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greg |
2.1 |
#ifndef lint |
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greg |
2.10 |
static const char RCSid[] = "$Id$"; |
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greg |
2.1 |
#endif |
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/* |
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* Mist volumetric material. |
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*/ |
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greg |
2.10 |
/* ==================================================================== |
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* The Radiance Software License, Version 1.0 |
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* |
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* Copyright (c) 1990 - 2002 The Regents of the University of California, |
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* through Lawrence Berkeley National Laboratory. All rights reserved. |
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* |
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* Redistribution and use in source and binary forms, with or without |
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* modification, are permitted provided that the following conditions |
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* are met: |
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* |
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* 1. Redistributions of source code must retain the above copyright |
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* notice, this list of conditions and the following disclaimer. |
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* |
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* 2. Redistributions in binary form must reproduce the above copyright |
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* notice, this list of conditions and the following disclaimer in |
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* the documentation and/or other materials provided with the |
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* distribution. |
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* |
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* 3. The end-user documentation included with the redistribution, |
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* if any, must include the following acknowledgment: |
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* "This product includes Radiance software |
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* (http://radsite.lbl.gov/) |
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* developed by the Lawrence Berkeley National Laboratory |
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* (http://www.lbl.gov/)." |
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* Alternately, this acknowledgment may appear in the software itself, |
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* if and wherever such third-party acknowledgments normally appear. |
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* |
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* 4. The names "Radiance," "Lawrence Berkeley National Laboratory" |
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* and "The Regents of the University of California" must |
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* not be used to endorse or promote products derived from this |
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* software without prior written permission. For written |
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* permission, please contact [email protected]. |
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* |
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* 5. Products derived from this software may not be called "Radiance", |
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* nor may "Radiance" appear in their name, without prior written |
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* permission of Lawrence Berkeley National Laboratory. |
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* |
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* THIS SOFTWARE IS PROVIDED ``AS IS'' AND ANY EXPRESSED OR IMPLIED |
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* WARRANTIES, INCLUDING, BUT NOT LIMITED TO, THE IMPLIED WARRANTIES |
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* OF MERCHANTABILITY AND FITNESS FOR A PARTICULAR PURPOSE ARE |
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* DISCLAIMED. IN NO EVENT SHALL Lawrence Berkeley National Laboratory OR |
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* ITS CONTRIBUTORS BE LIABLE FOR ANY DIRECT, INDIRECT, INCIDENTAL, |
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* SPECIAL, EXEMPLARY, OR CONSEQUENTIAL DAMAGES (INCLUDING, BUT NOT |
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* LIMITED TO, PROCUREMENT OF SUBSTITUTE GOODS OR SERVICES; LOSS OF |
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* USE, DATA, OR PROFITS; OR BUSINESS INTERRUPTION) HOWEVER CAUSED AND |
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* ON ANY THEORY OF LIABILITY, WHETHER IN CONTRACT, STRICT LIABILITY, |
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* OR TORT (INCLUDING NEGLIGENCE OR OTHERWISE) ARISING IN ANY WAY OUT |
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* OF THE USE OF THIS SOFTWARE, EVEN IF ADVISED OF THE POSSIBILITY OF |
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* SUCH DAMAGE. |
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* ==================================================================== |
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* |
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* This software consists of voluntary contributions made by many |
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* individuals on behalf of Lawrence Berkeley National Laboratory. For more |
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* information on Lawrence Berkeley National Laboratory, please see |
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* <http://www.lbl.gov/>. |
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*/ |
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greg |
2.1 |
#include "ray.h" |
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#include "source.h" |
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/* |
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* A mist volume is used to specify a region in the scene where a certain |
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* light source (or sources) is going to contribute to scattering. The |
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* material can add to the existing global medium, and override any ray |
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* settings for scattering albedo and eccentricity. Overlapping mist |
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* regions should agree w.r.t. albedo and eccentricity, and |
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* should have disjoint source lists. |
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* |
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* A pattern, if used, should compute the line integral of extinction, |
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* and will modify the first three arguments directly. This will tend |
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* to invalidate results when there are other objects intersected within |
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* the mist region. |
