1
2
3
4
5
6
7
8
9
10
11
12
13
14
15
16
17
18
19
20
21
22
23
24
25
26
27
28
29
30
31
32
33
34
35
36
37
38
39
40
41
42
43
44
45
46
47
48
49
50
51
52
53
54
55
56
57
58
59
60
61
62
63
64
65
66
67
68
69
70
71
72
73
74
75
76
77
78
79
80
81
82
83
84
85
86
87
88
89
90
91
92
93
94
95
96
97
98
99
100
101
102
103
104
105
106
107
108
109
110
111
112
113
114
115
116
117
118
119
120
121
122
123
124
125
126
127
128
129
130
131
132
133
134
135
136
137
138
139
140
141
142
143
144
145
146
147
148
149
150
151
152
153
154
155
156
157
158
159
160
161
162
163
164
165
166
167
168
169
170
171
172
173
174
175
176
177
178
179
180
181
182
183
184
185
186
187
188
189
190
191
192
193
194
195
196
197
198
199
200
201
202
203
204
205
206
207
208
209
210
211
212
213
214
215
216
217
218
219
220
221
222
223
224
225
226
227
228
229
230
231
232
233
234
235
236
237
238
239
240
241
242
243
244
245
246
247
248
249
250
251
252
253
254
255
256
257
258
259
260
261
262
263
264
265
266
267
268
269
270
271
272
273
274
275
276
277
278
279
280
281
282
283
284
285
286
287
288
289
290
291
292
293
294
295
296
297
298
299
300
301
302
303
304
305
306
307
308
309
310
311
312
313
314
315
316
317
318
319
320
321
322
323
324
325
326
327
328
329
330
331
332
333
334
335
336
337
338
339
340
341
342
343
344
345
346
347
348
349
350
351
352
353
354
355
356
357
358
359
360
361
362
363
364
365
366
367
368
369
370
371
372
373
374
375
376
377
378
379
380
381
382
383
384
385
386
387
388
389
390
391
392
393
394
395
396
397
398
399
400
401
402
403
404
405
406
407
408
409
410
411
412
413
414
415
416
417
418
419
420
421
422
423
424
425
426
427
428
429
430
431
432
433
434
435
436
437
438
439
440
441
442
443
444
445
446
447
448
449
450
451
452
453
454
455
456
457
458
459
460
461
462
463
464
465
466
467
468
469
470
471
472
473
474
475
476
477
478
479
480
481
482
483
484
485
486
487
488
489
490
491
492
493
494
495
496
497
498
499
500
501
502
503
504
505
506
507
508
509
510
511
512
513
514
515
516
517
518
519
520
521
522
523
524
525
526
527
528
529
530
531
532
533
534
535
536
537
538
539
540
541
542
543
544
545
546
547
548
549
550
551
552
553
554
555
556
557
558
559
560
561
562
563
564
565
566
567
568
569
570
571
572
573
574
575
576
577
578
579
580
581
582
583
584
585
586
587
588
589
590
591
592
593
594
595
596
597
598
599
600
601
602
603
604
605
606
607
608
609
610
611
612
613
614
615
616
617
618
619
620
621
622
623
624
625
626
627
628
629
630
631
632
633
634
635
636
637
638
639
640
641
642
643
644
645
646
647
648
649
650
651
652
653
654
655
656
657
658
659
660
661
662
663
664
665
666
667
668
669
670
671
672
673
674
675
676
677
678
679
680
681
682
683
684
685
686
687
688
689
690
691
692
693
694
695
696
697
698
699
700
701
702
703
704
705
706
707
708
709
710
711
712
713
714
715
716
717
718
719
720
721
722
723
724
725
726
727
728
729
730
731
732
733
734
735
736
737
738
739
740
741
742
743
744
745
746
747
748
749
750
751
752
753
754
755
756
757
758
759
760
761
762
763
764
765
766
767
768
769
770
771
772
773
774
775
776
777
778
779
780
781
782
783
784
785
786
787
788
789
790
791
792
793
794
795
796
797
798
799
800
801
802
803
804
805
806
807
808
809
810
811
812
813
814
815
816
817
818
819
820
821
822
823
824
|
/***********************************************************
Copyright (c) 2000, BeOpen.com.
Copyright (c) 1995-2000, Corporation for National Research Initiatives.
Copyright (c) 1990-1995, Stichting Mathematisch Centrum.
