solstice

Compute collected power and efficiencies of a solar plant
git clone git://git.meso-star.com/solstice.git
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commit 6f9b761e8ce9b524737a77eeb31a1e93b520ad31
parent c2c5a1f834c93b7ea89170d06ba418d93714803d
Author: Vincent Forest <vincent.forest@meso-star.com>
Date:   Tue, 23 May 2017 11:49:00 +0200

Add a "rendering" section to the solstice-ouput man page

Diffstat:
Mdoc/solstice-output.5.txt | 8++++++++
1 file changed, 8 insertions(+), 0 deletions(-)

diff --git a/doc/solstice-output.5.txt b/doc/solstice-output.5.txt @@ -454,6 +454,14 @@ VTK-RADIATIVE-PATHS ::= # vtk DataFile Version 2.0 <path-vertex-id> ::= INTEGER _______ +RENDERING +--------- +When invoked with the *-r* option, *solstice*(1) generates an image of the +solar facility for each submitted sun direction. Each image is preceded by its +associated sun direction and is saved with respect to the ASCII PPM file +format [1]. The output images are actually greyscale images whose pixels store +the average normalized radiance that reaches them. + NOTES ----- 1. Portable PixMap - <http://netpbm.sourceforge.net/doc/ppm.html>