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root/radiance/src/cv/ies2rad.c

Comparing src/cv/ies2rad.c (file contents):
Revision 2.6 by greg, Thu Mar 18 11:21:21 1993 UTC vs.
Revision 2.32 by greg, Sat Dec 28 18:05:14 2019 UTC

#	Line 1 | Line 1
1	–	/* Copyright (c) 1992 Regents of the University of California */
2	–
1		#ifndef lint
2	<	static char SCCSid[] = "$SunId$ LBL";
2	>	static const char       RCSid[] = "$Id$";
3		#endif
6	–
4		/*
5	<	* Convert IES luminaire data to Radiance description
5	>	* ies2rad -- Convert IES luminaire data to Radiance description
6		*
7	+	* ies2rad converts an IES LM-63 luminare description to a Radiance
8	+	* luminaire description.  In addition, ies2rad manages a local
9	+	* database of Radiance luminaire files.
10	+	*
11	+	* Ies2rad generates two or three files for each luminaire. For a
12	+	* luminaire named LUM, ies2rad will generate LUM.rad, a Radiance
13	+	* scene description file which describes the light source, LUM.dat,
14	+	* which contains the photometric data from the IES LM-63 file, and
15	+	* (if tilt data is provided) LUM%.dat, which contains the tilt data
16	+	* from the IES file.
17	+	*
18	+	* Ies2rad is supported by the Radiance function files source.cal and
19	+	* tilt.cal, which transform the coordinates in the IES data into
20	+	* Radiance (θ,φ) luminaire coordinates and then apply photometric and
21	+	* tilt data to generate Radiance light. θ is altitude from the
22	+	* negative z-axis and φ is azimuth from the positive x-axis,
23	+	* increasing towards the positive y-axis. This system matches none of
24	+	* the usual goniophotometric conventions, but it is closest to IES
25	+	* type C; V in type C photometry is θ in Radiance and L is -φ.
26	+	*
27	+	* The ies2rad scene description for a luminaire LUM, with tilt data,
28	+	* uses the following Radiance scene description primitives:
29	+	*
30	+	*     void brightdata LUM_tilt
31	+	*     …
32	+	*     LUM_tilt brightdata LUM_dist
33	+	*     …
34	+	*     LUM_dist light LUM_light
35	+	*     …
36	+	*     LUM_light surface1 name1
37	+	*     …
38	+	*     LUM_light surface2 name2
39	+	*     …
40	+	*     LUM_light surface_n name_n
41	+	*
42	+	* Without tilt data, the primitives are:
43	+	*
44	+	*     void brightdata LUM_dist
45	+	*     …
46	+	*     LUM_dist light LUM_light
47	+	*     …
48	+	*     LUM_light surface1 name1
49	+	*     …
50	+	*     LUM_light surface2 name2
51	+	*     …
52	+	*     LUM_light surface_n name_n
53	+	*
54	+	* As many surfaces are given as required to describe the light
55	+	* source. Illum may be used rather than light so that a visible form
56	+	* (impostor) may be given to the luminaire, rather than a simple
57	+	* glowing shape. If an impostor is provided, it must be wholly
58	+	* contained within the illum and if it provides impostor light
59	+	* sources, those must be given with glow, so that they do not
60	+	* themselves illuminate the scene, providing incorrect results.
61	+	*
62	+	* The ies2rad code uses the "bsd" style. For emacs, this is set up
63	+	* automatically in the "Local Variables" section at the end of the
64	+	* file. For vim, use ":set tabstop=8 shiftwidth=8".
65	+	*
66		*      07Apr90         Greg Ward
67	+	*
68	+	*  Fixed correction factor for flat sources 29Oct2001 GW
69	+	*  Extensive comments added by Randolph Fritz May2018
70		*/
71
72	<	#include <stdio.h>
72	>	#include <math.h>
73		#include <ctype.h>
74	+
75	+	#include "rtio.h"
76		#include "color.h"
77		#include "paths.h"
78
79		#define PI              3.14159265358979323846
80	<	/* floating comparisons */
80	>
81	>	/* floating comparisons -- floating point numbers within FTINY of each
82	>	* other are considered equal */
83		#define FTINY           1e-6
84		#define FEQ(a,b)        ((a)<=(b)+FTINY&&(a)>=(b)-FTINY)
85	<	/* tilt specs */
85	>
86	>
87	>	/* IESNA LM-63 keywords and constants */
88	>	/* Since 1991, LM-63 files have begun with the magic keyword IESNA */
89	>	#define MAGICID         "IESNA"
90	>	#define LMAGICID        5
91	>	/* But newer files start with IESNA:LM-63- */
92	>	#define MAGICID2        "IESNA:LM-63-"
93	>	#define LMAGICID2       12
94	>	/* ies2rad supports the 1986, 1991, and 1995 versions of
95	>	* LM-63. FIRSTREV describes the first version; LASTREV describes the
96	>	* 1995 version. */
97	>	#define FIRSTREV        86
98	>	#define LASTREV         95
99	>
100	>	/* The following definitions support LM-63 file keyword reading and
101	>	* analysis.
102	>	*
103	>	* This section defines two function-like macros: keymatch(i,s), which
104	>	* checks to see if keyword i matches string s, and checklamp(s),
105	>	* which checks to see if a string matches the keywords "LAMP" or
106	>	* "LAMPCAT".
107	>	*
108	>	* LM-63-1986 files begin with a list of free-form label lines.
109	>	* LM-63-1991 files begin with the identifying line "IESNA91" followed
110	>	* by a list of formatted keywords.  LM-63-1995 files begin with the
111	>	* identifying line "IESNA:LM-63-1995" followed by a list of formatted
112	>	* keywords.
113	>	*
114	>	* The K_* #defines enumerate the keywords used in the different
115	>	* versions of the file and give them symbolic names.
116	>	*
117	>	* The D86, D91, and D95 #defines validate the keywords in the 1986,
118	>	* 1991, and 1995 versions of the standard, one bit per keyword.
119	>	* Since the 1986 standard does not use keywords, D86 is zero.  The
120	>	* 1991 standard has 13 keywords, and D91 has the lower 13 bits set.
121	>	* The 1995 standard has 14 keywords, and D95 has the lower 14 bits
122	>	* set.
123	>	*
124	>	*/
125	>	#define D86             0
126	>
127	>	#define K_TST           0
128	>	#define K_MAN           1
129	>	#define K_LMC           2
130	>	#define K_LMN           3
131	>	#define K_LPC           4
132	>	#define K_LMP           5
133	>	#define K_BAL           6
134	>	#define K_MTC           7
135	>	#define K_OTH           8
136	>	#define K_SCH           9
137	>	#define K_MOR           10
138	>	#define K_BLK           11
139	>	#define K_EBK           12
140	>
141	>	/* keywords defined in LM-63-1991 */
142	>	#define D91             ((1L<<13)-1)
143	>
144	>	#define K_LMG           13
145	>
146	>	/* keywords defined in LM-63-1995 */
147	>	#define D95             ((1L<<14)-1)
148	>
149	>	char    k_kwd[][20] = {"TEST", "MANUFAC", "LUMCAT", "LUMINAIRE", "LAMPCAT",
150	>	"LAMP", "BALLAST", "MAINTCAT", "OTHER", "SEARCH",
151	>	"MORE", "BLOCK", "ENDBLOCK", "LUMINOUSGEOMETRY"};
152	>
153	>	long k_defined[] = {D86, D86, D86, D86, D86, D91, D91, D91, D91, D95};
154	>
155	>	int     filerev = FIRSTREV;
156	>
157	>	#define keymatch(i,s)   (k_defined[filerev-FIRSTREV]&1L<<(i) &&\
158	>	k_match(k_kwd[i],s))
159	>
160	>	#define checklamp(s)    (!(k_defined[filerev-FIRSTREV]&(1<<K_LMP|1<<K_LPC)) ||\
161	>	keymatch(K_LMP,s) || keymatch(K_LPC,s))
162	>
163	>	/* tilt specs
164	>	*
165	>	* This next series of definitions address metal-halide lamps, which
166	>	* change their brightness depending on the angle at which they are
167	>	* mounted. The section begins with "TILT=".  The constants in this
168	>	* section are all defined in LM-63.
169	>	*
170	>	*/
171	>
172		#define TLTSTR          "TILT="
173		#define TLTSTRLEN       5
174		#define TLTNONE         "NONE"
#	Line 27 | Line 176 | static char SCCSid[] = "$SunId$ LBL";
176		#define TLT_VERT        1
177		#define TLT_H0          2
178		#define TLT_H90         3
179	<	/* photometric types */
179	>
180	>	/* Constants from LM-63 files */
181	>
182	>	/* photometric types
183	>	*
184	>	* This enumeration reflects three different methods of measuring the
185	>	* distribution of light from a luminaire -- "goniophotometry" -- and
186	>	* the different coordinate systems related to these
187	>	* goniophotometers.  All are described in IES standard LM-75-01.
188	>	* Earlier and shorter descriptions may be found the LM-63 standards
189	>	* from 1986, 1991, and 1995.
190	>	*
191	>	* ies2rad does not support type A photometry.
192	>	*
193	>	* In the 1986 file format, LM-63-86, 1 is used for type C and type A
194	>	* photometric data.