All rights reserved.
See the file "Misc/COPYRIGHT" for information on usage and
redistribution of this file, and for a DISCLAIMER OF ALL WARRANTIES.
******************************************************************/
/* Time module */
#include "Python.h"
#include <ctype.h>
#ifdef macintosh
#include <time.h>
#include <OSUtils.h>
#ifdef USE_GUSI2
/* GUSI, the I/O library which has the time() function and such uses the
** Mac epoch of 1904. MSL, the C library which has localtime() and so uses
** the ANSI epoch of 1900.
*/
#define GUSI_TO_MSL_EPOCH (4*365*24*60*60)
#endif /* USE_GUSI2 */
#else
#include <sys/types.h>
#endif
#ifdef QUICKWIN
#include <io.h>
#endif
#ifdef HAVE_UNISTD_H
#include <unistd.h>
#endif
#ifdef HAVE_FTIME
#include <sys/timeb.h>
#if !defined(MS_WINDOWS) && !defined(PYOS_OS2)
extern int ftime(struct timeb *);
#endif /* MS_WINDOWS */
#endif /* HAVE_FTIME */
#if defined(__WATCOMC__) && !defined(__QNX__)
#include <i86.h>
#else
#ifdef MS_WINDOWS
#include <windows.h>
#ifdef MS_WIN16
/* These overrides not needed for Win32 */
#define timezone _timezone
#define tzname _tzname
#define daylight _daylight
#define altzone _altzone
#endif /* MS_WIN16 */
#endif /* MS_WINDOWS */
#endif /* !__WATCOMC__ || __QNX__ */
#if defined(MS_WIN32) && !defined(MS_WIN64)
/* Win32 has better clock replacement
XXX Win64 does not yet, but might when the platform matures. */
#include <largeint.h>
#undef HAVE_CLOCK /* We have our own version down below */
#endif /* MS_WIN32 && !MS_WIN64 */
#if defined(PYCC_VACPP)
#include <sys/time.h>
#endif
#ifdef __BEOS__
/* For bigtime_t, snooze(). - [cjh] */
#include <support/SupportDefs.h>
#include <kernel/OS.h>
#ifndef CLOCKS_PER_SEC
/* C'mon, fix the bloody headers... - [cjh] */
#define CLOCKS_PER_SEC 1000
#endif
#endif
/* Forward declarations */
static int floatsleep(double);
static double floattime(void);
/* For Y2K check */
static PyObject *moddict;
#ifdef macintosh
/* Our own timezone. We have enough information to deduce whether
** DST is on currently, but unfortunately we cannot put it to good
** use because we don't know the rules (and that is needed to have
** localtime() return correct tm_isdst values for times other than
** the current time. So, we cop out and only tell the user the current
** timezone.
*/
static long timezone;
static void
initmactimezone(void)
{
MachineLocation loc;
long delta;
ReadLocation(&loc);
if (loc.latitude == 0 && loc.longitude == 0 && loc.u.gmtDelta == 0)
return;
delta = loc.u.gmtDelta & 0x00FFFFFF;
if (delta & 0x00800000)
delta |= 0xFF000000;
timezone = -delta;
}
#endif /* macintosh */
static PyObject *
time_time(PyObject *self, PyObject *args)
{
double secs;
if (!PyArg_NoArgs(args))
return NULL;
secs = floattime();
if (secs == 0.0) {
PyErr_SetFromErrno(PyExc_IOError);
return NULL;
}
return PyFloat_FromDouble(secs);
}
static char time_doc[] =
"time() -> floating point number\n\
\n\
Return the current time in seconds since the Epoch.\n\
Fractions of a second may be present if the system clock provides them.";
#ifdef HAVE_CLOCK
#ifndef CLOCKS_PER_SEC
#ifdef CLK_TCK
#define CLOCKS_PER_SEC CLK_TCK
#else
#define CLOCKS_PER_SEC 1000000
#endif
#endif
static PyObject *
time_clock(PyObject *self, PyObject *args)
{
if (!PyArg_NoArgs(args))
return NULL;
return PyFloat_FromDouble(((double)clock()) / CLOCKS_PER_SEC);
}
#endif /* HAVE_CLOCK */
#if defined(MS_WIN32) && !defined(MS_WIN64)
/* Due to Mark Hammond */
static PyObject *
time_clock(PyObject *self, PyObject *args)
{
static LARGE_INTEGER ctrStart;
static LARGE_INTEGER divisor = {0,0};
LARGE_INTEGER now, diff, rem;
if (!PyArg_NoArgs(args))
return NULL;
if (LargeIntegerEqualToZero(divisor)) {
QueryPerformanceCounter(&ctrStart);
if (!QueryPerformanceFrequency(&divisor) ||
LargeIntegerEqualToZero(divisor)) {
/* Unlikely to happen -
this works on all intel machines at least!