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* |
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* The string arguments for MAT_MIST are the identifiers for the important |
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* light sources, which will be looked up in the source array. The last |
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* source found matching a name is the one used. A relayed light source |
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* may be indicated by the relay surface name, followed by a '>' character, |
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* followed by the relayed source name (which may be another relay). |
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* |
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* Up to five real arguments may be given for MAT_MIST: |
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* |
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greg |
2.6 |
* [ext_r ext_g ext_b [albedo_r albedo_g albedo_b [gecc]]] |
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greg |
2.1 |
* |
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* The primaries indicate medium extinction per unit length (absorption |
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greg |
2.5 |
* plus scattering), which is added to the global extinction coefficient, set |
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* by the -me option. The albedo is the ratio of scattering to extinction, |
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greg |
2.1 |
* and is set globally by the -ma option (salbedo) and overridden here. |
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* The Heyney-Greenstein eccentricity parameter (-mg seccg) indicates how much |
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* scattering favors the forward direction. A value of 0 means isotropic |
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* scattering. A value approaching 1 indicates strong forward scattering. |
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*/ |
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greg |
2.7 |
#ifndef MAXSLIST |
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#define MAXSLIST 32 /* maximum sources to check */ |
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#endif |
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greg |
2.1 |
#define RELAYDELIM '>' /* relay delimiter character */ |
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static int |
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inslist(sl, n) /* return index of source n if it's in list sl */ |
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register int *sl; |
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register int n; |
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{ |
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register int i; |
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for (i = sl[0]; i > 0; i--) |
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if (sl[i] == n) |
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return(i); |
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return(0); |
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} |
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static int |
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greg |
2.2 |
srcmatch(sp, id) /* check for an id match on a light source */ |
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register SRCREC *sp; |
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register char *id; |
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greg |
2.1 |
{ |
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extern char *index(); |
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register char *cp; |
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greg |
2.2 |
/* check for relay sources */ |
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while ((cp = index(id, RELAYDELIM)) != NULL) { |
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if (!(sp->sflags & SVIRTUAL) || sp->so == NULL) |
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greg |
2.1 |
return(0); |
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greg |
2.2 |
if (strncmp(id, sp->so->oname, cp-id) || sp->so->oname[cp-id]) |
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greg |
2.1 |
return(0); |
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greg |
2.2 |
id = cp + 1; /* relay to next */ |
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sp = source + sp->sa.sv.sn; |
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greg |
2.1 |
} |
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greg |
2.2 |
if (sp->sflags & SVIRTUAL || sp->so == NULL) |
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greg |
2.1 |
return(0); |
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greg |
2.2 |
return(!strcmp(id, sp->so->oname)); |
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greg |
2.1 |
} |
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greg |
2.10 |
static void |
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greg |
2.2 |
add2slist(r, sl) /* add source list to ray's */ |
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register RAY *r; |
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register int *sl; |
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{ |
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static int slspare[MAXSLIST+1]; /* in case of emergence */ |
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register int i; |
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if (sl == NULL || sl[0] == 0) /* nothing to add */ |
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return; |
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if (r->slights == NULL) |
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(r->slights = slspare)[0] = 0; /* just once per ray path */ |
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for (i = sl[0]; i > 0; i--) |
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if (!inslist(r->slights, sl[i])) { |
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if (r->slights[0] >= MAXSLIST) |
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gregl |
2.9 |
error(INTERNAL, |
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"scattering source list overflow"); |
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greg |
2.2 |
r->slights[++r->slights[0]] = sl[i]; |
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} |
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} |
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greg |
2.10 |
int |
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greg |
2.1 |
m_mist(m, r) /* process a ray entering or leaving some mist */ |
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OBJREC *m; |
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register RAY *r; |
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{ |
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RAY p; |
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int *myslist = NULL; |
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int newslist[MAXSLIST+1]; |
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COLOR mext; |
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double re, ge, be; |
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register int i, j; |
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/* check arguments */ |
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greg |
2.8 |
if (m->oargs.nfargs > 7) |
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greg |
2.1 |
