Welcome to mirror list, hosted at ThFree Co, Russian Federation.

git.blender.org/blender.git - Unnamed repository; edit this file 'description' to name the repository.
summaryrefslogtreecommitdiff
diff options
context:
space:
mode:
Diffstat (limited to 'intern/cycles/render/sky_model_data.h')
-rw-r--r--intern/cycles/render/sky_model_data.h29
1 files changed, 13 insertions, 16 deletions
diff --git a/intern/cycles/render/sky_model_data.h b/intern/cycles/render/sky_model_data.h
index 4171bd12756..e6f3f761532 100644
--- a/intern/cycles/render/sky_model_data.h
+++ b/intern/cycles/render/sky_model_data.h
@@ -4,7 +4,7 @@ This source is published under the following 3-clause BSD license.
Copyright (c) 2012 - 2013, Lukas Hosek and Alexander Wilkie
All rights reserved.
-Redistribution and use in source and binary forms, with or without
+Redistribution and use in source and binary forms, with or without
modification, are permitted provided that the following conditions are met:
* Redistributions of source code must retain the above copyright
@@ -12,8 +12,8 @@ modification, are permitted provided that the following conditions are met:
* Redistributions in binary form must reproduce the above copyright
notice, this list of conditions and the following disclaimer in the
documentation and/or other materials provided with the distribution.
- * None of the names of the contributors may be used to endorse or promote
- products derived from this software without specific prior written
+ * None of the names of the contributors may be used to endorse or promote
+ products derived from this software without specific prior written
permission.
THIS SOFTWARE IS PROVIDED BY THE COPYRIGHT HOLDERS AND CONTRIBUTORS "AS IS" AND
@@ -41,24 +41,24 @@ and the 2013 IEEE CG&A paper
"Adding a Solar Radiance Function to the Hosek Skylight Model"
- both by
+ both by
Lukas Hosek and Alexander Wilkie
Charles University in Prague, Czech Republic
Version: 1.4a, February 22nd, 2013
-
+
Version history:
1.4a February 22nd, 2013
- Removed unnecessary and counter-intuitive solar radius parameters
+ Removed unnecessary and counter-intuitive solar radius parameters
from the interface of the colourspace sky dome initialisation functions.
1.4 February 11th, 2013
Fixed a bug which caused the relative brightness of the solar disc
- and the sky dome to be off by a factor of about 6. The sun was too
- bright: this affected both normal and alien sun scenarios. The
+ and the sky dome to be off by a factor of about 6. The sun was too
+ bright: this affected both normal and alien sun scenarios. The
coefficients of the solar radiance function were changed to fix this.
1.3 January 21st, 2013 (not released to the public)
@@ -82,7 +82,7 @@ Version history:
the result of a simple conversion from spectral data via the CIE 2 degree
standard observer matching functions. Therefore, after multiplication
with 683 lm / W, the Y channel now corresponds to luminance in lm.
-
+
1.0 May 11th, 2012
Initial release.
@@ -96,15 +96,14 @@ CCL_NAMESPACE_BEGIN
/*
-This file contains the coefficient data for the XYZ colour space version of
+This file contains the coefficient data for the XYZ colour space version of
the model.
*/
// Uses Sep 9 pattern / Aug 23 mean dataset
-static const double datasetXYZ1[] =
-{
+static const double datasetXYZ1[] = {
// albedo 0, turbidity 1
-1.117001e+000,
-1.867262e-001,
@@ -3849,15 +3848,13 @@ static const double datasetXYZRad3[] =
-static const double* datasetsXYZ[] =
-{
+static const double* datasetsXYZ[] = {
datasetXYZ1,
datasetXYZ2,
datasetXYZ3
};
-static const double* datasetsXYZRad[] =
-{
+static const double* datasetsXYZRad[] = {
datasetXYZRad1,
datasetXYZRad2,
datasetXYZRad3