Revert to clock() */
return PyFloat_FromDouble(clock());
}
}
QueryPerformanceCounter(&now);
diff = LargeIntegerSubtract(now, ctrStart);
diff = LargeIntegerDivide(diff, divisor, &rem);
/* XXX - we assume both divide results fit in 32 bits. This is
true on Intels. First person who can afford a machine that
doesnt deserves to fix it :-)
*/
return PyFloat_FromDouble((double)diff.LowPart +
((double)rem.LowPart / (double)divisor.LowPart));
}
#define HAVE_CLOCK /* So it gets included in the methods */
#endif /* MS_WIN32 && !MS_WIN64 */
#ifdef HAVE_CLOCK
static char clock_doc[] =
"clock() -> floating point number\n\
\n\
Return the CPU time or real time since the start of the process or since\n\
the first call to clock(). This has as much precision as the system records.";
#endif
static PyObject *
time_sleep(PyObject *self, PyObject *args)
{
double secs;
if (!PyArg_Parse(args, "d", &secs))
return NULL;
if (floatsleep(secs) != 0)
return NULL;
Py_INCREF(Py_None);
return Py_None;
}
static char sleep_doc[] =
"sleep(seconds)\n\
\n\
Delay execution for a given number of seconds. The argument may be\n\
a floating point number for subsecond precision.";
static PyObject *
tmtotuple(struct tm *p)
{
return Py_BuildValue("(iiiiiiiii)",
p->tm_year + 1900,
p->tm_mon + 1, /* Want January == 1 */
p->tm_mday,
p->tm_hour,
p->tm_min,
p->tm_sec,
(p->tm_wday + 6) % 7, /* Want Monday == 0 */
p->tm_yday + 1, /* Want January, 1 == 1 */
p->tm_isdst);
}
static PyObject *
time_convert(time_t when, struct tm * (*function)(const time_t *))
{
struct tm *p;
errno = 0;
#if defined(macintosh) && defined(USE_GUSI204)
when = when + GUSI_TO_MSL_EPOCH;
#endif
p = function(&when);
if (p == NULL) {
#ifdef EINVAL
if (errno == 0)
errno = EINVAL;
#endif
return PyErr_SetFromErrno(PyExc_IOError);
}
return tmtotuple(p);
}
static PyObject *
time_gmtime(PyObject *self, PyObject *args)
{
double when;
if (!PyArg_Parse(args, "d", &when))
return NULL;
return time_convert((time_t)when, gmtime);
}
static char gmtime_doc[] =
"gmtime(seconds) -> tuple\n\
\n\
Convert seconds since the Epoch to a time tuple expressing UTC (a.k.a. GMT).";
static PyObject *
time_localtime(PyObject *self, PyObject *args)
{
double when;
if (!PyArg_Parse(args, "d", &when))
return NULL;
return time_convert((time_t)when, localtime);
}
static char localtime_doc[] =
"localtime(seconds) -> tuple\n\
Convert seconds since the Epoch to a time tuple expressing local time.";
static int
gettmarg(PyObject *args, struct tm *p)
{
int y;
memset((void *) p, '\0', sizeof(struct tm));
if (!PyArg_Parse(args, "(iiiiiiiii)",
&y,
&p->tm_mon,
&p->tm_mday,
&p->tm_hour,
&p->tm_min,
&p->tm_sec,
&p->tm_wday,
&p->tm_yday,
&p->tm_isdst))
return 0;
if (y < 1900) {
PyObject *accept = PyDict_GetItemString(moddict,
"accept2dyear");
if (accept == NULL || !PyInt_Check(accept) ||
PyInt_AsLong(accept) == 0) {
PyErr_SetString(PyExc_ValueError,
"year >= 1900 required");
return 0;
}
if (69 <= y && y <= 99)
y += 1900;
else if (0 <= y && y <= 68)
y += 2000;
else {
PyErr_SetString(PyExc_ValueError,
"year out of range (00-99, 1900-*)");
return 0;
}
}
p->tm_year = y - 1900;
p->tm_mon--;
p->tm_wday = (p->tm_wday + 1) % 7;
p->tm_yday--;
return 1;
}
#ifdef HAVE_STRFTIME
static PyObject *
time_strftime(PyObject *self, PyObject *args)
{
PyObject *tup;
struct tm buf;
const char *fmt;
size_t fmtlen, buflen;
char *outbuf = 0;
size_t i;
memset((void *) &buf, '\0', sizeof(buf));
if (!PyArg_ParseTuple(args, "sO:strftime", &fmt, &tup)
|| !gettmarg(tup, &buf))
return NULL;
fmtlen = strlen(fmt);
/* I hate these functions that presume you know how big the output
* will be ahead of time...