195	>	*
196	>	*/
197		#define PM_C            1
198		#define PM_B            2
199	<	/* unit types */
199	>	#define PM_A            3
200	>
201	>	/* unit types */
202		#define U_FEET          1
203		#define U_METERS        2
204	<	/* string lengths */
205	<	#define MAXLINE         132
206	<	#define MAXWORD         76
207	<	/* file types */
204	>
205	>	/* string lengths */
206	>	/* Maximum input line is 256 characters including CR LF at end. */
207	>	#define MAXLINE         257
208	>	#define RMAXWORD        76
209	>
210	>	/* End of LM-63-related #defines */
211	>
212	>	/* file extensions */
213		#define T_RAD           ".rad"
214		#define T_DST           ".dat"
215	<	#define T_TLT           "+.dat"
216	<	/* shape types */
215	>	#define T_TLT           "%.dat"
216	>	#define T_OCT           ".oct"
217	>
218	>	/* shape types
219	>	* These #defines enumerate the shapes of the Radiance objects which
220	>	* emit the light.
221	>	*/
222		#define RECT            1
223		#define DISK            2
224		#define SPHERE          3
225
226	<	#define MINDIM          .001            /* minimum dimension (point source) */
226	>	/* The diameter of a point source luminaire model. Also the minimum
227	>	* size (in meters) that the luminous opening of a luminaire must have
228	>	* to be treated as other than a point source. */
229	>	#define MINDIM          .001
230
231	<	#define F_M             .3048           /* feet to meters */
231	>	/* feet to meters */
232	>	/* length_in_meters = length_in_feet * F_M */
233	>	#define F_M             .3048
234
235	+	/* abspath - return true if a path begins with a directory separator
236	+	* or a '.' (current directory) */
237		#define abspath(p)      (ISDIRSEP((p)[0]) || (p)[0] == '.')
238
239	+	/* Global variables.
240	+	*
241	+	* Mostly, these are a way of communicating command line parameters to
242	+	* the rest of the program.
243	+	*/
244		static char     default_name[] = "default";
245
246		char    *libdir = NULL;                 /* library directory location */
#	Line 64 | Line 254 | float  defcolor[3] = {1.,1.,1.};       /* default lamp color
254		float   *lampcolor = defcolor;          /* pointer to current lamp color */
255		double  multiplier = 1.0;               /* multiplier for all light sources */
256		char    units[64] = "meters";           /* output units */
257	+	int     out2stdout = 0;                 /* put out to stdout r.t. file */
258	+	int     instantiate = 0;                /* instantiate geometry */
259		double  illumrad = 0.0;                 /* radius for illum sphere */
260
261	+	/* This struct describes the Radiance source object */
262		typedef struct {
263	+	int     isillum;                        /* do as illum */
264		int     type;                           /* RECT, DISK, SPHERE */
265	+	double  mult;                           /* candela multiplier */
266		double  w, l, h;                        /* width, length, height */
267		double  area;                           /* max. projected area */
268	<	} SHAPE;                                /* a source shape */
268	>	} SRCINFO;                              /* a source shape (units=meters) */
269
270	<	int     gargc;                          /* global argc (minus filenames) */
270	>	/* A count and pointer to the list of input file names */
271	>	int     gargc;                          /* global argc */
272		char    **gargv;                        /* global argv */
273
274	<	extern char     *strcpy(), *strcat(), *stradd(), *tailtrunc(), *filetrunc(),
275	<	*filename(), *libname(), *fullname(), *malloc(),
276	<	*getword(), *atos();
277	<	extern float    *matchlamp();
278	<
274	>	/* macros to scan numbers out of IES files
275	>	*
276	>	* fp is a file pointer.  scnint() places the number in the integer
277	>	* indicated by ip; scnflt() places the number in the double indicated
278	>	* by rp. The macros return 1 if successful, 0 if not.
279	>	*
280	>	*/
281		#define scnint(fp,ip)   cvtint(ip,getword(fp))
282		#define scnflt(fp,rp)   cvtflt(rp,getword(fp))
85	–	#define isint           isflt                   /* IES allows real as integer */
283
284	+	/* The original (1986) version of LM-63 allows decimals points in
285	+	* integers, so that, for instance, the number of lamps may be written
286	+	* 3.0 (the number, obviously, must still be an integer.) This
287	+	* confusing define accommodates that.  */
288	+	#define isint           isflt
289
290	<	main(argc, argv)
291	<	int     argc;
292	<	char    *argv[];
290	>	/* Function declarations */
291	>	static int ies2rad(char *inpname, char *outname);
292	>	static void initlamps(void);
293	>	static int dosource(SRCINFO *sinf, FILE *in, FILE *out, char *mod, char *name);
294	>	static int dotilt(FILE *in, FILE *out, char *dir, char *tltspec,
295	>	char *dfltname, char *tltid);
296	>	static int cvgeometry(char *inpname, SRCINFO *sinf, char *outname, FILE *outfp);
297	>	static int cvtint(int *ip, char *wrd);
298	>	static int cvdata(FILE *in, FILE *out, int ndim, int npts[], double mult,
299	>	double lim[][2]);
300	>	static int cvtflt(double *rp, char *wrd);
301	>	static int makeshape(SRCINFO *shp, double width, double length, double height);
302	>	static int putsource(SRCINFO *shp, FILE *fp, char *mod, char *name,
303	>	int dolower, int doupper, int dosides);
304	>	static void putrectsrc(SRCINFO *shp, FILE *fp, char *mod, char *name, int up);
305	>	static void putsides(SRCINFO *shp, FILE *fp, char *mod, char *name);
306	>	static void putdisksrc(SRCINFO *shp, FILE *fp, char *mod, char *name, int up);
307	>	static void putspheresrc(SRCINFO *shp, FILE *fp, char *mod, char *name);
308	>	static void putrect(SRCINFO *shp, FILE *fp, char *mod, char *name, char *suffix,
309	>	int a, int b, int c, int d);
310	>	static void putpoint(SRCINFO *shp, FILE *fp, int p);
311	>	static void putcyl(SRCINFO *shp, FILE *fp, char *mod, char *name);
312	>	static char * tailtrunc(char *name);
313	>	static char * filename(char *path);
314	>	static char * libname(char *path, char *fname, char *suffix);
315	>	static char * getword(FILE *fp);
316	>	static char * fullnam(char *path, char *fname, char *suffix);
317	>
318	>	/* main - process arguments and run the conversion
319	>	*
320	>	* Refer to the man page for details of the arguments.
321	>	*
322	>	* Following Unix environment conventions, main() exits with 0 on
323	>	* success and 1 on failure.
324	>	*
325	>	* ies2rad outputs either two or three files for a given IES
326	>	* file. There is always a .rad file containing Radiance scene
327	>	* description primitives and a .dat file for the photometric data. If
328	>	* tilt data is given, that is placed in a separate .dat file.  So
329	>	* ies2rad must have a filename to operate. Sometimes this name is the
330	>	* input file name, shorn of its extension; sometimes it is given in
331	>	* the -o option. But an output file name is required for ies2rad to
332	>	* do its work.
333	>	*
334	>	* Older versions of the LM-63 standard allowed inclusion of multiple
335	>	* luminaires in one IES file; this is not supported by ies2rad.
336	>	*
337	>	* This code sometimes does not check to make sure it has not run out
338	>	* of arguments; this can lead to segmentation faults and perhaps
339	>	* other errors.
340	>	*
341	>	*/
342	>	int
343	>	main(
344	>	int     argc,
345	>	char    *argv[]
346	>	)
347		{
348		char    *outfile = NULL;
349		int     status;
350	<	char    outname[MAXWORD];
350	>	char    outname[RMAXWORD];
351		double  d1;
352		int     i;
353	<
353	>
354	>	/* Scan the options */
355		for (i = 1; i < argc && argv[i][0] == '-'; i++)
356		switch (argv[i][1]) {
357		case 'd':               /* dimensions */
#	Line 156 | Line 413 | char   *argv[];
413		case 'f':               /* lamp data file */
414		lampdat = argv[++i];
415		break;
416	<	case 'o':               /* output file name */
416	>	case 'o':               /* output file root name */
417		outfile = argv[++i];
418		break;
419	+	case 's':               /* output to stdout */
420	+	out2stdout = !out2stdout;
421	+	break;
422		case 'i':               /* illum */
423		illumrad = atof(argv[++i]);
164	–	if (illumrad < MINDIM)
165	–	illumrad = MINDIM;
424		break;
425	+	case 'g':               /* instantiate geometry? */
426	+	instantiate = !instantiate;
427	+	break;
428		case 't':               /* override lamp type */
429		lamptype = argv[++i];
430		break;
#	Line 184 | Line 445 | char   *argv[];
445		argv[0], argv[i]);
446		exit(1);
447		}
448	+	/* Save pointers to the list of input file names */
449		gargc = i;
450		gargv = argv;
451	<	initlamps();                    /* get lamp data (if needed) */
452	<	/* convert ies file(s) */
451	>
452	>	/* get lamp data (if needed) */
453	>	initlamps();
454	>
455	>	/* convert ies file(s) */
456	>	/* If an output file name is specified */
457		if (outfile != NULL) {
458		if (i == argc)
459	+	/* If no input filename is given, use stdin as
460	+	* the source for the IES file */
461		exit(ies2rad(NULL, outfile) == 0 ? 0 : 1);
462		else if (i == argc-1)
463	+	/* If exactly one input file name is given, use it. */
464		exit(ies2rad(argv[i], outfile) == 0 ? 0 : 1);
465	<	else {
466	<	fprintf(stderr, "%s: single input file required\n",
198	<	argv[0]);
199	<	exit(1);
200	<	}
465	>	else
466	>	goto needsingle; /* Otherwise, error. */
467		} else if (i >= argc) {
468	+	/* If an output file and an input file are not give, error. */
469		fprintf(stderr, "%s: missing output file specification\n",
470		argv[0]);
471		exit(1);
472		}
473	+	/* If no input or output file is given, error. */
474	+	if (out2stdout && i != argc-1)
475	+	goto needsingle;
476	+	/* Otherwise, process each input file in turn. */
477		status = 0;
478		for ( ; i < argc; i++) {
479		tailtrunc(strcpy(outname,filename(argv[i])));
#	Line 210 | Line 481 | char   *argv[];
481		status = 1;
482		}
483		exit(status);
484	+	needsingle:
485	+	fprintf(stderr, "%s: single input file required\n", argv[0]);
486	+	exit(1);
487		}
488
489	<
490	<	initlamps()                             /* set up lamps */
489	>	/* Initlamps -- If necessary, read lamp data table */
490	>	void
491	>	initlamps(void)                         /* set up lamps */
492		{
493		float   *lcol;
494		int     status;
495
496	+	/* If the lamp name is set to default, don't bother to read
497	+	* the lamp data table. */
498		if (lamptype != NULL && !strcmp(lamptype, default_name) &&
499		deflamp == NULL)
500	<	return;                         /* no need for data */
501	<	/* else load file */
502	<	if ((status = loadlamps(lampdat)) < 0)
503	<	exit(1);
500	>	return;
501	>
502	>	if ((status = loadlamps(lampdat)) < 0) /* Load the lamp data table */
503	>	exit(1);                       /* Exit if problems
504	>	* with the file. */
505		if (status == 0) {
506	+	/* If can't open the file, just use the standard default lamp */
507		fprintf(stderr, "%s: warning - no lamp data\n", lampdat);
508		lamptype = default_name;
509		return;
510		}
511	<	if (deflamp != NULL) {                  /* match default type */
511	>	if (deflamp != NULL) {
512	>	/* Look up the specified default lamp type */
513		if ((lcol = matchlamp(deflamp)) == NULL)
514	+	/* If it can't be found, use the default */
515		fprintf(stderr,
516		"%s: warning - unknown default lamp type\n",
517		deflamp);
518		else
519	+	/* Use the selected default lamp color */
520		copycolor(defcolor, lcol);
521		}
522	<	if (lamptype != NULL) {                 /* match selected type */
522	>	/* If a lamp type is specified and can be found, use it, and
523	>	* release the lamp data table memory; it won't be needed any more. */
524	>	if (lamptype != NULL) {
525		if (strcmp(lamptype, default_name)) {
526		if ((lcol = matchlamp(lamptype)) == NULL) {
527		fprintf(stderr,
#	Line 249 | Line 533 | initlamps()                            /* set up lamps */
533		}
534		freelamps();                    /* all done with data */
535		}
536	<	/* else keep lamp data */
536	>	/* else keep lamp data */
537		}
538
539	+	/*
540	+	* File path operations
541	+	*
542	+	* These provide file path operations that operate on both MS-Windows
543	+	* and *nix. They will ignore and pass, but will not necessarily
544	+	* process correctly, Windows drive letters. Paths including Windows
545	+	* UNC network names (\\server\folder\file) may also cause problems.
