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NAME

i.topo.corr - Computes topographic correction of reflectance.

KEYWORDS

imagery, terrain, topographic correction

SYNOPSIS

i.topo.corr
i.topo.corr --help
i.topo.corr [-is] [input=name[,name,...]] output=name basemap=name zenith=float [azimuth=float] [method=string] [--overwrite] [--help] [--verbose] [--quiet] [--ui]

Flags:

-i
Output sun illumination terrain model
-s
Scale output to input and copy color rules
--overwrite
Allow output files to overwrite existing files
--help
Print usage summary
--verbose
Verbose module output
--quiet
Quiet module output
--ui
Force launching GUI dialog

Parameters:

input=name[,name,...]
Name of reflectance raster maps to be corrected topographically
output=name [required]
Name (flag -i) or prefix for output raster maps
basemap=name [required]
Name of input base raster map (elevation or illumination)
zenith=float [required]
Solar zenith in degrees
azimuth=float
Solar azimuth in degrees (only if flag -i)
method=string
Topographic correction method
Options: cosine, minnaert, c-factor, percent
Default: c-factor

Table of contents

DESCRIPTION

i.topo.corr is used to topographically correct reflectance from imagery files, e.g. obtained with i.landsat.toar, using a sun illumination terrain model. This illumination model represents the cosine of the incident angle i, i.e. the angle between the normal to the ground and the sun rays.

Note: If needed, the sun position can be calculated for a given date and time with r.sunmask.

Figure showing terrain and solar angles
Figure showing terrain and solar angles

Using the -i flag and given an elevation basemap (metric), i.topo.corr creates a simple illumination model using the formula:

where,

For each band file, the corrected reflectance (ref_c) is calculate from the original reflectance (ref_o) using one of the four offered methods (one lambertian and two non-lambertian).

Method: cosine

Method: minnaert

where, k is obtained by linear regression of
ln(ref_o) = ln(ref_c) - k ln(cos_i/cos_z)

Method: c-factor

where, c is a/m from ref_o = a + m * cos_i

Method: percent

We can use cos_i to estimate the percent of solar incidence on the surface, then the transformation (cos_i + 1)/2 varied from 0 (surface in the side in opposition to the sun: infinite correction) to 1 (direct exhibition to the sun: no correction) and the corrected reflectance can be calculated as

NOTES

  1. The illumination model (cos_i) with flag -i uses the actual region as limits and the resolution of the elevation map.
  2. The topographic correction use the full reflectance file (null remain null) and its resolution.
  3. The elevation map to calculate the illumination model should be metric.

EXAMPLES

First, make a illumination model from the elevation map (here, SRTM). Then make perform the topographic correction of e.g. the bands toar.5, toar.4 and toar.3 with output as tcor.toar.5, tcor.toar.4, and tcor.toar.3 using c-factor (= c-correction) method:

# first pass: create illumination model
i.topo.corr -i base=SRTM zenith=33.3631 azimuth=59.8897 output=SRTM.illumination

# second pass: apply illumination model
i.topo.corr base=SRTM.illumination input=toar.5,toar.4,toar.3 output=tcor \
  zenith=33.3631 method=c-factor

REFERENCES

SEE ALSO

i.landsat.toar, r.mapcalc, r.sun r.sunmask

AUTHOR

E. Jorge Tizado (ej.tizado unileon es)
Dept. Biodiversity and Environmental Management, University of León, Spain

Figure derived from Neteler & Mitasova, 2008.

SOURCE CODE

Available at: i.topo.corr source code (history)

Latest change: Wednesday Sep 04 00:03:59 2024 in commit: 9222822ae60ae327d09c07ee9c40053762e4b7a3


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