*/
for (i = 1024; ; i += i) {
outbuf = malloc(i);
if (outbuf == NULL) {
return PyErr_NoMemory();
}
buflen = strftime(outbuf, i, fmt, &buf);
if (buflen > 0 || i >= 256 * fmtlen) {
/* If the buffer is 256 times as long as the format,
it's probably not failing for lack of room!
More likely, the format yields an empty result,
e.g. an empty format, or %Z when the timezone
is unknown. */
PyObject *ret;
ret = PyString_FromStringAndSize(outbuf, buflen);
free(outbuf);
return ret;
}
free(outbuf);
}
}
static char strftime_doc[] =
"strftime(format, tuple) -> string\n\
\n\
Convert a time tuple to a string according to a format specification.\n\
See the library reference manual for formatting codes.";
#endif /* HAVE_STRFTIME */
#ifdef HAVE_STRPTIME
#if 0
/* Enable this if it's not declared in <time.h> */
extern char *strptime(const char *, const char *, struct tm *);
#endif
static PyObject *
time_strptime(PyObject *self, PyObject *args)
{
struct tm tm;
char *fmt = "%a %b %d %H:%M:%S %Y";
char *buf;
char *s;
if (!PyArg_ParseTuple(args, "s|s:strptime", &buf, &fmt))
return NULL;
memset((void *) &tm, '\0', sizeof(tm));
s = strptime(buf, fmt, &tm);
if (s == NULL) {
PyErr_SetString(PyExc_ValueError, "format mismatch");
return NULL;
}
while (*s && isspace(*s))
s++;
if (*s) {
PyErr_Format(PyExc_ValueError,
"unconverted data remains: '%.400s'", s);
return NULL;
}
return tmtotuple(&tm);
}
static char strptime_doc[] =
"strptime(string, format) -> tuple\n\
Parse a string to a time tuple according to a format specification.\n\
See the library reference manual for formatting codes (same as strftime()).";
#endif /* HAVE_STRPTIME */
static PyObject *
time_asctime(PyObject *self, PyObject *args)
{
PyObject *tup;
struct tm buf;
char *p;
if (!PyArg_ParseTuple(args, "O:asctime", &tup))
return NULL;
if (!gettmarg(tup, &buf))
return NULL;
p = asctime(&buf);
if (p[24] == '\n')
p[24] = '\0';
return PyString_FromString(p);
}
static char asctime_doc[] =
"asctime(tuple) -> string\n\
\n\
Convert a time tuple to a string, e.g. 'Sat Jun 06 16:26:11 1998'.";
static PyObject *
time_ctime(PyObject *self, PyObject *args)
{
double dt;
time_t tt;
char *p;
if (!PyArg_Parse(args, "d", &dt))
return NULL;
tt = (time_t)dt;
#if defined(macintosh) && defined(USE_GUSI204)
tt = tt + GUSI_TO_MSL_EPOCH;
#endif
p = ctime(&tt);
if (p == NULL) {
PyErr_SetString(PyExc_ValueError, "unconvertible time");
return NULL;
}
if (p[24] == '\n')
p[24] = '\0';
return PyString_FromString(p);
}
static char ctime_doc[] =
"ctime(seconds) -> string\n\
\n\
Convert a time in seconds since the Epoch to a string in local time.\n\
This is equivalent to asctime(localtime(seconds)).";
#ifdef HAVE_MKTIME
static PyObject *
time_mktime(PyObject *self, PyObject *args)
{
PyObject *tup;
struct tm buf;
time_t tt;
if (!PyArg_ParseTuple(args, "O:mktime", &tup))
return NULL;
tt = time(&tt);
buf = *localtime(&tt);
if (!gettmarg(tup, &buf))
return NULL;
tt = mktime(&buf);
if (tt == (time_t)(-1)) {
PyErr_SetString(PyExc_OverflowError,
"mktime argument out of range");
return NULL;
}
#if defined(macintosh) && defined(USE_GUSI2)
tt = tt - GUSI_TO_MSL_EPOCH;
#endif
return PyFloat_FromDouble((double)tt);
}
static char mktime_doc[] =
"mktime(tuple) -> floating point number\n\
