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			811 lines
		
	
	
	
		
			20 KiB
		
	
	
	
		
			C
		
	
	
	
	
	
			
		
		
	
	
			811 lines
		
	
	
	
		
			20 KiB
		
	
	
	
		
			C
		
	
	
	
	
	
| 
 | |
| /* Time module */
 | |
| 
 | |
| #include "Python.h"
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| 
 | |
| #include <ctype.h>
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| 
 | |
| #ifdef macintosh
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| #include <time.h>
 | |
| #include <OSUtils.h>
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| #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
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| #include <sys/types.h>
 | |
| #endif
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| 
 | |
| #ifdef QUICKWIN
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| #include <io.h>
 | |
| #endif
 | |
| 
 | |
| #ifdef HAVE_UNISTD_H
 | |
| #include <unistd.h>
 | |
| #endif
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| 
 | |
| #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__
 | |
| #include <time.h>
 | |
| /* For bigtime_t, snooze(). - [cjh] */
 | |
| #include <support/SupportDefs.h>
 | |
| #include <kernel/OS.h>
 | |
| #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\
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| \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 *
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| tmtotuple(struct tm *p)
 | |
| {
 | |
| 	return Py_BuildValue("(iiiiiiiii)",
 | |
| 			     p->tm_year + 1900,
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| 			     p->tm_mon + 1,	   /* Want January == 1 */
 | |
| 			     p->tm_mday,
 | |
| 			     p->tm_hour,
 | |
| 			     p->tm_min,
 | |
| 			     p->tm_sec,
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| 			     (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;
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| #if defined(macintosh) && defined(USE_GUSI204)
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| 	when = when + GUSI_TO_MSL_EPOCH;
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| #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))
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| 		return NULL;
 | |
| 	return time_convert((time_t)when, gmtime);
 | |
| }
 | |
| 
 | |
| static char gmtime_doc[] =
 | |
| "gmtime(seconds) -> tuple\n\
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| \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[] =
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| "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,
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| 			 &p->tm_isdst))
 | |
| 		return 0;
 | |
| 	if (y < 1900) {
 | |
| 		PyObject *accept = PyDict_GetItemString(moddict,
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| 							"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, METH_OLDARGS, time_doc},
 | |
| #ifdef HAVE_CLOCK
 | |
| 	{"clock",	time_clock, METH_OLDARGS, clock_doc},
 | |
| #endif
 | |
| 	{"sleep",	time_sleep, METH_OLDARGS, sleep_doc},
 | |
| 	{"gmtime",	time_gmtime, METH_OLDARGS, gmtime_doc},
 | |
| 	{"localtime",	time_localtime, METH_OLDARGS, localtime_doc},
 | |
| 	{"asctime",	time_asctime, METH_VARARGS, asctime_doc},
 | |
| 	{"ctime",	time_ctime, METH_OLDARGS, ctime_doc},
 | |
| #ifdef HAVE_MKTIME
 | |
| 	{"mktime",	time_mktime, METH_VARARGS, mktime_doc},
 | |
| #endif
 | |
| #ifdef HAVE_STRFTIME
 | |
| 	{"strftime",	time_strftime, METH_VARARGS, strftime_doc},
 | |
| #endif
 | |
| #ifdef HAVE_STRPTIME
 | |
| 	{"strptime",	time_strptime, METH_VARARGS, strptime_doc},
 | |
| #endif
 | |
| 	{NULL,		NULL}		/* sentinel */
 | |
| };
 | |
| 
 | |
| static void
 | |
| ins(PyObject *d, char *name, PyObject *v)
 | |
| {
 | |
| 	/* Don't worry too much about errors, they'll be caught by the
 | |
| 	 * caller of inittime().
 | |
| 	 */
 | |
| 	if (v)
 | |
| 		PyDict_SetItemString(d, name, v);
 | |
| 	Py_XDECREF(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__ */
 | |
| }
 | |
| 
 | |
| 
 | |
| /* 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;
 | |
| }
 | 