546	+	*
547	+	*/
548
549	+	/*
550	+	* stradd()
551	+	*
552	+	* Add a string to the end of a string, optionally concatenating a
553	+	* file path separator character.  If the path already ends with a
554	+	* path separator, no additional separator is appended.
555	+	*
556	+	*/
557		char *
558	<	stradd(dst, src, sep)                   /* add a string at dst */
559	<	register char   *dst, *src;
560	<	int     sep;
558	>	stradd(                 /* add a string at dst */
559	>	char    *dst,
560	>	char    *src,
561	>	int     sep
562	>	)
563		{
564		if (src && *src) {
565		do
#	Line 269 | Line 572 | int    sep;
572		return(dst);
573		}
574
575	<
575	>	/*
576	>	* fullnam () - return a usable path name for an output file
577	>	*/
578		char *
579	<	fullname(path, fname, suffix)           /* return full path name */
580	<	char    *path, *fname, *suffix;
579	>	fullnam(
580	>	char    *path,          /* The base directory path */
581	>	char    *fname,         /* The file name */
582	>	char    *suffix         /* A suffix, which usually contains
583	>	* a file name extension. */
584	>	)
585		{
586	+	extern char *prefdir;
587	+	extern char *libdir;
588	+
589		if (prefdir != NULL && abspath(prefdir))
590	+	/* If the subdirectory path is absolute or '.', just
591	+	* concatenate the names together */
592		libname(path, fname, suffix);
593		else if (abspath(fname))
594	+	/* If there is no subdirectory, and the file name is
595	+	* an absolute path or '.', concatenate the path,
596	+	* filename, and suffix. */
597		strcpy(stradd(path, fname, 0), suffix);
598		else
599	+	/* If the file name is relative, concatenate path,
600	+	* library directory, directory separator, file name,
601	+	* and suffix.  */
602		libname(stradd(path, libdir, DIRSEP), fname, suffix);
603
604		return(path);
605		}
606
607
608	+	/*
609	+	* libname - convert a file name to a path
610	+	*/
611		char *
612	<	libname(path, fname, suffix)            /* return library relative name */
613	<	char    *path, *fname, *suffix;
612	>	libname(
613	>	char    *path,          /* The base directory path */
614	>	char    *fname,         /* The file name */
615	>	char    *suffix         /* A suffix, which usually contains
616	>	* a file name extension. */
617	>	)
618		{
619	+	extern char *prefdir;   /* The subdirectory where the file
620	+	* name is stored. */
621	+
622		if (abspath(fname))
623	+	/* If the file name begins with '/' or '.', combine
624	+	* it with the path and attach the suffix */
625		strcpy(stradd(path, fname, 0), suffix);
626		else
627	+	/* If the file name is relative, attach it to the
628	+	* path, include the subdirectory, and append the suffix. */
629		strcpy(stradd(stradd(path, prefdir, DIRSEP), fname, 0), suffix);
630
631		return(path);
632		}
633
634	<
634	>	/* filename - find the base file name in a buffer containing a path
635	>	*
636	>	* The pointer is to a character within the buffer, not a string in itself;
637	>	* it will become invalid when the buffer is freed.
638	>	*
639	>	*/
640		char *
641	<	filename(path)                  /* get final component of pathname */
642	<	register char   *path;
641	>	filename(
642	>	char    *path
643	>	)
644		{
645	<	register char   *cp;
645	>	char    *cp;
646
647		for (cp = path; *path; path++)
648		if (ISDIRSEP(*path))
#	Line 311 | Line 651 | register char  *path;
651		}
652
653
654	+	/* filetrunc() - return the directory portion of a path
655	+	*
656	+	* The path is passed in in a pointer to a buffer; a null character is
657	+	* inserted in the buffer after the last directory separator
658	+	*
659	+	*/
660		char *
661	<	filetrunc(path)                         /* truncate filename at end of path */
662	<	char    *path;
661	>	filetrunc(
662	>	char    *path
663	>	)
664		{
665	<	register char   *p1, *p2;
665	>	char    *p1, *p2;
666
667		for (p1 = p2 = path; *p2; p2++)
668		if (ISDIRSEP(*p2))
669		p1 = p2;
670	+	if (p1 == path && ISDIRSEP(*p1))
671	+	p1++;
672		*p1 = '\0';
673		return(path);
674		}
675
676	<
676	>	/* tailtrunc() - trim a file name extension, if any.
677	>	*
678	>	* The file name is passed in in a buffer indicated by *name; the
679	>	* period which begins the extension is replaced with a 0 byte.
680	>	*/
681		char *
682	<	tailtrunc(name)                         /* truncate tail of filename */
683	<	char    *name;
682	>	tailtrunc(
683	>	char    *name
684	>	)
685		{
686	<	register char   *p1, *p2;
686	>	char    *p1, *p2;
687
688	+	/* Skip leading periods */
689		for (p1 = filename(name); *p1 == '.'; p1++)
690		;
691	+	/* Find the last period in a file name */
692		p2 = NULL;
693		for ( ; *p1; p1++)
694		if (*p1 == '.')
695		p2 = p1;
696	+	/* If present, trim the filename at that period */
697		if (p2 != NULL)
698		*p2 = '\0';
699		return(name);
700		}
701
702	<
703	<	blanktrunc(s)                           /* truncate spaces at end of line */
704	<	char    *s;
702	>	/* blanktrunc() - trim spaces at the end of a string
703	>	*
704	>	* the string is passed in a character array, which is modified
705	>	*/
706	>	void
707	>	blanktrunc(
708	>	char    *s
709	>	)
710		{
711	<	register char   *cp;
711	>	char    *cp;
712
713		for (cp = s; *cp; cp++)
714		;
#	Line 355 | Line 717 | char   *s;
717		*++cp = '\0';
718		}
719
720	+	/* k_match - return true if keyword matches header line */
721	+	int
722	+	k_match(
723	+	char    *kwd,           /* keyword */
724	+	char    *hdl            /* header line */
725	+	)
726	+	{
727	+	/* Skip leading spaces */
728	+	while (isspace(*hdl))
729	+	hdl++;
730	+	/* The line has to begin with '[' */
731	+	if (*hdl++ != '[')
732	+	return(0);
733	+	/* case-independent keyword match */
734	+	while (toupper(*hdl) == *kwd++)
735	+	if (!*hdl++)
736	+	return(0);
737	+	/* If we have come to the end of the keyword, and the keyword
738	+	* at the beginning of the matched line is terminated with
739	+	* ']', return 1 */
740	+	return(!kwd[-1] & (*hdl == ']'));
741	+	}
742
743	<	putheader(out)                          /* print header */
744	<	FILE    *out;
743	>	/* keyargs - return the argument of a keyword, without leading spaces
744	>	*
745	>	* keyargs is passed a pointer to a buffer; it returns a pointer to
746	>	* where the argument starts in the buffer
747	>	*
748	>	*/
749	>	char *
750	>	keyargs(
751	>	char    *hdl /* header line */
752	>	)
753		{
754	<	register int    i;
755	<
754	>	while (*hdl && *hdl++ != ']')
755	>	;
756	>	while (isspace(*hdl))
757	>	hdl++;
758	>	return(hdl);
759	>	}
760	>
761	>
762	>	/* putheader - output the header of the .rad file
763	>	*
764	>	* Header is:
765	>	*   # <file> <file> <file> (all files from input line)
766	>	*   # Dimensions in [feet,meters,etc.]