\n\
Convert a time tuple in local time to seconds since the Epoch.";
#endif /* HAVE_MKTIME */
static PyMethodDef time_methods[] = {
{"time", time_time, 0, time_doc},
#ifdef HAVE_CLOCK
{"clock", time_clock, 0, clock_doc},
#endif
{"sleep", time_sleep, 0, sleep_doc},
{"gmtime", time_gmtime, 0, gmtime_doc},
{"localtime", time_localtime, 0, localtime_doc},
{"asctime", time_asctime, 1, asctime_doc},
{"ctime", time_ctime, 0, ctime_doc},
#ifdef HAVE_MKTIME
{"mktime", time_mktime, 1, mktime_doc},
#endif
#ifdef HAVE_STRFTIME
{"strftime", time_strftime, 1, strftime_doc},
#endif
#ifdef HAVE_STRPTIME
{"strptime", time_strptime, 1, strptime_doc},
#endif
{NULL, NULL} /* sentinel */
};
static void
ins(PyObject *d, char *name, PyObject *v)
{
if (v == NULL)
Py_FatalError("Can't initialize time module -- NULL value");
if (PyDict_SetItemString(d, name, v) != 0)
Py_FatalError(
"Can't initialize time module -- PyDict_SetItemString failed");
Py_DECREF(v);
}
static char module_doc[] =
"This module provides various functions to manipulate time values.\n\
\n\
There are two standard representations of time. One is the number\n\
of seconds since the Epoch, in UTC (a.k.a. GMT). It may be an integer\n\
or a floating point number (to represent fractions of seconds).\n\
The Epoch is system-defined; on Unix, it is generally January 1st, 1970.\n\
The actual value can be retrieved by calling gmtime(0).\n\
\n\
The other representation is a tuple of 9 integers giving local time.\n\
The tuple items are:\n\
year (four digits, e.g. 1998)\n\
month (1-12)\n\
day (1-31)\n\
hours (0-23)\n\
minutes (0-59)\n\
seconds (0-59)\n\
weekday (0-6, Monday is 0)\n\
Julian day (day in the year, 1-366)\n\
DST (Daylight Savings Time) flag (-1, 0 or 1)\n\
If the DST flag is 0, the time is given in the regular time zone;\n\
if it is 1, the time is given in the DST time zone;\n\
if it is -1, mktime() should guess based on the date and time.\n\
\n\
Variables:\n\
\n\
timezone -- difference in seconds between UTC and local standard time\n\
altzone -- difference in seconds between UTC and local DST time\n\
daylight -- whether local time should reflect DST\n\
tzname -- tuple of (standard time zone name, DST time zone name)\n\
\n\
Functions:\n\
\n\
time() -- return current time in seconds since the Epoch as a float\n\
clock() -- return CPU time since process start as a float\n\
sleep() -- delay for a number of seconds given as a float\n\
gmtime() -- convert seconds since Epoch to UTC tuple\n\
localtime() -- convert seconds since Epoch to local time tuple\n\
asctime() -- convert time tuple to string\n\
ctime() -- convert time in seconds to string\n\
mktime() -- convert local time tuple to seconds since Epoch\n\
strftime() -- convert time tuple to string according to format specification\n\
strptime() -- parse string to time tuple according to format specification\n\
";
DL_EXPORT(void)
inittime(void)
{
PyObject *m, *d;
char *p;
m = Py_InitModule3("time", time_methods, module_doc);
d = PyModule_GetDict(m);
/* Accept 2-digit dates unless PYTHONY2K is set and non-empty */
p = getenv("PYTHONY2K");
ins(d, "accept2dyear", PyInt_FromLong((long) (!p || !*p)));
/* Squirrel away the module's dictionary for the y2k check */
