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merge r.sun and r.in.xyz doc updates from devbr6

git-svn-id: https://svn.osgeo.org/grass/grass/trunk@37275 15284696-431f-4ddb-bdfa-cd5b030d7da7
Hamish Bowman 16 years ago
parent
commit
9146d73631
2 changed files with 24 additions and 9 deletions
  1. 8 3
      raster/r.in.xyz/r.in.xyz.html
  2. 16 6
      raster/r.sun2/r.sun.html

+ 8 - 3
raster/r.in.xyz/r.in.xyz.html

@@ -224,10 +224,15 @@ Development Team.
 <a href="r.to.rast3.html">r.to.rast3</a><br>
 <a href="r.to.rast3.html">r.to.rast3</a><br>
 <a href="r.to.vect.html">r.to.vect</a><br>
 <a href="r.to.vect.html">r.to.vect</a><br>
 <a href="r.univar.html">r.univar</a><br>
 <a href="r.univar.html">r.univar</a><br>
-<a href="r.univar.sh.html">r.univar.sh</a><br>
 <a href="v.in.ascii.html">v.in.ascii</a><br>
 <a href="v.in.ascii.html">v.in.ascii</a><br>
-<a href="v.out.ascii.html">v.out.ascii</a><br>
-<a href="v.surf.rst.html">v.surf.rst</a></i>
+<a href="v.surf.rst.html">v.surf.rst</a><br>
+<br>
+<a href="v.lidar.correction.html">v.lidar.correction</a>,
+<a href="v.lidar.edgedetection.html">v.lidar.edgedetection</a>,
+<a href="v.lidar.growing.html">v.lidar.growing</a>,
+<a href="v.outlier.html">v.outlier</a>,
+<a href="v.surf.bspline.html">v.surf.bspline</a>
+</i>
 <p>
 <p>
 <i><a href="http://www.ivarch.com/programs/pv.shtml">pv</a></i>
 <i><a href="http://www.ivarch.com/programs/pv.shtml">pv</a></i>
  - The UNIX pipe viewer utility
  - The UNIX pipe viewer utility

+ 16 - 6
raster/r.sun2/r.sun.html

@@ -86,12 +86,22 @@ A default, single value of Linke factor is <i>lin</i>=3.0 and
 is near the annual average for rural-city areas. The Linke
 is near the annual average for rural-city areas. The Linke
 factor for an absolutely clear atmosphere is <i>lin</i>=1.0. See notes below
 factor for an absolutely clear atmosphere is <i>lin</i>=1.0. See notes below
 to learn more about this factor. The incidence solar angle is the angle between
 to learn more about this factor. The incidence solar angle is the angle between
-horizon and solar beam vector. The solar radiation maps for given day are
-computed integrating the relevant irradiance between sunrise and sunset times
-for given day. The user can set finer or coarser time step <i>step</i> used 
-for all-day radiation calculations. A default value of <i>step</i> is 0.5 
-hour. Larger steps (e.g. 1.0-2.0) can speed-up calculations but produce less
-reliable results. The output units are in Wh per squared meter per given
+horizon and solar beam vector. 
+<P>
+The solar radiation maps for a given day are computed by integrating the
+relevant irradiance between sunrise and sunset times for that day. The
+user can set a finer or coarser time step used for all-day radiation
+calculations with the <i>step</i> option. The default value of <i>step</i> is
+0.5 hour. Larger steps (e.g. 1.0-2.0) can speed-up calculations but produce
+less reliable (and more jagged) results. As the sun moves through approx.
+15&deg of the sky in an hour, the default <i>step</i> of half an hour will
+produce 7.5&deg; steps in the data. For relatively smooth output with the
+sun placed for every degree of movement in the sky you should set the
+<i>step</i> to 4 minutes or less. <i>step</i><tt>=0.05</tt> is equivalent
+to every 3 minutes. Of course setting the time step to be very fine
+proportionally increases the module's running time.
+<P>
+The output units are in Wh per squared meter per given
 day [Wh/(m*m)/day]. The incidence angle and irradiance/irradiation maps can
 day [Wh/(m*m)/day]. The incidence angle and irradiance/irradiation maps can
 be computed without shadowing influence of relief by default or they can
 be computed without shadowing influence of relief by default or they can
 be computed with this influence using the flag <i>-s</i>. In mountainous areas
 be computed with this influence using the flag <i>-s</i>. In mountainous areas