767	>	*
768	>	* ??? Is listing all the input file names correct behavior?
769	>	*
770	>	*/
771	>	void
772	>
773	>	putheader(
774	>	FILE    *out
775	>	)
776	>	{
777	>	int     i;
778	>
779		putc('#', out);
780		for (i = 0; i < gargc; i++) {
781		putc(' ', out);
#	Line 371 | Line 786 | FILE   *out;
786		putc('\n', out);
787		}
788
789	<
790	<	ies2rad(inpname, outname)               /* convert IES file */
791	<	char    *inpname, *outname;
789	>	/* ies2rad - convert an IES LM-63 file to a Radiance light source desc.
790	>	*
791	>	* Return -1 in case of failure, 0 in case of success.
792	>	*
793	>	* The file version recognition is confused and will treat 1995 and
794	>	* 2002 version files as 1986 version files.
795	>	*
796	>	*/
797	>	int
798	>	ies2rad(                /* convert IES file */
799	>	char    *inpname,
800	>	char    *outname
801	>	)
802		{
803	<	char    buf[MAXLINE], tltid[MAXWORD];
803	>	SRCINFO srcinfo;
804	>	char    buf[MAXLINE], tltid[RMAXWORD];
805	>	char    geomfile[128];
806		FILE    *inpfp, *outfp;
807	+	int     lineno = 0;
808
809	+	/* Open input and output files */
810	+	geomfile[0] = '\0';
811	+	srcinfo.isillum = 0;
812		if (inpname == NULL) {
813		inpname = "<stdin>";
814		inpfp = stdin;
#	Line 385 | Line 816 | char   *inpname, *outname;
816		perror(inpname);
817		return(-1);
818		}
819	<	if ((outfp = fopen(fullname(buf,outname,T_RAD), "w")) == NULL) {
819	>	if (out2stdout)
820	>	outfp = stdout;
821	>	else if ((outfp = fopen(fullnam(buf,outname,T_RAD), "w")) == NULL) {
822		perror(buf);
823		fclose(inpfp);
824		return(-1);
825		}
826	+
827	+	/* Output the output file header */
828		putheader(outfp);
829	+
830	+	/* If the lamp type wasn't given on the command line, mark
831	+	* the lamp color as missing */
832		if (lamptype == NULL)
833		lampcolor = NULL;
834	+
835	+	/* Read the input file header, copying lines to the .rad file
836	+	* and looking for a lamp type. Stop at EOF or a line
837	+	* beginning with "TILT=". */
838		while (fgets(buf,sizeof(buf),inpfp) != NULL
839		&& strncmp(buf,TLTSTR,TLTSTRLEN)) {
840	<	blanktrunc(buf);
841	<	if (!buf[0])
840	>	blanktrunc(buf); /* Trim trailing spaces, CR, LF. */
841	>	if (!buf[0])     /* Skip blank lines */
842		continue;
843	+	/* increment the header line count, and check for the
844	+	* "TILT=" line that terminates the header */
845	+	if (!lineno++) {        /* first line may be magic */
846	+	if (!strncmp(buf, MAGICID2, LMAGICID2))
847	+	filerev = atoi(buf+LMAGICID2) - 1900;
848	+	else if (!strncmp(buf, MAGICID, LMAGICID))
849	+	filerev = atoi(buf+LMAGICID);
850	+	if (filerev < FIRSTREV)
851	+	filerev = FIRSTREV;
852	+	else if (filerev > LASTREV)
853	+	filerev = LASTREV;
854	+	}
855	+	/* Output the header line as a comment in the .rad file. */
856		fputs("#<", outfp);
857		fputs(buf, outfp);
858		putc('\n', outfp);
859	<	if (lampcolor == NULL)
860	<	lampcolor = matchlamp(buf);
859	>
860	>	/* If the header line is a keyword line (file version
861	>	* later than 1986 and begins with '['), check a lamp
862	>	* in the "[LAMP]" and "[LAMPCAT]" keyword lines;
863	>	* otherwise check all lines.  */
864	>	if (lampcolor == NULL && checklamp(buf))
865	>	lampcolor = matchlamp(*sskip2(buf,0) == '[' ?
866	>	keyargs(buf) : buf );
867	>	/* Look for a materials and geometry file in the keywords. */
868	>	if (keymatch(K_LMG, buf)) {
869	>	strcpy(geomfile, inpname);
870	>	strcpy(filename(geomfile), keyargs(buf));
871	>	srcinfo.isillum = 1;
872	>	}
873		}
874	+
875	+	/* Done reading header information. If a lamp color still
876	+	* hasn't been found, print a warning and use the default
877	+	* color; if a lamp type hasn't been found, but a color has
878	+	* been specified, used the specified color. */
879		if (lampcolor == NULL) {
880		fprintf(stderr, "%s: warning - no lamp type\n", inpname);
881	+	fputs("# Unknown lamp type (used default)\n", outfp);
882		lampcolor = defcolor;
883	<	}
883	>	} else if (lamptype == NULL)
884	>	fprintf(outfp,"# CIE(x,y) = (%f,%f)\n# Depreciation = %.1f%%\n",
885	>	lampcolor[3], lampcolor[4], 100.*lampcolor[5]);
886	>
887	>	/* If the file ended before a "TILT=" line, that's an error. */
888		if (feof(inpfp)) {
889		fprintf(stderr, "%s: not in IES format\n", inpname);
890		goto readerr;
891		}
892	<	atos(tltid, MAXWORD, buf+TLTSTRLEN);
892	>
893	>	/* Process the tilt section of the file. */
894	>	/* Get the tilt file name, or the keyword "INCLUDE". */
895	>	atos(tltid, RMAXWORD, buf+TLTSTRLEN);
896		if (inpfp == stdin)
897		buf[0] = '\0';
898		else
899		filetrunc(strcpy(buf, inpname));
900	+	/* Process the tilt data. */
901		if (dotilt(inpfp, outfp, buf, tltid, outname, tltid) != 0) {
902		fprintf(stderr, "%s: bad tilt data\n", inpname);
903		goto readerr;
904		}
905	<	if (dosource(inpfp, outfp, tltid, outname) != 0) {
905	>
906	>	/* Process the luminaire data. */
907	>	if (dosource(&srcinfo, inpfp, outfp, tltid, outname) != 0) {
908		fprintf(stderr, "%s: bad luminaire data\n", inpname);
909		goto readerr;
910		}
911	<	fclose(outfp);
911	>
912	>	/* Close the input file */
913		fclose(inpfp);
914	+
915	+	/* Process an MGF file, if present. cvgeometry() closes outfp. */
916	+	if (cvgeometry(geomfile, &srcinfo, outname, outfp) != 0) {
917	+	fprintf(stderr, "%s: bad geometry file\n", geomfile);
918	+	return(-1);
919	+	}
920		return(0);
921	+
922		readerr:
923	<	fclose(outfp);
923	>	/* If there is an error reading the file, close the input and
924	>	* .rad output files, and delete the .rad file, returning -1. */
925		fclose(inpfp);
926	<	unlink(fullname(buf,outname,T_RAD));
926	>	fclose(outfp);
927	>	unlink(fullnam(buf,outname,T_RAD));
928		return(-1);
929		}
930
931	<
932	<	dotilt(in, out, dir, tltspec, dfltname, tltid)  /* convert tilt data */
933	<	FILE    *in, *out;
934	<	char    *dir, *tltspec, *dfltname, *tltid;
931	>	/* dotilt -- process tilt data
932	>	*
933	>	* Generate a brightdata primitive which describes the effect of
934	>	* luminaire tilt on luminaire output and return its identifier in tltid.
935	>	*
936	>	* Tilt data (if present) is given as a number 1, 2, or 3, which
937	>	* specifies the orientation of the lamp within the luminaire, a
938	>	* number, n, of (angle, multiplier) pairs, followed by n angles and n
939	>	* multipliers.
