| /*********************************************************** | 
 | 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, 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) | 
 | { | 
 | 	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; | 
 | } |