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root/radiance/ray/src/rt/m_mist.c
Revision: 2.10
Committed: Sat Feb 22 02:07:28 2003 UTC (21 years, 2 months ago) by greg
Content type: text/plain
Branch: MAIN
Changes since 2.9: +60 -9 lines
Log Message:
Changes and check-in for 3.5 release
Includes new source files and modifications not recorded for many years
See ray/doc/notes/ReleaseNotes for notes between 3.1 and 3.5 release

File Contents

# Content
1 #ifndef lint
2 static const char RCSid[] = "$Id$";
3 #endif
4 /*
5 * Mist volumetric material.
6 */
7
8 /* ====================================================================
9 * The Radiance Software License, Version 1.0
10 *
11 * Copyright (c) 1990 - 2002 The Regents of the University of California,
12 * through Lawrence Berkeley National Laboratory. All rights reserved.
13 *
14 * Redistribution and use in source and binary forms, with or without
15 * modification, are permitted provided that the following conditions
16 * are met:
17 *
18 * 1. Redistributions of source code must retain the above copyright
19 * notice, this list of conditions and the following disclaimer.
20 *
21 * 2. Redistributions in binary form must reproduce the above copyright
22 * notice, this list of conditions and the following disclaimer in
23 * the documentation and/or other materials provided with the
24 * distribution.
25 *
26 * 3. The end-user documentation included with the redistribution,
27 * if any, must include the following acknowledgment:
28 * "This product includes Radiance software
29 * (http://radsite.lbl.gov/)
30 * developed by the Lawrence Berkeley National Laboratory
31 * (http://www.lbl.gov/)."
32 * Alternately, this acknowledgment may appear in the software itself,
33 * if and wherever such third-party acknowledgments normally appear.
34 *
35 * 4. The names "Radiance," "Lawrence Berkeley National Laboratory"
36 * and "The Regents of the University of California" must
37 * not be used to endorse or promote products derived from this
38 * software without prior written permission. For written
39 * permission, please contact [email protected].
40 *
41 * 5. Products derived from this software may not be called "Radiance",
42 * nor may "Radiance" appear in their name, without prior written
43 * permission of Lawrence Berkeley National Laboratory.
44 *
45 * THIS SOFTWARE IS PROVIDED ``AS IS'' AND ANY EXPRESSED OR IMPLIED
46 * WARRANTIES, INCLUDING, BUT NOT LIMITED TO, THE IMPLIED WARRANTIES
47 * OF MERCHANTABILITY AND FITNESS FOR A PARTICULAR PURPOSE ARE
48 * DISCLAIMED. IN NO EVENT SHALL Lawrence Berkeley National Laboratory OR
49 * ITS CONTRIBUTORS BE LIABLE FOR ANY DIRECT, INDIRECT, INCIDENTAL,
50 * SPECIAL, EXEMPLARY, OR CONSEQUENTIAL DAMAGES (INCLUDING, BUT NOT
51 * LIMITED TO, PROCUREMENT OF SUBSTITUTE GOODS OR SERVICES; LOSS OF
52 * USE, DATA, OR PROFITS; OR BUSINESS INTERRUPTION) HOWEVER CAUSED AND
53 * ON ANY THEORY OF LIABILITY, WHETHER IN CONTRACT, STRICT LIABILITY,
54 * OR TORT (INCLUDING NEGLIGENCE OR OTHERWISE) ARISING IN ANY WAY OUT
55 * OF THE USE OF THIS SOFTWARE, EVEN IF ADVISED OF THE POSSIBILITY OF
56 * SUCH DAMAGE.
57 * ====================================================================
58 *
59 * This software consists of voluntary contributions made by many
60 * individuals on behalf of Lawrence Berkeley National Laboratory. For more
61 * information on Lawrence Berkeley National Laboratory, please see
62 * <http://www.lbl.gov/>.