940	>	*
941	>	* returns 0 for success, -1 for error
942	>	*/
943	>	int
944	>	dotilt(
945	>	FILE    *in,
946	>	FILE    *out,
947	>	char    *dir,
948	>	char    *tltspec,
949	>	char    *dfltname,
950	>	char    *tltid
951	>	)
952		{
953		int     nangles, tlt_type;
954	<	double  minmax[2];
955	<	char    buf[MAXPATH], tltname[MAXWORD];
954	>	double  minmax[1][2];
955	>	char    buf[PATH_MAX], tltname[RMAXWORD];
956		FILE    *datin, *datout;
957
958	+	/* Decide where the tilt data is; if the luminaire description
959	+	* doesn't have a tilt section, set the identifier to "void". */
960		if (!strcmp(tltspec, TLTNONE)) {
961	+	/* If the line is "TILT=NONE", set the input file
962	+	* pointer to NULL and the identifier to "void". */
963		datin = NULL;
964		strcpy(tltid, "void");
965		} else if (!strcmp(tltspec, TLTINCL)) {
966	+	/* If the line is "TILT=INCLUDE" use the main IES
967	+	* file as the source of tilt data. */
968		datin = in;
969		strcpy(tltname, dfltname);
970		} else {
971	+	/* If the line is "TILE=<filename>", use that file
972	+	* name as the source of tilt data. */
973		if (ISDIRSEP(tltspec[0]))
974		strcpy(buf, tltspec);
975		else
#	Line 462 | Line 980 | char   *dir, *tltspec, *dfltname, *tltid;
980		}
981		tailtrunc(strcpy(tltname,filename(tltspec)));
982		}
983	+	/* If tilt data is present, read, process, and output it. */
984		if (datin != NULL) {
985	<	if ((datout = fopen(fullname(buf,tltname,T_TLT),"w")) == NULL) {
985	>	/* Try to open the output file */
986	>	if ((datout = fopen(fullnam(buf,tltname,T_TLT),"w")) == NULL) {
987		perror(buf);
988		if (datin != in)
989		fclose(datin);
990		return(-1);
991		}
992	+	/* Try to copy the tilt data to the tilt data file */
993		if (!scnint(datin,&tlt_type) || !scnint(datin,&nangles)
994		|| cvdata(datin,datout,1,&nangles,1.,minmax) != 0) {
995		fprintf(stderr, "%s: data format error\n", tltspec);
996		fclose(datout);
997		if (datin != in)
998		fclose(datin);
999	<	unlink(fullname(buf,tltname,T_TLT));
999	>	unlink(fullnam(buf,tltname,T_TLT));
1000		return(-1);
1001		}
1002		fclose(datout);
1003		if (datin != in)
1004		fclose(datin);
1005	+
1006	+	/* Generate the identifier of the brightdata; the filename
1007	+	* with "_tilt" appended. */
1008		strcat(strcpy(tltid, filename(tltname)), "_tilt");
1009	+	/* Write out the brightdata primitive */
1010		fprintf(out, "\nvoid brightdata %s\n", tltid);
1011		libname(buf,tltname,T_TLT);
1012	+	/* Generate the tilt description */
1013		switch (tlt_type) {
1014	<	case TLT_VERT:                  /* vertical */
1014	>	case TLT_VERT:
1015	>	/* The lamp is mounted vertically; either
1016	>	* base up or base down. */
1017		fprintf(out, "4 noop %s tilt.cal %s\n", buf,
1018	<	minmax[1]>90.+FTINY ? "tilt_ang" : "tilt_ang2");
1018	>	minmax[0][1]>90.+FTINY ? "tilt_ang" : "tilt_ang2");
1019		break;
1020	<	case TLT_H0:                    /* horiz. in 0 deg. plane */
1020	>	case TLT_H0:
1021	>	/* The lamp is mounted horizontally and
1022	>	* rotates but does not tilt when the
1023	>	* luminaire is tilted. */
1024		fprintf(out, "6 noop %s tilt.cal %s -rz 90\n", buf,
1025	<	minmax[1]>90.+FTINY ? "tilt_xang" : "tilt_xang2");
1025	>	minmax[0][1]>90.+FTINY ? "tilt_xang" : "tilt_xang2");
1026		break;
1027		case TLT_H90:
1028	+	/* The lamp is mounted horizontally, and
1029	+	* tilts when the luminaire is tilted. */
1030		fprintf(out, "4 noop %s tilt.cal %s\n", buf,
1031	<	minmax[1]>90.+FTINY ? "tilt_xang" : "tilt_xang2");
1031	>	minmax[0][1]>90.+FTINY ? "tilt_xang" : "tilt_xang2");
1032		break;
1033		default:
1034	+	/* otherwise, this is a bad IES file */
1035		fprintf(stderr,
1036		"%s: illegal lamp to luminaire geometry (%d)\n",
1037		tltspec, tlt_type);
1038		return(-1);
1039		}
1040	+	/* And finally output the numbers of integer and real
1041	+	* arguments, of which there are none. */
1042		fprintf(out, "0\n0\n");
1043		}
1044		return(0);
1045		}
1046
1047	<
1048	<	dosource(in, out, mod, name)            /* create source and distribution */
1049	<	FILE    *in, *out;
1050	<	char    *mod, *name;
1047	>	/* dosource -- create the source and distribution primitives */
1048	>	int
1049	>	dosource(
1050	>	SRCINFO *sinf,
1051	>	FILE    *in,
1052	>	FILE    *out,
1053	>	char    *mod,
1054	>	char    *name
1055	>	)
1056		{
1057	<	SHAPE   srcshape;
517	<	char    buf[MAXPATH], id[MAXWORD];
1057	>	char    buf[PATH_MAX], id[RMAXWORD];
1058		FILE    *datout;
1059		double  mult, bfactor, pfactor, width, length, height, wattage;
1060		double  bounds[2][2];
1061		int     nangles[2], pmtype, unitype;
1062		double  d1;
1063	+	int     doupper, dolower, dosides;
1064
1065	+	/* Read in the luminaire description header */
1066		if (!isint(getword(in)) || !isflt(getword(in)) || !scnflt(in,&mult)
1067		|| !scnint(in,&nangles[0]) || !scnint(in,&nangles[1])
1068		|| !scnint(in,&pmtype) || !scnint(in,&unitype)
#	Line 530 | Line 1072 | char   *mod, *name;
1072		fprintf(stderr, "dosource: bad lamp specification\n");
1073		return(-1);
1074		}
1075	+	/* Type A photometry is not supported */
1076	+	if (pmtype != PM_C && pmtype != PM_B) {
1077	+	fprintf(stderr, "dosource: unsupported photometric type (%d)\n",
1078	+	pmtype);
1079	+	return(-1);
1080	+	}
1081	+
1082	+	/* Multiplier = the multiplier from the -m option, times the
1083	+	* multiplier from the IES file, times the ballast factor,
1084	+	* times the "ballast lamp photometric factor," which was part
1085	+	* of the 1986 and 1991 standards. In the 1995 standard, it is
1086	+	* always supposed to be 1. */
1087	+	sinf->mult = multiplier*mult*bfactor*pfactor;
1088	+
1089	+	/* If the count of angles is wrong, raise an error and quit. */
1090		if (nangles[0] < 2 || nangles[1] < 1) {
1091		fprintf(stderr, "dosource: too few measured angles\n");
1092		return(-1);
1093		}
1094	+
1095	+	/* For internal computation, convert units to meters. */
1096		if (unitype == U_FEET) {
1097		width *= F_M;
1098		length *= F_M;
1099		height *= F_M;
1100		}
1101	<	if (makeshape(&srcshape, width, length, height) != 0) {
1101	>
1102	>	/* Make decisions about the shape of the light source
1103	>	* geometry, and store them in sinf. */
1104	>	if (makeshape(sinf, width, length, height) != 0) {
1105		fprintf(stderr, "dosource: illegal source dimensions");
1106		return(-1);
1107		}
1108	<	if ((datout = fopen(fullname(buf,name,T_DST), "w")) == NULL) {
1108	>
1109	>	/* Copy the candela values into a Radiance data file. */
1110	>	if ((datout = fopen(fullnam(buf,name,T_DST), "w")) == NULL) {
1111		perror(buf);
1112		return(-1);
1113		}
1114		if (cvdata(in, datout, 2, nangles, 1./WHTEFFICACY, bounds) != 0) {
1115		fprintf(stderr, "dosource: bad distribution data\n");
1116		fclose(datout);
1117	<	unlink(fullname(buf,name,T_DST));
1117	>	unlink(fullnam(buf,name,T_DST));
1118		return(-1);
1119		}
1120		fclose(datout);
1121	+
1122	+	/* Output explanatory comment */
1123		fprintf(out, "# %g watt luminaire, lamp*ballast factor = %g\n",
1124		wattage, bfactor*pfactor);
1125	+	/* Output distribution "brightdata" primitive. Start handling
1126	+	the various cases of symmetry of the distribution. */
1127		strcat(strcpy(id, filename(name)), "_dist");
1128		fprintf(out, "\n%s brightdata %s\n", mod, id);
1129		if (nangles[1] < 2)
#	Line 563 | Line 1131 | char   *mod, *name;
1131		else if (pmtype == PM_B)
1132		fprintf(out, "5 ");
1133		else if (FEQ(bounds[1][0],90.) && FEQ(bounds[1][1],270.))
1134	<	fprintf(out, "8 ");
1134	>	fprintf(out, "7 ");
1135		else
1136	<	fprintf(out, "6 ");
1136	>	fprintf(out, "5 ");
1137	>
1138	>	/* If the generated source geometry will be a box, a flat
1139	>	* rectangle, or a disk figure out if it needs a top, a
1140	>	* bottom, and/or sides. */
1141	>	dolower = (bounds[0][0] < 90.-FTINY); /* Bottom */
1142	>	doupper = (bounds[0][1] > 90.+FTINY); /* Top */
1143	>	dosides = (doupper & dolower && sinf->h > MINDIM); /* Sides */
1144	>
1145	>	/* Select the appropriate function and parameters from source.cal */
1146		fprintf(out, "%s %s source.cal ",
1147	<	srcshape.type==SPHERE ? "corr" : "flatcorr",
1147	>	sinf->type==SPHERE ? "corr" :
1148	>	!dosides ? "flatcorr" :
1149	>	sinf->type==DISK ? "cylcorr" : "boxcorr",
1150		libname(buf,name,T_DST));
1151		if (pmtype == PM_B) {
1152		if (FEQ(bounds[1][0],0.))
#	Line 575 | Line 1154 | char   *mod, *name;
1154		else
1155		fprintf(out, "srcB_horiz ");
1156		fprintf(out, "srcB_vert ");
1157	<	} else {
1157	>	} else /* pmtype == PM_C */ {
1158		if (nangles[1] >= 2) {
1159		d1 = bounds[1][1] - bounds[1][0];
1160		if (d1 <= 90.+FTINY)
1161		fprintf(out, "src_phi4 ");
1162	<	else if (d1 <= 180.+FTINY)
1163	<	fprintf(out, "src_phi2 ");
1164	<	else
1162	>	else if (d1 <= 180.+FTINY) {
1163	>	if (FEQ(bounds[1][0],90.))
