solstice

commit 62a98a1ba3b9ccd9a6ad3109407e4320b079a032
parent 63159677d75f384db01649b3efaaf5071fe0bafd
Author: Vincent Forest <vincent.forest@meso-star.com>
Date:   Wed, 17 May 2017 11:38:41 +0200

Fix typos

Diffstat:
M
doc/solstice-input.5.ronn
 | 
2
+-
M
doc/solstice.1.ronn.in
 | 
2
+-

2 files changed, 2 insertions(+), 2 deletions(-)
diff --git a/doc/solstice-input.5.ronn b/doc/solstice-input.5.ronn
@@ -727,7 +727,7 @@ around the X, Y and Z axis defined as:
 where `c<X|Y|Z>` and `s<X|Y|Z>` are the cosine and the sinus, respectively, of
 the rotation angles around the X, Y and Z axis.
 
-## EXAMPLE
+## EXAMPLES
 
 Declare 2 entities and a point source sun. The first entity is a purely
 specular square of size 10, whose center is at the origin. The second entity
diff --git a/doc/solstice.1.ronn.in b/doc/solstice.1.ronn.in
@@ -189,7 +189,7 @@ estimate the per-pixel radiance and fix the up camera vector to {`0`,`0`,`1`}.
 Write the `solstice-output`(5) result to standard output and use the `sed`(1)
 Unix command to remove the first line which stores the sun direction used to
 draw the image. Finally, visualise the rendered picture by redirecting the
-remaining data to the `feh`(5) image viewer.
+remaining data to the `feh`(1) image viewer.
 
     $ solstice -D180,45 -r up=0,0,1:rmode=pt:spp=64 solplant.yaml | sed '1d' | feh -