63 */
64
65 #include "ray.h"
66
67 #include "source.h"
68
69 /*
70 * A mist volume is used to specify a region in the scene where a certain
71 * light source (or sources) is going to contribute to scattering. The
72 * material can add to the existing global medium, and override any ray
73 * settings for scattering albedo and eccentricity. Overlapping mist
74 * regions should agree w.r.t. albedo and eccentricity, and
75 * should have disjoint source lists.
76 *
77 * A pattern, if used, should compute the line integral of extinction,
78 * and will modify the first three arguments directly. This will tend
79 * to invalidate results when there are other objects intersected within
80 * the mist region.
81 *
82 * The string arguments for MAT_MIST are the identifiers for the important
83 * light sources, which will be looked up in the source array. The last
84 * source found matching a name is the one used. A relayed light source
85 * may be indicated by the relay surface name, followed by a '>' character,
86 * followed by the relayed source name (which may be another relay).
87 *
88 * Up to five real arguments may be given for MAT_MIST:
89 *
90 * [ext_r ext_g ext_b [albedo_r albedo_g albedo_b [gecc]]]
91 *
92 * The primaries indicate medium extinction per unit length (absorption
93 * plus scattering), which is added to the global extinction coefficient, set
94 * by the -me option. The albedo is the ratio of scattering to extinction,
95 * and is set globally by the -ma option (salbedo) and overridden here.
96 * The Heyney-Greenstein eccentricity parameter (-mg seccg) indicates how much
97 * scattering favors the forward direction. A value of 0 means isotropic
98 * scattering. A value approaching 1 indicates strong forward scattering.
99 */
100
101 #ifndef MAXSLIST
102 #define MAXSLIST 32 /* maximum sources to check */
103 #endif
104
105 #define RELAYDELIM '>' /* relay delimiter character */
106
107
108 static int
109 inslist(sl, n) /* return index of source n if it's in list sl */
110 register int *sl;
111 register int n;
112 {
113 register int i;
114
115 for (i = sl[0]; i > 0; i--)
116 if (sl[i] == n)
117 return(i);
118 return(0);
119 }
120
121
122 static int
123 srcmatch(sp, id) /* check for an id match on a light source */
124 register SRCREC *sp;
125 register char *id;
126 {
127 extern char *index();
128 register char *cp;
129 /* check for relay sources */
130 while ((cp = index(id, RELAYDELIM)) != NULL) {
131 if (!(sp->sflags & SVIRTUAL) || sp->so == NULL)
132 return(0);
133 if (strncmp(id, sp->so->oname, cp-id) || sp->so->oname[cp-id])
134 return(0);
135 id = cp + 1; /* relay to next */
136 sp = source + sp->sa.sv.sn;
137 }
138 if (sp->sflags & SVIRTUAL || sp->so == NULL)
139 return(0);
140 return(!strcmp(id, sp->so->oname));
141 }
142
143
144 static void
145 add2slist(r, sl) /* add source list to ray's */
146 register RAY *r;
147 register int *sl;
148 {
149 static int slspare[MAXSLIST+1]; /* in case of emergence */
150 register int i;
151
152 if (sl == NULL || sl[0] == 0) /* nothing to add */
153 return;
154 if (r->slights == NULL)
155 (r->slights = slspare)[0] = 0; /* just once per ray path */
156 for (i = sl[0]; i > 0; i--)
157 if (!inslist(r->slights, sl[i])) {
158 if (r->slights[0] >= MAXSLIST)
159 error(INTERNAL,
160 "scattering source list overflow");
161 r->slights[++r->slights[0]] = sl[i];
162 }