1164	>	fprintf(out, "src_phi2+90 ");
1165	>	else
1166	>	fprintf(out, "src_phi2 ");
1167	>	} else
1168		fprintf(out, "src_phi ");
1169	<	fprintf(out, "src_theta -my ");
1169	>	fprintf(out, "src_theta ");
1170		if (FEQ(bounds[1][0],90.) && FEQ(bounds[1][1],270.))
1171		fprintf(out, "-rz -90 ");
1172		} else
1173		fprintf(out, "src_theta ");
1174		}
1175	<	fprintf(out, "\n0\n1 %g\n", multiplier*mult*bfactor*pfactor);
1176	<	if (putsource(&srcshape, out, id, filename(name),
1177	<	bounds[0][0]<90., bounds[0][1]>90.) != 0)
1175	>	/* finish the brightdata primitive with appropriate data */
1176	>	if (!dosides || sinf->type == SPHERE)
1177	>	fprintf(out, "\n0\n1 %g\n", sinf->mult/sinf->area);
1178	>	else if (sinf->type == DISK)
1179	>	fprintf(out, "\n0\n3 %g %g %g\n", sinf->mult,
1180	>	sinf->w, sinf->h);
1181	>	else
1182	>	fprintf(out, "\n0\n4 %g %g %g %g\n", sinf->mult,
1183	>	sinf->l, sinf->w, sinf->h);
1184	>	/* Brightdata primitive written out. */
1185	>
1186	>	/* Finally, output the descriptions of the actual radiant
1187	>	* surfaces. */
1188	>	if (putsource(sinf, out, id, filename(name),
1189	>	dolower, doupper, dosides) != 0)
1190		return(-1);
1191		return(0);
1192		}
1193
1194	<
1195	<	putsource(shp, fp, mod, name, dolower, doupper)         /* put out source */
1196	<	SHAPE   *shp;
1197	<	FILE    *fp;
1198	<	char    *mod, *name;
1199	<	int     dolower, doupper;
1194	>	/* putsource - output the actual light emitting geometry
1195	>	*
1196	>	* Three kinds of geometry are produced: rectangles and boxes, disks
1197	>	* ("ring" primitive, but the radius of the hole is always zero) and
1198	>	* cylinders, and spheres.
1199	>	*/
1200	>	int
1201	>	putsource(
1202	>	SRCINFO *shp,
1203	>	FILE    *fp,
1204	>	char    *mod,
1205	>	char    *name,
1206	>	int     dolower,
1207	>	int     doupper,
1208	>	int     dosides
1209	>	)
1210		{
1211	<	char    buf[MAXWORD];
1212	<
1213	<	fprintf(fp, "\n%s %s %s_light\n", mod,
1214	<	illumrad>=MINDIM/2. ? "illum" : "light",
1215	<	name);
1211	>	char    lname[RMAXWORD];
1212	>
1213	>	/* First, describe the light. If a materials and geometry
1214	>	* file is given, generate an illum instead. */
1215	>	strcat(strcpy(lname, name), "_light");
1216	>	fprintf(fp, "\n%s %s %s\n", mod,
1217	>	shp->isillum ? "illum" : "light", lname);
1218		fprintf(fp, "0\n0\n3 %g %g %g\n",
1219	<	lampcolor[0]/shp->area,
614	<	lampcolor[1]/shp->area,
615	<	lampcolor[2]/shp->area);
616	<	if (doupper && dolower && shp->type != SPHERE && shp->h > MINDIM) {
617	<	fprintf(fp, "\n%s glow %s_glow\n", mod, name);
618	<	fprintf(fp, "0\n0\n4 %g %g %g -1\n",
619	<	lampcolor[0]/shp->area,
620	<	lampcolor[1]/shp->area,
621	<	lampcolor[2]/shp->area);
622	<	}
1219	>	lampcolor[0], lampcolor[1], lampcolor[2]);
1220		switch (shp->type) {
1221		case RECT:
1222	<	strcat(strcpy(buf, name), "_light");
1222	>	/* Output at least one rectangle. If light is radiated
1223	>	* from the sides of the luminaire, output rectangular
1224	>	* sides as well. */
1225		if (dolower)
1226	<	putrectsrc(shp, fp, buf, name, 0);
1226	>	putrectsrc(shp, fp, lname, name, 0);
1227		if (doupper)
1228	<	putrectsrc(shp, fp, buf, name, 1);
1229	<	if (doupper && dolower && shp->h > MINDIM) {
1230	<	strcat(strcpy(buf, name), "_glow");
632	<	putsides(shp, fp, buf, name);
633	<	}
1228	>	putrectsrc(shp, fp, lname, name, 1);
1229	>	if (dosides)
1230	>	putsides(shp, fp, lname, name);
1231		break;
1232		case DISK:
1233	<	strcat(strcpy(buf, name), "_light");
1233	>	/* Output at least one disk. If light is radiated from
1234	>	* the sides of luminaire, output a cylinder as well. */
1235		if (dolower)
1236	<	putdisksrc(shp, fp, buf, name, 0);
1236	>	putdisksrc(shp, fp, lname, name, 0);
1237		if (doupper)
1238	<	putdisksrc(shp, fp, buf, name, 1);
1239	<	if (doupper && dolower && shp->h > MINDIM) {
1240	<	strcat(strcpy(buf, name), "_glow");
643	<	putcyl(shp, fp, buf, name);
644	<	}
1238	>	putdisksrc(shp, fp, lname, name, 1);
1239	>	if (dosides)
1240	>	putcyl(shp, fp, lname, name);
1241		break;
1242		case SPHERE:
1243	<	strcat(strcpy(buf, name), "_light");
1244	<	putspheresrc(shp, fp, buf, name);
1243	>	/* Output a sphere. */
1244	>	putspheresrc(shp, fp, lname, name);
1245		break;
1246		}
1247		return(0);
1248		}
1249
1250	<
1251	<	makeshape(shp, width, length, height)           /* make source shape */
1252	<	register SHAPE  *shp;
1253	<	double  width, length, height;
1250	>	/* makeshape -- decide what shape will be used
1251	>	*
1252	>	* makeshape decides what Radiance geometry will be used to represent
1253	>	* the light source and stores information about it in shp.
1254	>	*/
1255	>	int
1256	>	makeshape(
1257	>	SRCINFO *shp,
1258	>	double  width,
1259	>	double  length,
1260	>	double  height
1261	>	)
1262		{
1263	<	if (illumrad >= MINDIM/2.) {
1263	>	/* Categorize the shape */
1264	>	if (illumrad/meters2out >= MINDIM/2.) {
1265	>	/* If the -i command line option is used, and the
1266	>	* object is not a point source, output an "illum"
1267	>	* sphere */
1268	>	shp->isillum = 1;
1269		shp->type = SPHERE;
1270	<	shp->w = shp->l = shp->h = 2.*illumrad;
1270	>	shp->w = shp->l = shp->h = 2.*illumrad / meters2out;
1271		} else if (width < MINDIM) {
1272	+	/* The width is either zero or negative. */
1273		width = -width;
1274		if (width < MINDIM) {
1275	+	/* The width is zero. Use a tiny sphere to
1276	+	* represent a point source. */
1277		shp->type = SPHERE;
1278		shp->w = shp->l = shp->h = MINDIM;
1279		} else if (height < .5*width) {
1280	+	/* The width is negative and the height is
1281	+	* modest; output either a disk or a thin
1282	+	* vertical cylinder. */
1283		shp->type = DISK;
1284		shp->w = shp->l = width;
1285		if (height >= MINDIM)
#	Line 672 | Line 1287 | double width, length, height;
1287		else
1288		shp->h = .5*MINDIM;
1289		} else {
1290	+	/* The width is negative and the object is
1291	+	* tall; output a sphere. */
1292		shp->type = SPHERE;
1293		shp->w = shp->l = shp->h = width;
1294		}
1295		} else {
1296	+	/* The width is positive. Output a box, possibly very
1297	+	* thin. */
1298		shp->type = RECT;
1299		shp->w = width;
1300		if (length >= MINDIM)
#	Line 687 | Line 1306 | double width, length, height;
1306		else
1307		shp->h = .5*MINDIM;
1308		}
1309	+
1310	+	/* Done choosing the shape; calculate its area in the x-y plane. */
1311		switch (shp->type) {
1312		case RECT:
1313		shp->area = shp->w * shp->l;
#	Line 699 | Line 1320 | double width, length, height;
1320		return(0);
1321		}
1322
1323	+	/* Rectangular or box-shaped light source.
1324	+	*
1325	+	* putrectsrc, putsides, putrect, and putpoint are used to output the
1326	+	* Radiance description of a box.  The box is centered on the origin
1327	+	* and has the dimensions given in the IES file.  The coordinates
1328	+	* range from [-1/2*length, -1/2*width, -1/2*height] to [1/2*length,
1329	+	* 1/2*width, 1/2*height].
1330	+	*
1331	+	* The location of the point is encoded in the low-order three bits of
1332	+	* an integer. If the integer is p, then: bit 0 is (p & 1),
1333	+	* representing length (x), bit 1 is (p & 2) representing width (y),
1334	+	* and bit 2 is (p & 4), representing height (z).
1335	+	*
1336	+	* Looking down from above (towards -z), the vertices of the box or
1337	+	* rectangle are numbered so:
1338	+	*
1339	+	*     2,6                                        3,7
1340	+	*        +--------------------------------------+
1341	+	*        |                                      |
1342	+	*        |                                      |
1343	+	*        |                                      |
1344	+	*        |                                      |
1345	+	*        +--------------------------------------+
1346	+	*     0,4                                        1,5
1347	+	*
1348	+	* The higher number of each pair is above the x-y plane (positive z),
1349	+	* the lower number is below the x-y plane (negative z.)
