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root/radiance/ray/src/rt/m_mist.c
Revision: 2.1
Committed: Fri Dec 8 21:27:10 1995 UTC (28 years, 4 months ago) by greg
Content type: text/plain
Branch: MAIN
Log Message:
Initial revision

File Contents

# Content
1 /* Copyright (c) 1995 Regents of the University of California */
2
3 #ifndef lint
4 static char SCCSid[] = "$SunId$ LBL";
5 #endif
6
7 /*
8 * Mist volumetric material.
9 */
10
11 #include "ray.h"
12
13 #include "source.h"
14
15 /*
16 * A mist volume is used to specify a region in the scene where a certain
17 * light source (or sources) is going to contribute to scattering. The
18 * material can add to the existing global medium, and override any ray
19 * settings for scattering albedo and eccentricity. Overlapping mist
20 * regions should agree w.r.t. albedo and eccentricity, and
21 * should have disjoint source lists.
22 *
23 * A pattern, if used, should compute the line integral of extinction,
24 * and will modify the first three arguments directly. This will tend
25 * to invalidate results when there are other objects intersected within
26 * the mist region.
27 *
28 * The string arguments for MAT_MIST are the identifiers for the important
29 * light sources, which will be looked up in the source array. The last
30 * source found matching a name is the one used. A relayed light source
31 * may be indicated by the relay surface name, followed by a '>' character,
32 * followed by the relayed source name (which may be another relay).
33 *
34 * Up to five real arguments may be given for MAT_MIST:
35 *
36 * [ext_r ext_g ext_b [albedo [gecc]]]
37 *
38 * The primaries indicate medium extinction per unit length (absorption
39 * plus scattering). The albedo is the ratio of scattering to extinction,
40 * and is set globally by the -ma option (salbedo) and overridden here.
41 * The Heyney-Greenstein eccentricity parameter (-mg seccg) indicates how much
42 * scattering favors the forward direction. A value of 0 means isotropic
43 * scattering. A value approaching 1 indicates strong forward scattering.
44 */
45
46 #define MAXSLIST 32 /* maximum sources to check */
47 #define RELAYDELIM '>' /* relay delimiter character */
48
49 extern COLOR cextinction; /* global coefficient of extinction */
50 extern double salbedo; /* global scattering albedo */
51 extern double seccg; /* global scattering eccentricity */
52
53
54 static int
55 inslist(sl, n) /* return index of source n if it's in list sl */
56 register int *sl;
57 register int n;
58 {
59 register int i;
60
61 for (i = sl[0]; i > 0; i--)
62 if (sl[i] == n)
63 return(i);
64 return(0);
65 }
66
67
68 static int
69 srcmatch(sn, id) /* check for an id match on a light source */
70 register int sn;
71 char *id;
72 {
73 extern char *index();
74 register char *cp;
75 again:
76 if (source[sn].so == NULL) /* just in case */
77 return(0);
78 if ((cp = index(id, RELAYDELIM)) != NULL) { /* relay source */
79 if (!(source[sn].sflags & SVIRTUAL))
80 return(0);
81 *cp = '\0';
82 if (strcmp(id, source[sn].so->oname)) {
83 *cp = RELAYDELIM;
84 return(0);
85 }
86 *cp = RELAYDELIM;
87 id = cp + 1; /* recurse */
88 sn = source[sn].sa.sv.sn;
89 goto again;
90 }
91 if (source[sn].sflags & SVIRTUAL)
92 return(0);
93 return(!strcmp(id, source[sn].so->oname));
94 }
95
96
97 m_mist(m, r) /* process a ray entering or leaving some mist */
98 OBJREC *m;
99 register RAY *r;
100 {
101 RAY p;
102 int *myslist = NULL;
103 int newslist[MAXSLIST+1];
104 COLOR mext;
105 double re, ge, be;
106 register int i, j;
107 /* check arguments */
108 if (m->oargs.nfargs > 5)
109 objerror(m, USER, "bad arguments");
110 if (m->oargs.nsargs > MAXSLIST)
111 objerror(m, USER, "too many sources in list");
112 /* get source indices */
113 if (m->oargs.nsargs > 0 && (myslist = (int *)m->os) == NULL) {
114 myslist = (int *)malloc((m->oargs.nsargs+1)*sizeof(int));
115 if (myslist == NULL)
116 goto memerr;
117 myslist[0] = m->oargs.nsargs; /* size is first in set */
118 for (j = myslist[0]; j > 0; j--) {
119 i = nsources; /* look up each source id */
120 while (i--)
121 if (srcmatch(i, m->oargs.sarg[j-1]))
122 break;
123 if (i < 0) {
124 sprintf(errmsg, "unknown source \"%s\"",
125 m->oargs.sarg[j-1]);
126 objerror(m, WARNING, errmsg);
127 } else
128 myslist[j] = i;
129 }
130 m->os = (char *)myslist;
131 }
132 if (m->oargs.nfargs > 2) { /* compute extinction */
133 setcolor(mext, m->oargs.farg[0], m->oargs.farg[1],
134 m->oargs.farg[2]);
135 raytexture(r, m->omod); /* get modifiers */
136 multcolor(mext, r->pcol);
137 } else
138 setcolor(mext, 0., 0., 0.);
139 /* start transmitted ray */
140 if (rayorigin(&p, r, TRANS, 1.) < 0)
141 return(1);
142 VCOPY(p.rdir, r->rdir);
143 p.slights = newslist;
144 if (r->slights != NULL)
145 for (j = r->slights[0]; j >= 0; j--)
146 p.slights[j] = r->slights[j];
147 else
148 p.slights[0] = 0;
149 if (r->rod > 0.) { /* entering ray */
150 addcolor(p.cext, mext);
151 if (m->oargs.nfargs > 3)
152 p.albedo = m->oargs.farg[3];
153 if (m->oargs.nfargs > 4)
154 p.gecc = m->oargs.farg[4];
155 if (myslist != NULL) /* add to list */
156 for (j = myslist[0]; j > 0; j--)
157 if (!inslist(p.slights, myslist[j])) {
158 if (p.slights[0] >= MAXSLIST)
159 error(USER,
160 "scattering source list overflow");
161 p.slights[++p.slights[0]] = myslist[j];
162 }
163 } else { /* leaving ray */
164 re = colval(r->cext,RED) - colval(mext,RED);
165 ge = colval(r->cext,GRN) - colval(mext,GRN);
166 be = colval(r->cext,BLU) - colval(mext,BLU);
167 setcolor(p.cext, re<0. ? 0. : re,
168 ge<0. ? 0. : ge,
169 be<0. ? 0. : be);
170 if (m->oargs.nfargs > 3)
171 p.albedo = salbedo;
172 if (m->oargs.nfargs > 4)
173 p.gecc = seccg;
174 if (myslist != NULL) { /* delete from list */
175 for (j = myslist[0]; j > 0; j--)
176 if (i = inslist(p.slights, myslist[j]))
177 p.slights[i] = -1;
178 for (i = 0, j = 1; j <= p.slights[0]; j++)
179 if (p.slights[j] != -1)
180 p.slights[++i] = p.slights[j];
181 p.slights[0] = i;
182 }
183 }
184 rayvalue(&p); /* calls rayparticipate() */
185 copycolor(r->rcol, p.rcol); /* return value */
186 r->rt = r->rot + p.rt;
187 return(1);
188 memerr:
189 error(SYSTEM, "out of memory in m_mist");
190 }