| |
| /* Time module */ |
| |
| #include "Python.h" |
| |
| #include <ctype.h> |
| |
| #ifdef macintosh |
| #include <time.h> |
| #include <OSUtils.h> |
| #ifdef USE_GUSI211 |
| /* 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__ |
| #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_ParseTuple(args, ":time")) |
| 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_ParseTuple(args, ":clock")) |
| 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_ParseTuple(args, ":clock")) |
| 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_ParseTuple(args, "d:sleep", &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 (PyTuple_Size(args) == 0) |
| when = floattime(); |
| if (!PyArg_ParseTuple(args, "|d:gmtime", &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.\n\ |
| GMT). When 'seconds' is not passed in, convert the current time instead."; |
| |
| static PyObject * |
| time_localtime(PyObject *self, PyObject *args) |
| { |
| double when; |
| if (PyTuple_Size(args) == 0) |
| when = floattime(); |
| if (!PyArg_ParseTuple(args, "|d:localtime", &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.\n\ |
| When 'seconds' is not passed in, convert the current time instead."; |
| |
| 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 = NULL; |
| 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, "s|O:strftime", &fmt, &tup)) |
| return NULL; |
| |
| if (tup == NULL) { |
| time_t tt = time(NULL); |
| buf = *localtime(&tt); |
| } else if (!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. When the time tuple\n\ |
| is not present, current time as returned by localtime() is used."; |
| #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 = NULL; |
| struct tm buf; |
| char *p; |
| if (!PyArg_ParseTuple(args, "|O:asctime", &tup)) |
| return NULL; |
| if (tup == NULL) { |
| time_t tt = time(NULL); |
| buf = *localtime(&tt); |
| } else 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'.\n\ |
| When the time tuple is not present, current time as returned by localtime()\n\ |
| is used."; |
| |
| static PyObject * |
| time_ctime(PyObject *self, PyObject *args) |
| { |
| double dt; |
| time_t tt; |
| char *p; |
| |
| if (PyTuple_Size(args) == 0) |
| tt = time(NULL); |
| else { |
| if (!PyArg_ParseTuple(args, "|d:ctime", &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)). When the time tuple is\n\ |
| not present, current time as returned by localtime() is used."; |
| |
| #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_GUSI211) |
| 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_VARARGS, time_doc}, |
| #ifdef HAVE_CLOCK |
| {"clock", time_clock, METH_VARARGS, clock_doc}, |
| #endif |
| {"sleep", time_sleep, METH_VARARGS, sleep_doc}, |
| {"gmtime", time_gmtime, METH_VARARGS, gmtime_doc}, |
| {"localtime", time_localtime, METH_VARARGS, localtime_doc}, |
| {"asctime", time_asctime, METH_VARARGS, asctime_doc}, |
| {"ctime", time_ctime, METH_VARARGS, 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; |
| } |