1350	+	*
1351	+	*/
1352
1353	<	putrectsrc(shp, fp, mod, name, up)              /* rectangular source */
1354	<	SHAPE   *shp;
1355	<	FILE    *fp;
1356	<	char    *mod, *name;
1357	<	int     up;
1353	>	/* putrecsrc - output a rectangle parallel to the x-y plane
1354	>	*
1355	>	* Putrecsrc calls out the vertices of a rectangle parallel to the x-y
1356	>	* plane.  The order of the vertices is different for the upper and
1357	>	* lower rectangles of a box, since a right-hand rule based on the
1358	>	* order of the vertices is used to determine the surface normal of
1359	>	* the rectangle, and the surface normal determines the direction the
1360	>	* light radiated by the rectangle.
1361	>	*
1362	>	*/
1363	>	void
1364	>	putrectsrc(
1365	>	SRCINFO *shp,
1366	>	FILE    *fp,
1367	>	char    *mod,
1368	>	char    *name,
1369	>	int     up
1370	>	)
1371		{
1372		if (up)
1373		putrect(shp, fp, mod, name, ".u", 4, 5, 7, 6);
#	Line 712 | Line 1375 | int    up;
1375		putrect(shp, fp, mod, name, ".d", 0, 2, 3, 1);
1376		}
1377
1378	<
1379	<	putsides(shp, fp, mod, name)                    /* put out sides of box */
1380	<	register SHAPE  *shp;
1381	<	FILE    *fp;
1382	<	char    *mod, *name;
1378	>	/* putsides - put out sides of box */
1379	>	void
1380	>	putsides(
1381	>	SRCINFO *shp,
1382	>	FILE    *fp,
1383	>	char    *mod,
1384	>	char    *name
1385	>	)
1386		{
1387		putrect(shp, fp, mod, name, ".1", 0, 1, 5, 4);
1388		putrect(shp, fp, mod, name, ".2", 1, 3, 7, 5);
1389		putrect(shp, fp, mod, name, ".3", 3, 2, 6, 7);
1390		putrect(shp, fp, mod, name, ".4", 2, 0, 4, 6);
1391		}
726	–
1392
1393	<	putrect(shp, fp, mod, name, suffix, a, b, c, d) /* put out a rectangle */
1394	<	SHAPE   *shp;
1395	<	FILE    *fp;
1396	<	char    *mod, *name, *suffix;
1397	<	int     a, b, c, d;
1393	>	/* putrect - put out a rectangle
1394	>	*
1395	>	* putrect generates the "polygon" primitive which describes a
1396	>	* rectangle.
1397	>	*/
1398	>	void
1399	>	putrect(
1400	>	SRCINFO *shp,
1401	>	FILE    *fp,
1402	>	char    *mod,
1403	>	char    *name,
1404	>	char    *suffix,
1405	>	int     a,
1406	>	int b,
1407	>	int c,
1408	>	int d
1409	>	)
1410		{
1411		fprintf(fp, "\n%s polygon %s%s\n0\n0\n12\n", mod, name, suffix);
1412		putpoint(shp, fp, a);
#	Line 738 | Line 1415 | int    a, b, c, d;
1415		putpoint(shp, fp, d);
1416		}
1417
1418	<
1419	<	putpoint(shp, fp, p)                            /* put out a point */
1420	<	register SHAPE  *shp;
1421	<	FILE    *fp;
1422	<	int     p;
1418	>	/* putpoint -- output a the coordinates of a vertex
1419	>	*
1420	>	* putpoint maps vertex numbers to coordinates and outputs the
1421	>	* coordinates.
1422	>	*/
1423	>	void
1424	>	putpoint(
1425	>	SRCINFO *shp,
1426	>	FILE    *fp,
1427	>	int     p
1428	>	)
1429		{
1430		static double   mult[2] = {-.5, .5};
1431
#	Line 752 | Line 1435 | int    p;
1435		mult[p>>2]*shp->h*meters2out);
1436		}
1437
1438	+	/* End of routines to output a box-shaped light source */
1439
1440	<	putdisksrc(shp, fp, mod, name, up)              /* put out a disk source */
1441	<	register SHAPE  *shp;
1442	<	FILE    *fp;
1443	<	char    *mod, *name;
1444	<	int     up;
1440	>	/* Routines to output a cylindrical or disk shaped light source
1441	>	*
1442	>	* As with other shapes, the light source is centered on the origin.
1443	>	* The "ring" and "cylinder" primitives are used.
1444	>	*
1445	>	*/
1446	>	void
1447	>	putdisksrc(             /* put out a disk source */
1448	>	SRCINFO *shp,
1449	>	FILE    *fp,
1450	>	char    *mod,
1451	>	char    *name,
1452	>	int     up
1453	>	)
1454		{
1455		if (up) {
1456		fprintf(fp, "\n%s ring %s.u\n", mod, name);
#	Line 775 | Line 1468 | int    up;
1468		}
1469
1470
1471	<	putcyl(shp, fp, mod, name)                      /* put out a cylinder */
1472	<	register SHAPE  *shp;
1473	<	FILE    *fp;
1474	<	char    *mod, *name;
1471	>	void
1472	>	putcyl(                 /* put out a cylinder */
1473	>	SRCINFO *shp,
1474	>	FILE    *fp,
1475	>	char    *mod,
1476	>	char    *name
1477	>	)
1478		{
1479		fprintf(fp, "\n%s cylinder %s.c\n", mod, name);
1480		fprintf(fp, "0\n0\n7\n");
#	Line 787 | Line 1483 | char   *mod, *name;
1483		fprintf(fp, "\t%g\n", .5*shp->w*meters2out);
1484		}
1485
1486	+	/* end of of routines to output cylinders and disks */
1487
1488	<	putspheresrc(shp, fp, mod, name)                /* put out a sphere source */
1489	<	SHAPE   *shp;
1490	<	FILE    *fp;
1491	<	char    *mod, *name;
1488	>	void
1489	>	putspheresrc(           /* put out a sphere source */
1490	>	SRCINFO *shp,
1491	>	FILE    *fp,
1492	>	char    *mod,
1493	>	char    *name
1494	>	)
1495		{
1496		fprintf(fp, "\n%s sphere %s.s\n", mod, name);
1497		fprintf(fp, "0\n0\n4 0 0 0 %g\n", .5*shp->w*meters2out);
1498		}
1499
1500	<
1501	<	cvdata(in, out, ndim, npts, mult, lim)          /* convert data */
1502	<	FILE    *in, *out;
1503	<	int     ndim, npts[];
1504	<	double  mult, lim[][2];
1500	>	/* cvdata - convert LM-63 tilt and candela data to Radiance brightdata format
1501	>	*
1502	>	* The files created by this routine are intended for use with the Radiance
1503	>	* "brightdata" material type.
1504	>	*
1505	>	* Two types of data are converted; one-dimensional tilt data, which
1506	>	* is given in polar coordinates, and two-dimensional candela data,
1507	>	* which is given in spherical co-ordinates.
1508	>	*
1509	>	* Return 0 for success, -1 for failure.
1510	>	*
1511	>	*/
1512	>	int
1513	>	cvdata(
1514	>	FILE    *in,            /* Input file */
1515	>	FILE    *out,           /* Output file */
1516	>	int     ndim,           /* Number of dimensions; 1 for
1517	>	* tilt data, 2 for photometric data. */
1518	>	int     npts[],         /* Number of points in each dimension */
1519	>	double  mult,           /* Multiple each value by this
1520	>	* number. For tilt data, always
1521	>	* 1. For candela values, the
1522	>	* efficacy of white Radiance light.  */
1523	>	double  lim[][2]        /* The range of angles in each dimension. */
1524	>	)
1525		{
1526	<	double  *pt[4];
1527	<	register int    i, j;
1526	>	double  *pt[4];         /* Four is the expected maximum of ndim. */
1527	>	int     i, j;
1528		double  val;
1529		int     total;
1530
1531	+	/* Calculate and output the number of data values */
1532		total = 1; j = 0;
1533		for (i = 0; i < ndim; i++)
1534		if (npts[i] > 1) {
#	Line 815 | Line 1536 | double mult, lim[][2];
1536		j++;
1537		}
1538		fprintf(out, "%d\n", j);
1539	<	/* get coordinates */
1539	>
1540	>	/* Read in the angle values, and note the first and last in
1541	>	* each dimension, if there is a place to store them. In the
1542	>	* case of tilt data, there is only one list of angles. In the
1543	>	* case of candela values, vertical angles appear first, and
1544	>	* horizontal angles occur second. */
1545		for (i = 0; i < ndim; i++) {
1546	+	/* Allocate space for the angle values. */
1547		pt[i] = (double *)malloc(npts[i]*sizeof(double));
1548		for (j = 0; j < npts[i]; j++)
1549		if (!scnflt(in, &pt[i][j]))
#	Line 826 | Line 1553 | double mult, lim[][2];
1553		lim[i][1] = pt[i][npts[i]-1];
1554		}
1555		}
1556	<	/* write out in reverse */
1556	>
1557	>	/* Output the angles. If this is candela data, horizontal
1558	>	* angles output first. There are two cases: the first where
1559	>	* the angles are evenly spaced, the second where they are
1560	>	* not.
1561	>	*
1562	>	* When the angles are evenly spaced, three numbers are
1563	>	* output: the first angle, the last angle, and the number of
1564	>	* angles.  When the angles are not evenly spaced, instead
1565	>	* zero, zero, and the count of angles is given, followed by a
1566	>	* list of angles.  In this case, angles are output four to a line.