Py_INCREF(d);
moddict = d;
#if defined(HAVE_TZNAME) && !defined(__GLIBC__)
tzset();
#ifdef PYOS_OS2
ins(d, "timezone", PyInt_FromLong((long)_timezone));
#else /* !PYOS_OS2 */
ins(d, "timezone", PyInt_FromLong((long)timezone));
#endif /* PYOS_OS2 */
#ifdef HAVE_ALTZONE
ins(d, "altzone", PyInt_FromLong((long)altzone));
#else
#ifdef PYOS_OS2
ins(d, "altzone", PyInt_FromLong((long)_timezone-3600));
#else /* !PYOS_OS2 */
ins(d, "altzone", PyInt_FromLong((long)timezone-3600));
#endif /* PYOS_OS2 */
#endif
ins(d, "daylight", PyInt_FromLong((long)daylight));
ins(d, "tzname", Py_BuildValue("(zz)", tzname[0], tzname[1]));
#else /* !HAVE_TZNAME || __GLIBC__ */
#ifdef HAVE_TM_ZONE
{
#define YEAR ((time_t)((365 * 24 + 6) * 3600))
time_t t;
struct tm *p;
long janzone, julyzone;
char janname[10], julyname[10];
t = (time((time_t *)0) / YEAR) * YEAR;
p = localtime(&t);
janzone = -p->tm_gmtoff;
strncpy(janname, p->tm_zone ? p->tm_zone : " ", 9);
janname[9] = '\0';
t += YEAR/2;
p = localtime(&t);
julyzone = -p->tm_gmtoff;
strncpy(julyname, p->tm_zone ? p->tm_zone : " ", 9);
julyname[9] = '\0';
if( janzone < julyzone ) {
/* DST is reversed in the southern hemisphere */
ins(d, "timezone", PyInt_FromLong(julyzone));
ins(d, "altzone", PyInt_FromLong(janzone));
ins(d, "daylight",
PyInt_FromLong((long)(janzone != julyzone)));
ins(d, "tzname",
Py_BuildValue("(zz)", julyname, janname));
} else {
ins(d, "timezone", PyInt_FromLong(janzone));
ins(d, "altzone", PyInt_FromLong(julyzone));
ins(d, "daylight",
PyInt_FromLong((long)(janzone != julyzone)));
ins(d, "tzname",
Py_BuildValue("(zz)", janname, julyname));
}
}
#else
#ifdef macintosh
/* The only thing we can obtain is the current timezone
** (and whether dst is currently _active_, but that is not what
** we're looking for:-( )
*/
initmactimezone();
ins(d, "timezone", PyInt_FromLong(timezone));
ins(d, "altzone", PyInt_FromLong(timezone));
ins(d, "daylight", PyInt_FromLong((long)0));
ins(d, "tzname", Py_BuildValue("(zz)", "", ""));
#endif /* macintosh */
#endif /* HAVE_TM_ZONE */
#endif /* !HAVE_TZNAME || __GLIBC__ */
if (PyErr_Occurred())
Py_FatalError("Can't initialize time module");
}
/* Implement floattime() for various platforms */
static double
floattime(void)
{
/* There are three ways to get the time:
(1) gettimeofday() -- resolution in microseconds
(2) ftime() -- resolution in milliseconds
(3) time() -- resolution in seconds
In all cases the return value is a float in seconds.
Since on some systems (e.g. SCO ODT 3.0) gettimeofday() may
fail, so we fall back on ftime() or time().
Note: clock resolution does not imply clock accuracy! */
#ifdef HAVE_GETTIMEOFDAY
{
struct timeval t;
#ifdef GETTIMEOFDAY_NO_TZ
if (gettimeofday(&t) == 0)
return (double)t.tv_sec + t.tv_usec*0.000001;
#else /* !GETTIMEOFDAY_NO_TZ */
if (gettimeofday(&t, (struct timezone *)NULL) == 0)
return (double)t.tv_sec + t.tv_usec*0.000001;
#endif /* !GETTIMEOFDAY_NO_TZ */
}
#endif /* !HAVE_GETTIMEOFDAY */
{
#if defined(HAVE_FTIME)
struct timeb t;
ftime(&t);
return (double)t.time + (double)t.millitm * (double)0.001;
#else /* !HAVE_FTIME */
time_t secs;
time(&secs);
return (double)secs;
#endif /* !HAVE_FTIME */
}
}
/* Implement floatsleep() for various platforms.
