htrdr

Solving radiative transfer in heterogeneous media
git clone git://git.meso-star.fr/htrdr.git
Log | Files | Refs | README | LICENSE

commit de301c2ea98810954287d37388a5bb7ae18647e5
parent a96d16dbe2907170f93031ddd8f6d3d17aef170a
Author: Vincent Forest <vincent.forest@meso-star.com>
Date:   Thu,  4 Jun 2020 17:47:07 +0200

Fix the htrdr-image man page

Diffstat:
Mdoc/htrdr-image.5.txt | 2+-
1 file changed, 1 insertion(+), 1 deletion(-)

diff --git a/doc/htrdr-image.5.txt b/doc/htrdr-image.5.txt @@ -42,7 +42,7 @@ microseconds of the per radiative path computation time and its standard error. If the image is an infrared rendering (*-s* *lw*=_wlen-min_,_wlen_max_ option -in *htrdr(1)), the first and second pixel components store the expected value +in *htrdr*(1)), the first and second pixel components store the expected value and the standard error, respectively, of the estimated brightness temperature in Kelvin. The third and fourth components save the expected value and standard deviation of the pixel radiance that is either an integrated radiance in