163 }
164
165
166 int
167 m_mist(m, r) /* process a ray entering or leaving some mist */
168 OBJREC *m;
169 register RAY *r;
170 {
171 RAY p;
172 int *myslist = NULL;
173 int newslist[MAXSLIST+1];
174 COLOR mext;
175 double re, ge, be;
176 register int i, j;
177 /* check arguments */
178 if (m->oargs.nfargs > 7)
179 objerror(m, USER, "bad arguments");
180 /* get source indices */
181 if (m->oargs.nsargs > 0 && (myslist = (int *)m->os) == NULL) {
182 if (m->oargs.nsargs > MAXSLIST)
183 objerror(m, INTERNAL, "too many sources in list");
184 myslist = (int *)malloc((m->oargs.nsargs+1)*sizeof(int));
185 if (myslist == NULL)
186 goto memerr;
187 myslist[0] = 0; /* size is first in list */
188 for (j = 0; j < m->oargs.nsargs; j++) {
189 i = nsources; /* look up each source id */
190 while (i--)
191 if (srcmatch(source+i, m->oargs.sarg[j]))
192 break;
193 if (i < 0) {
194 sprintf(errmsg, "unknown source \"%s\"",
195 m->oargs.sarg[j]);
196 objerror(m, WARNING, errmsg);
197 } else if (inslist(myslist, i)) {
198 sprintf(errmsg, "duplicate source \"%s\"",
199 m->oargs.sarg[j]);
200 objerror(m, WARNING, errmsg);
201 } else
202 myslist[++myslist[0]] = i;
203 }
204 m->os = (char *)myslist;
205 }
206 if (m->oargs.nfargs > 2) { /* compute extinction */
207 setcolor(mext, m->oargs.farg[0], m->oargs.farg[1],
208 m->oargs.farg[2]);
209 raytexture(r, m->omod); /* get modifiers */
210 multcolor(mext, r->pcol);
211 } else
212 setcolor(mext, 0., 0., 0.);
213 /* start transmitted ray */
214 if (rayorigin(&p, r, TRANS, 1.) < 0)
215 return(1);
216 VCOPY(p.rdir, r->rdir);
217 p.slights = newslist;
218 if (r->slights != NULL) /* copy old list if one */
219 for (j = r->slights[0]; j >= 0; j--)
220 p.slights[j] = r->slights[j];
221 else
222 p.slights[0] = 0;
223 if (r->rod > 0.) { /* entering ray */
224 addcolor(p.cext, mext);
225 if (m->oargs.nfargs > 5)
226 setcolor(p.albedo, m->oargs.farg[3],
227 m->oargs.farg[4], m->oargs.farg[5]);
228 if (m->oargs.nfargs > 6)
229 p.gecc = m->oargs.farg[6];
230 add2slist(&p, myslist); /* add to list */
231 } else { /* leaving ray */
232 if (myslist != NULL) { /* delete from list */
233 for (j = myslist[0]; j > 0; j--)
234 if (i = inslist(p.slights, myslist[j]))
235 p.slights[i] = -1;
236 for (i = 0, j = 1; j <= p.slights[0]; j++)
237 if (p.slights[j] != -1)
238 p.slights[++i] = p.slights[j];
239 if (p.slights[0] - i < myslist[0]) { /* fix old */
240 addcolor(r->cext, mext);
241 if (m->oargs.nfargs > 5)
242 setcolor(r->albedo, m->oargs.farg[3],
243 m->oargs.farg[4], m->oargs.farg[5]);
244 if (m->oargs.nfargs > 6)
245 r->gecc = m->oargs.farg[6];
246 add2slist(r, myslist);
247 }
248 p.slights[0] = i;
249 }
250 if ((re = colval(r->cext,RED) - colval(mext,RED)) <
251 colval(cextinction,RED))
252 re = colval(cextinction,RED);
253 if ((ge = colval(r->cext,GRN) - colval(mext,GRN)) <
254 colval(cextinction,GRN))
255 ge = colval(cextinction,GRN);
256 if ((be = colval(r->cext,BLU) - colval(mext,BLU)) <
257 colval(cextinction,BLU))
258 be = colval(cextinction,BLU);
259 setcolor(p.cext, re, ge, be);
260 if (m->oargs.nfargs > 5)
261 copycolor(p.albedo, salbedo);
262 if (m->oargs.nfargs > 6)
263 p.gecc = seccg;
264 }
265 rayvalue(&p); /* calls rayparticipate() */
266 copycolor(r->rcol, p.rcol); /* return value */
267 r->rt = r->rot + p.rt;
268 return(1);
269 memerr:
270 error(SYSTEM, "out of memory in m_mist");
271 }