When interrupted (or when another error occurs), return -1 and
set an exception; else return 0. */
static int
floatsleep(double secs)
{
/* XXX Should test for MS_WIN32 first! */
#if defined(HAVE_SELECT) && !defined(__BEOS__)
struct timeval t;
double frac;
frac = fmod(secs, 1.0);
secs = floor(secs);
t.tv_sec = (long)secs;
t.tv_usec = (long)(frac*1000000.0);
Py_BEGIN_ALLOW_THREADS
if (select(0, (fd_set *)0, (fd_set *)0, (fd_set *)0, &t) != 0) {
#ifdef EINTR
if (errno != EINTR) {
#else
if (1) {
#endif
Py_BLOCK_THREADS
PyErr_SetFromErrno(PyExc_IOError);
return -1;
}
}
Py_END_ALLOW_THREADS
#else /* !HAVE_SELECT || __BEOS__ */
#ifdef macintosh
#define MacTicks (* (long *)0x16A)
long deadline;
deadline = MacTicks + (long)(secs * 60.0);
while (MacTicks < deadline) {
/* XXX Should call some yielding function here */
if (PyErr_CheckSignals())
return -1;
}
#else /* !macintosh */
#if defined(__WATCOMC__) && !defined(__QNX__)
/* XXX Can't interrupt this sleep */
Py_BEGIN_ALLOW_THREADS
delay((int)(secs * 1000 + 0.5)); /* delay() uses milliseconds */
Py_END_ALLOW_THREADS
#else /* !__WATCOMC__ || __QNX__ */
#ifdef MSDOS
struct timeb t1, t2;
double frac;
extern double fmod(double, double);
extern double floor(double);
if (secs <= 0.0)
return;
frac = fmod(secs, 1.0);
secs = floor(secs);
ftime(&t1);
t2.time = t1.time + (int)secs;
t2.millitm = t1.millitm + (int)(frac*1000.0);
while (t2.millitm >= 1000) {
t2.time++;
t2.millitm -= 1000;
}
for (;;) {
#ifdef QUICKWIN
Py_BEGIN_ALLOW_THREADS
_wyield();
Py_END_ALLOW_THREADS
#endif
if (PyErr_CheckSignals())
return -1;
ftime(&t1);
if (t1.time > t2.time ||
t1.time == t2.time && t1.millitm >= t2.millitm)
break;
}
#else /* !MSDOS */
#ifdef MS_WIN32
{
double millisecs = secs * 1000.0;
if (millisecs > (double)ULONG_MAX) {
PyErr_SetString(PyExc_OverflowError, "sleep length is too large");
return -1;
}
/* XXX Can't interrupt this sleep */
Py_BEGIN_ALLOW_THREADS
Sleep((unsigned long)millisecs);
Py_END_ALLOW_THREADS
}
#else /* !MS_WIN32 */
#ifdef PYOS_OS2
/* This Sleep *IS* Interruptable by Exceptions */
Py_BEGIN_ALLOW_THREADS
if (DosSleep(secs * 1000) != NO_ERROR) {
Py_BLOCK_THREADS
PyErr_SetFromErrno(PyExc_IOError);
return -1;
}
Py_END_ALLOW_THREADS
#else /* !PYOS_OS2 */
#ifdef __BEOS__
/* This sleep *CAN BE* interrupted. */
{
if( secs <= 0.0 ) {
return;
}
Py_BEGIN_ALLOW_THREADS
/* BeOS snooze() is in microseconds... */
if( snooze( (bigtime_t)( secs * 1000.0 * 1000.0 ) ) == B_INTERRUPTED ) {
Py_BLOCK_THREADS
PyErr_SetFromErrno( PyExc_IOError );
return -1;
}
Py_END_ALLOW_THREADS
}
#else /* !__BEOS__ */
/* XXX Can't interrupt this sleep */
Py_BEGIN_ALLOW_THREADS
sleep((int)secs);
Py_END_ALLOW_THREADS
#endif /* !__BEOS__ */
#endif /* !PYOS_OS2 */
#endif /* !MS_WIN32 */
#endif /* !MSDOS */
#endif /* !__WATCOMC__ || __QNX__ */
#endif /* !macintosh */
#endif /* !HAVE_SELECT */
return 0;
}
|