficient to consider the effect of the curvature and refrac- tion. When calculating visibility between two points (i.e. Line Of Sight or Viewshed), The magnitude of this effect varies with atmospheric conditions and depends on the wavelength. Different applications for calculating visibility use different interchangeable notation to describe this phenomena: Refraction Coefficient, Curvature Coefficient, and Sphere Diameter Factor. gdal_viewshed uses the Curvature Coefficient notation. {CurvCoeff}=1-{RefractionCoeff} Changes in air density curve the light downward causing an ob- server to see further and the earth to appear less curved, as if the sphere (earth) diameter is larger then it actually is. The ratio between that imaginary sphere diameter and the actual sphere diameter is given by the formula: {SphereDiameterFactor}=1/{CurvCoeff}=1/(1-{RefractionCoeff}) For visible light, the standard atmospheric refraction coeffi- cient that is generally used is 1/7. Thus the default value (since GDAL 3.4) for CurvCoeff that gdal_viewshed uses is 0.85714 (=~ 1-1/7) for Earth CRS. Starting with GDAL 3.6, for non-Earth CRS (those whole semi-major axis differs by more than 5% with the one of WGS 84), CurvCoeff default value is 1.0, to account for the no refraction use case. The height of the DEM is corrected according to the following formula: Height_{Corrected}=Height_{DEM}-{CurvCoeff}\frac{{TargetDistance}^2}{SphereDiameter} Typical coefficient values are given in the table below (use Curvature Coeff value for the cc option) ------------------------------------------------------------------------- Use Case Refraction Coeff Curvature Coeff Sphere Diameter Factor ------------------------------------------------------------------------- No Refraction 0 1 1 ------------------------------------------------------------------------- Visible Light 1/7 6/7 (=~0.85714) 7/6 (=~1.1666) ------------------------------------------------------------------------- Radio Waves 0.25 ~ 0.325 0.75 ~ 0.675 1.33 ~ 1.48 ------------------------------------------------------------------------- Flat Earth 1 0 inf +---------------+------------------+-----------------+------------------+ | | | | | -iv <value> | | | | | Pixel value to set for invisible areas. (Not supported in cumu- | | lative mode) Default: 0 | | | | | | | | -ov <value> | | | | | Pixel value|to set for the cells that fall outside of the range | | specified by the observer location and the maximum distance. | | (Not supported in cumulative mode) Default: 0 | | | | | | | -vv <value> | | | | | Pixel value|to set for visible|areas. (Not supported in cumula- | | tive mode) Default: 255 | | | | | | | | -om <output mode> | | | | | Sets what information the output contains. | | | | | | | | Possible values: NORMAL, DEM, GROUND, ACCUM | | | | | | | | NORMAL returns a raster of type Byte containing visible loca- | | tions. | | | | | | | | | | DEM and GROUND will return a raster of type Float64 containing | | the minimum target height for|target to be visible from the DEM | | surface or ground level respectively. Flags -tz, -iv and -vv | | will be ignored. | | | | | | | | | Cumulative (ACCUM) mode will create an eight bit|raster the same | | size as the|input raster where|each cell represents the relative | | observability from a grid of|observer points. |See the -os op- | | tion. | | | | | | | | | | Default NORMAL | | | | | | | | -os <value> | | | | | Cell Spacing between observers| (only supported| in cumulative | | mode) Default: 10 | | | | | | | | -j|<value> | | | | | Relative number of jobs to run|at once. (only supported in cumu- | | lative mode) Default: 3 | | | | | | | | C API | | | | | Functionality of| this utility |can be done |from C with | GDALViewshedGenerate(). | | | | | | | | EXAMPLE | | | | | Screenshot of 2 combined viewshed analysis, with the| yellow pixels | showing the area| that is visible from the both observation locations | (the green dots), while the small green area is only visible from one | location. | | | | [image] | | | | | | | | | Create a viewshed|raster with a radius of 500 for a person standing at | location (-10147017, 5108065). | | | | | | | | |gdal_viewshed -md 500 -ox -10147017 -oy 5108065 source.tif destination.tif REFERENCE [Wang2000] Generating Viewsheds without Using Sightlines. Wang, Jianjun, Robinson, Gary J., and White, Kevin. Photogrammetric Engineering and Remote Sensing. p81. https://www.asprs.org/wp-content/uploads/pers/2000journal/january/2000_jan_87-90.pdf AUTHOR Tamas Szekeres <szekerest@gmail.com> COPYRIGHT 1998-2025 Feb 11, 2025 GDAL_VIEWSHED(1)
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