Note: A new GRASS GIS stable version has been released: GRASS GIS 7.8, available here.

Updated manual page: here

The module has two different modes of operation: 1. Computes the entire horizon around a single point whose coordinates are given with the 'coord' option. The horizon height (in radians). 2. Computes one or more raster maps of the horizon height in a single direction. The input for this is the angle (in degrees), which is measured counterclockwise with east=0, north=90 etc. The output is the horizon height in radians.

**-d**- Write output in degrees (default is radians)
**-c**- Write output in compass orientation (default is CCW, East=0)
**--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

**elevation**=*name***[required]**- Name of input elevation raster map
**direction**=*float*- Direction in which you want to know the horizon height
**step**=*float*- Angle step size for multidirectional horizon [degrees]
**start**=*float*- Start angle for multidirectional horizon [degrees]
- Default:
*0.0* **end**=*float*- End angle for multidirectional horizon [degrees]
- Default:
*360.0* **bufferzone**=*float*- For horizon rasters, read from the DEM an extra buffer around the present region
**e_buff**=*float*- For horizon rasters, read from the DEM an extra buffer eastward the present region
**w_buff**=*float*- For horizon rasters, read from the DEM an extra buffer westward the present region
**n_buff**=*float*- For horizon rasters, read from the DEM an extra buffer northward the present region
**s_buff**=*float*- For horizon rasters, read from the DEM an extra buffer southward the present region
**maxdistance**=*float*- The maximum distance to consider when finding the horizon height
**output**=*basename*- Name for output basename raster map(s)
**coordinates**=*east,north*- Coordinate for which you want to calculate the horizon
**distance**=*float*- Sampling distance step coefficient (0.5-1.5)
- Default:
*1.0* **file**=*name*- Name of file for output (use output=- for stdout)
- Default:
*-*

- single point: as a series of horizon heights in the specified directions from the given point. The results are written to the stdout.
- raster: in this case the output is one or more raster maps, with each point in a raster giving the horizon height in a specific direction. One raster is created for each direction.

The directions are given as azimuthal angles (in degrees), with the angle starting with 0 towards East and moving counterclockwise (North is 90, etc.). The calculation takes into account the actual projection, so the angles are corrected for direction distortions imposed by it. The directions are thus aligned to those of the geographic projection and not the coordinate system given by the rows and columns of the raster map. This correction implies that the resulting cardinal directions represent true orientation towards the East, North, West and South. The only exception of this feature is LOCATION with x,y coordinate system, where this correction is not applied.

Using the **-c** flag, the azimuthal angles will be printed in compass
orientation (North=0, clockwise).

The *elevation* parameter is an input elevation raster map. If
the buffer options are used (see below), this raster should extend
over the area that accommodate the presently defined region plus
defined buffer zones.

The *step* parameter gives the angle step (in degrees)
between successive azimuthal directions for the calculation of the
horizon. Thus, a value of 5 for the *step* will give a total of
360/5=72 directions (72 raster maps if used in the raster map mode).

The *start* parameter gives the angle start (in degrees)
for the calculation of the horizon. The default value is 0 (East with
North being 90 etc.).

The *end* parameter gives the angle end (in degrees)
for the calculation of the horizon. The end point is omitted!
So for example if we run r.horizon with step=10, start=30 and end=70
the raster maps generated by r.horizon will be only for angles:
30, 40, 50, 60. The default value is 360.

The *direction* parameter gives the initial direction of the
first output. This parameter acts as an direction angle offset. For
example, if you want to get horizon angles for directions 45 and 225
degrees, the *direction* should be set to 45 and *step* to
180. If you only want one single direction, use this parameter to
specify desired direction of horizon angle, and set the *step*
size to 0 degrees. Otherwise all angles for a given starting *direction*
with step of *step* are calculated.

The *distance* controls the sampling distance step size for the
search for horizon along the line of sight. The default value is 1.0
meaning that the step size will be taken from the raster resolution.
Setting the value below 1.0 might slightly improve results for
directions apart from the cardinal ones, but increasing the
processing load of the search algorithm.

The *maxdistance* value gives a maximum distance to move away
from the origin along the line of sight in order to search for the
horizon height.
The default *maxdistance* is the full map extent.
The smaller this value the faster the calculation but
the higher the risk that you may miss a terrain feature that can
contribute significantly to the horizon outline. Note that a viewshed
can be calculated with *r.viewshed*.

The *coordinate* parameter takes a pair of easting-northing values
in the current coordinate system and calculates the values of angular
height of the horizon around this point. To achieve the
consistency of the results, the point coordinate is
aligned to the midpoint of the closest elevation raster cell.

If an analyzed point (or raster cell) lies close to the edge of
the defined region, the horizon calculation may not be realistic,
since it may not see some significant terrain features which could
have contributed to the horizon, because these features are outside
the region. There are to options how to set the size of the buffer
that is used to increase the area of the horizon analysis. The
*bufferzone* parameter allows you to specify the same size of
buffer for all cardinal directions and the parameters *e_buff*,
*n_buff*, *s_buff*, and *w_buff* allow you to specify
a buffer size individually for each of the four directions. The
buffer parameters influence only size of the read elevation map,
while the analysis in the raster mode will be done only for the
area specified by the current region definition.

