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root/radiance/ray/src/gen/illum.cal
Revision: 2.2
Committed: Mon Aug 10 15:55:12 1992 UTC (31 years, 8 months ago) by greg
Branch: MAIN
Changes since 2.1: +28 -5 lines
Log Message:
eliminated star patterns at poles by adding pole interpolation

File Contents

# Content
1 { SCCSid "$SunId$ LBL" }
2
3 {
4 Coordinate computations for mkillum output.
5
6 For the spherical case, A1-A3 is the value at the positive pole,
7 A4-A6 is the value at the negative pole, and A7 is the pole influence:
8
9 il_alt - Altitude (1 to -1) for spherical coordinates
10 il_azi - Azimuth (0 to 2*PI) for sphere
11
12 For the hemispherical case, A1-A3 and A4 are the pole value and
13 influence, respectively, and A5-A13 are the unit vectors for the
14 hemisphere's coordinate system:
15
16 il_alth - Altitude (1 to 0) for hemispherical coordinates
17 il_azih - Azimuth (0 to 2*PI) for hemisphere
18 }
19
20 norm_rad(r) : if( r, r, r+2*PI );
21 { sphere coordinates }
22 il_alt = Dz;
23 il_azi = norm_rad(atan2(Dy, Dx));
24
25 s_val(v, vN, vS) = noneg(if( il_alt-A7,
26 linterp((il_alt-A7)/(1-A7), v, vN),
27 if ( -il_alt-A7,
28 linterp((-il_alt-A7)/(1-A7), v, vS),
29 v ),
30 v ));
31 { sphere values }
32 s_red(r,g,b) = s_val(r, A1, A4);
33 s_grn(r,g,b) = s_val(g, A2, A5);
34 s_blu(r,g,b) = s_val(b, A3, A6);
35 s_gry(r,g,b) = s_val(grey(r,g,b), grey(A1,A2,A3), grey(A4,A5,A6));
36
37 { hemisphere coordinates }
38 il_alth = sq(-Dx*arg(11)-Dy*arg(12)-Dz*arg(13));
39 il_azih = norm_rad(atan2(-Dx*arg(8)-Dy*arg(9)-Dz*arg(10),
40 -Dx*arg(5)-Dy*arg(6)-Dz*arg(7)));
41
42 h_val(v, vN) = noneg(if( il_alth-A4, linterp((il_alth-A4)/(1-A4), v, vN), v ));
43 { hemisphere values }
44 h_red(r,g,b) = h_val(r, A1);
45 h_grn(r,g,b) = h_val(g, A2);
46 h_blu(r,g,b) = h_val(b, A3);
47 h_gry(r,g,b) = h_val(grey(r,g,b), grey(A1,A2,A3));