objerror(m, USER, "bad arguments"); |
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/* get source indices */ |
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greg |
2.4 |
if (m->oargs.nsargs > 0 && (myslist = (int *)m->os) == NULL) { |
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greg |
2.2 |
if (m->oargs.nsargs > MAXSLIST) |
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gregl |
2.9 |
objerror(m, INTERNAL, "too many sources in list"); |
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greg |
2.1 |
myslist = (int *)malloc((m->oargs.nsargs+1)*sizeof(int)); |
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if (myslist == NULL) |
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goto memerr; |
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greg |
2.2 |
myslist[0] = 0; /* size is first in list */ |
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for (j = 0; j < m->oargs.nsargs; j++) { |
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greg |
2.1 |
i = nsources; /* look up each source id */ |
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while (i--) |
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greg |
2.2 |
if (srcmatch(source+i, m->oargs.sarg[j])) |
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greg |
2.1 |
break; |
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if (i < 0) { |
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sprintf(errmsg, "unknown source \"%s\"", |
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greg |
2.2 |
m->oargs.sarg[j]); |
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greg |
2.1 |
objerror(m, WARNING, errmsg); |
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greg |
2.2 |
} else if (inslist(myslist, i)) { |
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sprintf(errmsg, "duplicate source \"%s\"", |
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m->oargs.sarg[j]); |
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objerror(m, WARNING, errmsg); |
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greg |
2.1 |
} else |
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greg |
2.2 |
myslist[++myslist[0]] = i; |
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greg |
2.1 |
} |
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m->os = (char *)myslist; |
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} |
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if (m->oargs.nfargs > 2) { /* compute extinction */ |
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setcolor(mext, m->oargs.farg[0], m->oargs.farg[1], |
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m->oargs.farg[2]); |
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raytexture(r, m->omod); /* get modifiers */ |
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multcolor(mext, r->pcol); |
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} else |
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setcolor(mext, 0., 0., 0.); |
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/* start transmitted ray */ |
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if (rayorigin(&p, r, TRANS, 1.) < 0) |
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return(1); |
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VCOPY(p.rdir, r->rdir); |
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p.slights = newslist; |
218 |
greg |
2.2 |
if (r->slights != NULL) /* copy old list if one */ |
219 |
greg |
2.1 |
for (j = r->slights[0]; j >= 0; j--) |
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p.slights[j] = r->slights[j]; |
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else |
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p.slights[0] = 0; |
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if (r->rod > 0.) { /* entering ray */ |
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addcolor(p.cext, mext); |
225 |
greg |
2.6 |
if (m->oargs.nfargs > 5) |
226 |
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setcolor(p.albedo, m->oargs.farg[3], |
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m->oargs.farg[4], m->oargs.farg[5]); |
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if (m->oargs.nfargs > 6) |
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p.gecc = m->oargs.farg[6]; |
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greg |
2.2 |
add2slist(&p, myslist); /* add to list */ |
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} else { /* leaving ray */ |
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if (myslist != NULL) { /* delete from list */ |
233 |
greg |
2.1 |
for (j = myslist[0]; j > 0; j--) |
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greg |
2.2 |
if (i = inslist(p.slights, myslist[j])) |
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p.slights[i] = -1; |
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for (i = 0, j = 1; j <= p.slights[0]; j++) |
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if (p.slights[j] != -1) |
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p.slights[++i] = p.slights[j]; |
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if (p.slights[0] - i < myslist[0]) { /* fix old */ |
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addcolor(r->cext, mext); |
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greg |
2.6 |
if (m->oargs.nfargs > 5) |
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setcolor(r->albedo, m->oargs.farg[3], |
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m->oargs.farg[4], m->oargs.farg[5]); |
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if (m->oargs.nfargs > 6) |
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r->gecc = m->oargs.farg[6]; |
246 |
greg |
2.2 |
add2slist(r, myslist); |
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} |
248 |
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p.slights[0] = i; |
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} |
250 |
greg |
2.5 |
if ((re = colval(r->cext,RED) - colval(mext,RED)) < |
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colval(cextinction,RED)) |
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re = colval(cextinction,RED); |
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if ((ge = colval(r->cext,GRN) - colval(mext,GRN)) < |
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colval(cextinction,GRN)) |
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ge = colval(cextinction,GRN); |
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if ((be = colval(r->cext,BLU) - colval(mext,BLU)) < |
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colval(cextinction,BLU)) |
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be = colval(cextinction,BLU); |
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setcolor(p.cext, re, ge, be); |
260 |
greg |
2.6 |
if (m->oargs.nfargs > 5) |
261 |
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copycolor(p.albedo, salbedo); |
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if (m->oargs.nfargs > 6) |
263 |
greg |
2.1 |
p.gecc = seccg; |
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} |
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rayvalue(&p); /* calls rayparticipate() */ |
266 |
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copycolor(r->rcol, p.rcol); /* return value */ |
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r->rt = r->rot + p.rt; |
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return(1); |
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memerr: |
270 |
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error(SYSTEM, "out of memory in m_mist"); |
271 |
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} |