1
2
3
4
5
6
7
8
9
10
11
12
13
14
15
16
17
18
19
20
21
22
23
24
25
26
27
28
29
30
31
32
33
34
35
36
37
38
39
40
41
42
43
44
45
46
47
48
49
50
51
52
53
54
55
56
57
58
59
60
61
62
63
64
65
66
67
68
69
70
71
72
73
74
75
76
77
78
79
80
81
82
83
84
85
86
87
88
89
90
91
92
93
94
95
96
97
98
99
100
101
102
103
104
105
106
107
108
109
110
111
112
113
114
115
116
117
118
119
120
121
122
123
124
125
126
127
128
129
|
/**
* @file class1/deferred/skyF.glsl
*
* $LicenseInfo:firstyear=2005&license=viewerlgpl$
* Second Life Viewer Source Code
* Copyright (C) 2005, Linden Research, Inc.
*
* This library is free software; you can redistribute it and/or
* modify it under the terms of the GNU Lesser General Public
* License as published by the Free Software Foundation;
* version 2.1 of the License only.
*
* This library is distributed in the hope that it will be useful,
* but WITHOUT ANY WARRANTY; without even the implied warranty of
* MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU
* Lesser General Public License for more details.
*
* You should have received a copy of the GNU Lesser General Public
* License along with this library; if not, write to the Free Software
* Foundation, Inc., 51 Franklin Street, Fifth Floor, Boston, MA 02110-1301 USA
*
* Linden Research, Inc., 945 Battery Street, San Francisco, CA 94111 USA
* $/LicenseInfo$
*/
// Inputs
in vec3 vary_HazeColor;
in float vary_LightNormPosDot;
#ifdef HAS_HDRI
in vec4 vary_position;
in vec3 vary_rel_pos;
uniform float sky_hdr_scale;
uniform float hdri_split_screen;
uniform mat3 env_mat;
uniform sampler2D environmentMap;
#endif
uniform sampler2D rainbow_map;
uniform sampler2D halo_map;
uniform float moisture_level;
uniform float droplet_radius;
uniform float ice_level;
out vec4 frag_data[4];
vec3 srgb_to_linear(vec3 c);
vec3 linear_to_srgb(vec3 c);
#define PI 3.14159265
/////////////////////////////////////////////////////////////////////////
// The fragment shader for the sky
/////////////////////////////////////////////////////////////////////////
vec3 rainbow(float d)
{
// 'Interesting' values of d are -0.75 .. -0.825, i.e. when view vec nearly opposite of sun vec
// Rainbox tex is mapped with REPEAT, so -.75 as tex coord is same as 0.25. -0.825 -> 0.175. etc.
// SL-13629
// Unfortunately the texture is inverted, so we need to invert the y coord, but keep the 'interesting'
// part within the same 0.175..0.250 range, i.e. d = (1 - d) - 1.575
d = clamp(-0.575 - d, 0.0, 1.0);
// With the colors in the lower 1/4 of the texture, inverting the coords leaves most of it inaccessible.
// So, we can stretch the texcoord above the colors (ie > 0.25) to fill the entire remaining coordinate
// space. This improves gradation, reduces banding within the rainbow interior. (1-0.25) / (0.425/0.25) = 4.2857
float interior_coord = max(0.0, d - 0.25) * 4.2857;
d = clamp(d, 0.0, 0.25) + interior_coord;
float rad = (droplet_radius - 5.0f) / 1024.0f;
return pow(texture(rainbow_map, vec2(rad+0.5, d)).rgb, vec3(1.8)) * moisture_level;
}
vec3 halo22(float d)
{
d = clamp(d, 0.1, 1.0);
float v = sqrt(clamp(1 - (d * d), 0, 1));
return texture(halo_map, vec2(0, v)).rgb * ice_level;
}
void main()
{
vec3 color;
#ifdef HAS_HDRI
vec3 frag_coord = vary_position.xyz/vary_position.w;
if (-frag_coord.x > ((1.0-hdri_split_screen)*2.0-1.0))
{
vec3 pos = normalize(vary_rel_pos);
pos = env_mat * pos;
vec2 texCoord = vec2(atan(pos.z, pos.x) + PI, acos(pos.y)) / vec2(2.0 * PI, PI);
color = textureLod(environmentMap, texCoord.xy, 0).rgb * sky_hdr_scale;
color = min(color, vec3(8192*8192*16)); // stupidly large value arrived at by binary search -- avoids framebuffer corruption from some HDRIs
frag_data[2] = vec4(0.0,0.0,0.0,GBUFFER_FLAG_HAS_HDRI);
}
else
#endif
{
// Potential Fill-rate optimization. Add cloud calculation
// back in and output alpha of 0 (so that alpha culling kills
// the fragment) if the sky wouldn't show up because the clouds
// are fully opaque.
color = vary_HazeColor;
float rel_pos_lightnorm = vary_LightNormPosDot;
float optic_d = rel_pos_lightnorm;
vec3 halo_22 = halo22(optic_d);
color.rgb += rainbow(optic_d);
color.rgb += halo_22;
color.rgb *= 2.;
color.rgb = clamp(color.rgb, vec3(0), vec3(5));
frag_data[2] = vec4(0.0,0.0,0.0,GBUFFER_FLAG_SKIP_ATMOS);
}
frag_data[1] = vec4(0);
#if defined(HAS_EMISSIVE)
frag_data[0] = vec4(0);
frag_data[3] = vec4(color.rgb, 1.0);
#else
frag_data[0] = vec4(color.rgb, 1.0);
#endif
}
|