1567	>	*/
1568		for (i = ndim-1; i >= 0; i--) {
1569		if (npts[i] > 1) {
1570	+	/* Determine if the angles are evenly spaces */
1571		for (j = 1; j < npts[i]-1; j++)
1572		if (!FEQ(pt[i][j]-pt[i][j-1],
1573		pt[i][j+1]-pt[i][j]))
1574		break;
1575	+	/* If they are, output the first angle, the
1576	+	* last angle, and a count */
1577		if (j == npts[i]-1)
1578		fprintf(out, "%g %g %d\n", pt[i][0], pt[i][j],
1579		npts[i]);
1580		else {
1581	+	/* otherwise, output 0, 0, and a
1582	+	* count, followed by the list of
1583	+	* angles, one to a line. */
1584		fprintf(out, "0 0 %d", npts[i]);
1585		for (j = 0; j < npts[i]; j++) {
1586		if (j%4 == 0)
#	Line 846 | Line 1590 | double mult, lim[][2];
1590		putc('\n', out);
1591		}
1592		}
1593	<	free((char *)pt[i]);
1593	>	/* Free the storage containing the angle values. */
1594	>	free((void *)pt[i]);
1595		}
1596	+
1597	+	/* Finally, read in the data values (candela or multiplier values,
1598	+	* depending on the part of the file) and output them four to
1599	+	* a line. */
1600		for (i = 0; i < total; i++) {
1601		if (i%4 == 0)
1602		putc('\n', out);
#	Line 859 | Line 1608 | double mult, lim[][2];
1608		return(0);
1609		}
1610
1611	<
1611	>	/* getword - get an LM-63 delimited word from fp
1612	>	*
1613	>	* Getword gets a word from an IES file delimited by either white
1614	>	* space or a comma surrounded by white space. A pointer to the word
1615	>	* is returned, which will persist only until getword is called again.
1616	>	* At EOF, return NULL instead.
1617	>	*
1618	>	*/
1619		char *
1620	<	getword(fp)                     /* scan a word from fp */
1621	<	register FILE   *fp;
1620	>	getword(                        /* scan a word from fp */
1621	>	FILE    *fp
1622	>	)
1623		{
1624	<	static char     word[MAXWORD];
1625	<	register char   *cp;
1626	<	register int    c;
1624	>	static char     wrd[RMAXWORD];
1625	>	char    *cp;
1626	>	int     c;
1627
1628	+	/* Skip initial spaces */
1629		while (isspace(c=getc(fp)))
1630		;
1631	<	for (cp = word; c != EOF && cp < word+MAXWORD-1;
1631	>	/* Get characters to a delimiter or until wrd is full */
1632	>	for (cp = wrd; c != EOF && cp < wrd+RMAXWORD-1;
1633		*cp++ = c, c = getc(fp))
1634		if (isspace(c) || c == ',') {
1635	+	/* If we find a delimiter */
1636	+	/* Gobble up whitespace */
1637		while (isspace(c))
1638		c = getc(fp);
1639	<	if (c != EOF & c != ',')
1639	>	/* If it's not a comma, put the first
1640	>	* character of the next data item back */
1641	>	if ((c != EOF) & (c != ','))
1642		ungetc(c, fp);
1643	+	/* Close out the strimg */
1644		*cp = '\0';
1645	<	return(word);
1645	>	/* return it */
1646	>	return(wrd);
1647		}
1648	+	/* If we ran out of space or are at the end of the file,
1649	+	* return either the word or NULL, as appropriate. */
1650		*cp = '\0';
1651	<	return(cp > word ? word : NULL);
1651	>	return(cp > wrd ? wrd : NULL);
1652		}
1653
1654	<
1655	<	cvtint(ip, word)                /* convert a word to an integer */
1656	<	int     *ip;
1657	<	char    *word;
1654	>	/* cvtint - convert an IES word to an integer
1655	>	*
1656	>	* A pointer to the word is passed in wrd; ip is expected to point to
1657	>	* an integer.  cvtint() will silently truncate a floating point value
1658	>	* to an integer; "1", "1.0", and "1.5" will all return 1.
1659	>	*
1660	>	* cvtint() returns 0 if it fails, 1 if it succeeds.
1661	>	*/
1662	>	int
1663	>	cvtint(
1664	>	int     *ip,
1665	>	char    *wrd
1666	>	)
1667		{
1668	<	if (word == NULL || !isint(word))
1668	>	if (wrd == NULL || !isint(wrd))
1669		return(0);
1670	<	*ip = atoi(word);
1670	>	*ip = atoi(wrd);
1671		return(1);
1672		}
1673
1674
1675	<	cvtflt(rp, word)                /* convert a word to a double */
1676	<	double  *rp;
1677	<	char    *word;
1675	>	/* cvtflt - convert an IES word to a double precision floating-point number
1676	>	*
1677	>	* A pointer to the word is passed in wrd; rp is expected to point to
1678	>	* a double.
1679	>	*
1680	>	* cvtflt returns 0 if it fails, 1 if it succeeds.
1681	>	*/
1682	>	int
1683	>	cvtflt(
1684	>	double  *rp,
1685	>	char    *wrd
1686	>	)
1687		{
1688	<	if (word == NULL || !isflt(word))
1688	>	if (wrd == NULL || !isflt(wrd))
1689		return(0);
1690	<	*rp = atof(word);
1690	>	*rp = atof(wrd);
1691		return(1);
1692		}
1693	+
1694	+	/* cvgeometry - process materials and geometry format luminaire data
1695	+	*
1696	+	* The materials and geometry format (MGF) for describing luminaires
1697	+	* was a part of Radiance that was first adopted and then retracted by
1698	+	* the IES as part of LM-63.  It provides a way of describing
1699	+	* luminaire geometry similar to the Radiance scene description
1700	+	* format.
1701	+	*
1702	+	* cvgeometry() generates an mgf2rad command and then, if "-g" is given
1703	+	* on the command line, an oconv command, both of which are then
1704	+	* executed with the system() function.
1705	+	*
1706	+	* The generated commands are:
1707	+	*   mgf2rad -e <multiplier> -g <size> <mgf_filename> \
1708	+	*     | xform -s <scale_factor> \
1709	+	*     >> <luminare_scene_description_file
1710	+	* or:
1711	+	*   mgf2rad -e <multiplier> -g <size> <mgf_filename> \
1712	+	*     oconv - > <instance_filename>
1713	+	*/
1714	+	int
1715	+	cvgeometry(
1716	+	char    *inpname,
1717	+	SRCINFO *sinf,
1718	+	char    *outname,
1719	+	FILE    *outfp                  /* close output file upon return */
1720	+	)
1721	+	{
1722	+	char    buf[256];
1723	+	char    *cp;
1724	+
1725	+	if (inpname == NULL || !inpname[0]) {   /* no geometry file */
1726	+	fclose(outfp);
1727	+	return(0);
1728	+	}
1729	+	putc('\n', outfp);
1730	+	strcpy(buf, "mgf2rad ");                /* build mgf2rad command */
1731	+	cp = buf+8;
1732	+	if (!FEQ(sinf->mult, 1.0)) {
1733	+	/* if there's an output multiplier, include in the
1734	+	* mgf2rad command */
1735	+	sprintf(cp, "-e %f ", sinf->mult);
1736	+	cp += strlen(cp);
1737	+	}
1738	+	/* Include the glow distance for the geometry */
1739	+	sprintf(cp, "-g %f %s ",
1740	+	sqrt(sinf->w*sinf->w + sinf->h*sinf->h + sinf->l*sinf->l),
1741	+	inpname);
1742	+	cp += strlen(cp);
1743	+	if (instantiate) {              /* instantiate octree */
1744	+	/* If "-g" is given on the command line, include an
1745	+	* "oconv" command in the pipe. */
1746	+	strcpy(cp, "| oconv - > ");
1747	+	cp += 12;
1748	+	fullnam(cp,outname,T_OCT);
1749	+	/* Only update if the input file is newer than the
1750	+	* output file */
1751	+	if (fdate(inpname) > fdate(outname) &&
1752	+	system(buf)) {          /* create octree */
1753	+	fclose(outfp);
1754	+	return(-1);
1755	+	}
1756	+	/* Reference the instance file in the scene description */
1757	+	fprintf(outfp, "void instance %s_inst\n", outname);
1758	+	/* If the geometry isn't in meters, scale it appropriately. */
1759	+	if (!FEQ(meters2out, 1.0))
1760	+	fprintf(outfp, "3 %s -s %f\n",
1761	+	libname(buf,outname,T_OCT),
1762	+	meters2out);
1763	+	else
1764	+	fprintf(outfp, "1 %s\n", libname(buf,outname,T_OCT));
1765	+	/* Close off the "instance" primitive. */
1766	+	fprintf(outfp, "0\n0\n");
1767	+	/* And the Radiance scene description. */
1768	+	fclose(outfp);
1769	+	} else {                        /* else append to luminaire file */
1770	+	if (!FEQ(meters2out, 1.0)) {    /* apply scalefactor */
1771	+	sprintf(cp, "| xform -s %f ", meters2out);
1772	+	cp += strlen(cp);
1773	+	}
1774	+	if (!out2stdout) {
1775	+	fclose(outfp);
1776	+	strcpy(cp, ">> ");      /* append works for DOS? */
1777	+	cp += 3;
1778	+	fullnam(cp,outname,T_RAD);
1779	+	}
1780	+	if (system(buf))
1781	+	return(-1);
1782	+	}
1783	+	return(0);
1784	+	}
1785	+
1786	+	/* Set up emacs indentation */
1787	+	/* Local Variables: */
1788	+	/*   c-file-style: "bsd" */
1789	+	/* End: */
1790	+
1791	+	/* For vim, use ":set tabstop=8 shiftwidth=8" */

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