The *output* parameter defines the basename of the output
horizon raster maps. The raster name of each horizon direction
raster will be constructed as *basename_*ANGLE, where ANGLE
is the angle in degrees with the direction. If you use **r.horizon**
in the single point mode this option will be ignored.

The *file* parameter allows saving the resulting horizon
angles in a comma separated ASCII file (single point mode only). If
you use **r.horizon** in the raster map mode this option will be ignored.

At the moment the elevation and maximum distance must be measured in meters, even if you use geographical coordinates (longitude/latitude). If your projection is based on distance (easting and northing), these too must be in meters. The buffer parameters must be in the same units as the raster coordinates (e.g., for latitude-longitude locations buffers are measured in degree unit).

The calculation method is based on the method used in **r.sun**
to calculate shadows. It starts at a very shallow angle and walks
along the line of sight and asks at each step whether the line of
sight "hits" the terrain. If so, the angle is increased to
allow the line of sight to pass just above the terrain at that point.
This is continued until the line of sight reaches a height that is
higher than any point in the region or until it reaches the border of
the region (see also the *bufferzone,e_buff*, *n_buff*,
*s_buff*, and *w_buff*). The the number of lines of sight (azimuth
directions) is determined from the *direction* and
*step* parameters. The method takes into account the curvature
of the Earth whereby remote features will seem to be lower than they
actually are. It also accounts for the changes of angles towards
cardinal directions caused by the projection (see above).

g.region raster=elevation -p r.horizon elevation=elevation direction=215 step=0 bufferzone=200 \ coordinates=638871.6,223384.4 maxdistance=5000

**Example 2**: determine horizon values starting at 90 deg (North),
step size of 5 deg, saving result as CSV file:

r.horizon elevation=elevation direction=90 step=5 bufferzone=200 \ coordinates=638871.6,223384.4 maxdistance=5000 file=horizon.csv

**Example 3**: test point near highway intersection, saving result
as CSV file for plotting the horizon around the highway intersection:

g.region n=223540 s=220820 w=634650 e=638780 res=10 -p r.horizon elevation=elevation direction=0 step=5 bufferzone=200 \ coordinates=636483.54,222176.25 maxdistance=5000 -d file=horizon.csv

Test point near high way intersection (North Carolina sample dataset)

Horizon angles for test point (CCW from East)

We can plot horizon in polar coordinates using Matplotlib in Python:

import numpy as np import matplotlib.pyplot as plt horizon = np.genfromtxt('horizon.csv', delimiter=',') horizon = horizon[1:, :] ax = plt.subplot(111, polar=True) bars = ax.plot(horizon[:, 0] / 180 * np.pi, (90 - horizon[:, 1]) / 180 * np.pi) # uncomment the 2 following lines when using -c flag # ax.set_theta_direction(-1) # ax.set_theta_zero_location('N') plt.show()

Horizon plot in polar coordinates.

g.region raster=elevation -p # we put a bufferzone of 10% of maxdistance around the study area # compute only direction between 90 and 270 degrees r.horizon elevation=elevation step=30 start=90 end=300 \ bufferzone=200 output=horangle maxdistance=5000

Hofierka J., 1997. Direct solar radiation modelling within an open GIS environment. Proceedings of JEC-GI'97 conference in Vienna, Austria, IOS Press Amsterdam, 575-584

Hofierka J., Huld T., Cebecauer T., Suri M., 2007. Open Source Solar Radiation Tools for Environmental and Renewable Energy Applications, International Symposium on Environmental Software Systems, Prague, 2007

Neteler M., Mitasova H., 2004. Open Source GIS: A GRASS GIS Approach, Springer, New York. ISBN: 1-4020-8064-6, 2nd Edition 2004 (reprinted 2005), 424 pages

Project PVGIS, European Commission, DG Joint Research Centre 2001-2007

Suri M., Hofierka J., 2004. A New GIS-based Solar Radiation Model and Its Application for Photovoltaic Assessments. Transactions in GIS, 8(2), 175-190

Thomas Huld, Joint Research Centre of
the European Commission, Ispra, Italy

Tomas Cebecauer, Joint Research Centre
of the European Commission, Ispra, Italy

Jaroslav Hofierka, GeoModel s.r.o.,
Bratislava, Slovakia

Marcel Suri, Joint Research Centre of the
European Commission, Ispra, Italy

© 2007, Thomas Huld, Tomas Cebecauer, Jaroslav Hofierka, Marcel Suri

Thomas.Huld@jrc.it Tomas.Cebecauer@jrc.it hofierka@geomodel.sk Marcel.Suri@jrc.it*Last changed: $Date$*

Available at: r.horizon source code (history)

Note: A new GRASS GIS stable version has been released: GRASS GIS 7.8, available here.

Updated manual page: here

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