ntp_calendar.c revision 275970
1/*
2 * ntp_calendar.c - calendar and helper functions
3 *
4 * Written by Juergen Perlinger (perlinger@ntp.org) for the NTP project.
5 * The contents of 'html/copyright.html' apply.
6 */
7#include <config.h>
8#include <sys/types.h>
9
10#include "ntp_types.h"
11#include "ntp_calendar.h"
12#include "ntp_stdlib.h"
13#include "ntp_fp.h"
14#include "ntp_unixtime.h"
15
16/*
17 *---------------------------------------------------------------------
18 * replacing the 'time()' function
19 * --------------------------------------------------------------------
20 */
21
22static systime_func_ptr systime_func = &time;
23static inline time_t now(void);
24
25
26systime_func_ptr
27ntpcal_set_timefunc(
28	systime_func_ptr nfunc
29	)
30{
31	systime_func_ptr res;
32
33	res = systime_func;
34	if (NULL == nfunc)
35		nfunc = &time;
36	systime_func = nfunc;
37
38	return res;
39}
40
41
42static inline time_t
43now(void)
44{
45	return (*systime_func)(NULL);
46}
47
48/*
49 *---------------------------------------------------------------------
50 * Convert between 'time_t' and 'vint64'
51 *---------------------------------------------------------------------
52 */
53vint64
54time_to_vint64(
55	const time_t * ptt
56	)
57{
58	vint64 res;
59	time_t tt;
60
61	tt = *ptt;
62
63#if SIZEOF_TIME_T <= 4
64
65	res.D_s.hi = 0;
66	if (tt < 0) {
67		res.D_s.lo = (uint32_t)-tt;
68		M_NEG(res.D_s.hi, res.D_s.lo);
69	} else {
70		res.D_s.lo = (uint32_t)tt;
71	}
72
73#elif defined(HAVE_INT64)
74
75	res.q_s = tt;
76
77#else
78	/*
79	 * shifting negative signed quantities is compiler-dependent, so
80	 * we better avoid it and do it all manually. And shifting more
81	 * than the width of a quantity is undefined. Also a don't do!
82	 */
83	if (tt < 0) {
84		tt = -tt;
85		res.D_s.lo = (uint32_t)tt;
86		res.D_s.hi = (uint32_t)(tt >> 32);
87		M_NEG(res.D_s.hi, res.D_s.lo);
88	} else {
89		res.D_s.lo = (uint32_t)tt;
90		res.D_s.hi = (uint32_t)(tt >> 32);
91	}
92
93#endif
94
95	return res;
96}
97
98
99time_t
100vint64_to_time(
101	const vint64 *tv
102	)
103{
104	time_t res;
105
106#if SIZEOF_TIME_T <= 4
107
108	res = (time_t)tv->D_s.lo;
109
110#elif defined(HAVE_INT64)
111
112	res = (time_t)tv->q_s;
113
114#else
115
116	res = ((time_t)tv->d_s.hi << 32) | tv->D_s.lo;
117
118#endif
119
120	return res;
121}
122
123/*
124 *---------------------------------------------------------------------
125 * Get the build date & time
126 *---------------------------------------------------------------------
127 */
128int
129ntpcal_get_build_date(
130	struct calendar * jd
131	)
132{
133	/* The C standard tells us the format of '__DATE__':
134	 *
135	 * __DATE__ The date of translation of the preprocessing
136	 * translation unit: a character string literal of the form "Mmm
137	 * dd yyyy", where the names of the months are the same as those
138	 * generated by the asctime function, and the first character of
139	 * dd is a space character if the value is less than 10. If the
140	 * date of translation is not available, an
141	 * implementation-defined valid date shall be supplied.
142	 *
143	 * __TIME__ The time of translation of the preprocessing
144	 * translation unit: a character string literal of the form
145	 * "hh:mm:ss" as in the time generated by the asctime
146	 * function. If the time of translation is not available, an
147	 * implementation-defined valid time shall be supplied.
148	 *
149	 * Note that MSVC declares DATE and TIME to be in the local time
150	 * zone, while neither the C standard nor the GCC docs make any
151	 * statement about this. As a result, we may be +/-12hrs off
152	 * UTC.  But for practical purposes, this should not be a
153	 * problem.
154	 *
155	 */
156	static const char build[] = __TIME__ "/" __DATE__;
157	static const char mlist[] = "JanFebMarAprMayJunJulAugSepOctNovDec";
158
159	char		  monstr[4];
160	const char *	  cp;
161	unsigned short	  hour, minute, second, day, year;
162 	/* Note: The above quantities are used for sscanf 'hu' format,
163	 * so using 'uint16_t' is contra-indicated!
164	 */
165
166#ifdef DEBUG
167	static int        ignore  = 0;
168#endif
169
170	ZERO(*jd);
171	jd->year     = 1970;
172	jd->month    = 1;
173	jd->monthday = 1;
174
175#ifdef DEBUG
176	/* check environment if build date should be ignored */
177	if (0 == ignore) {
178	    const char * envstr;
179	    envstr = getenv("NTPD_IGNORE_BUILD_DATE");
180	    ignore = 1 + (envstr && (!*envstr || !strcasecmp(envstr, "yes")));
181	}
182	if (ignore > 1)
183	    return FALSE;
184#endif
185
186	if (6 == sscanf(build, "%hu:%hu:%hu/%3s %hu %hu",
187			&hour, &minute, &second, monstr, &day, &year)) {
188		cp = strstr(mlist, monstr);
189		if (NULL != cp) {
190			jd->year     = year;
191			jd->month    = (uint8_t)((cp - mlist) / 3 + 1);
192			jd->monthday = (uint8_t)day;
193			jd->hour     = (uint8_t)hour;
194			jd->minute   = (uint8_t)minute;
195			jd->second   = (uint8_t)second;
196
197			return TRUE;
198		}
199	}
200
201	return FALSE;
202}
203
204
205/*
206 *---------------------------------------------------------------------
207 * basic calendar stuff
208 * --------------------------------------------------------------------
209 */
210
211/* month table for a year starting with March,1st */
212static const uint16_t shift_month_table[13] = {
213	0, 31, 61, 92, 122, 153, 184, 214, 245, 275, 306, 337, 366
214};
215
216/* month tables for years starting with January,1st; regular & leap */
217static const uint16_t real_month_table[2][13] = {
218	/* -*- table for regular years -*- */
219	{ 0, 31, 59, 90, 120, 151, 181, 212, 243, 273, 304, 334, 365 },
220	/* -*- table for leap years -*- */
221	{ 0, 31, 60, 91, 121, 152, 182, 213, 244, 274, 305, 335, 366 }
222};
223
224/*
225 * Some notes on the terminology:
226 *
227 * We use the proleptic Gregorian calendar, which is the Gregorian
228 * calendar extended in both directions ad infinitum. This totally
229 * disregards the fact that this calendar was invented in 1582, and
230 * was adopted at various dates over the world; sometimes even after
231 * the start of the NTP epoch.
232 *
233 * Normally date parts are given as current cycles, while time parts
234 * are given as elapsed cycles:
235 *
236 * 1970-01-01/03:04:05 means 'IN the 1970st. year, IN the first month,
237 * ON the first day, with 3hrs, 4minutes and 5 seconds elapsed.
238 *
239 * The basic calculations for this calendar implementation deal with
240 * ELAPSED date units, which is the number of full years, full months
241 * and full days before a date: 1970-01-01 would be (1969, 0, 0) in
242 * that notation.
243 *
244 * To ease the numeric computations, month and day values outside the
245 * normal range are acceptable: 2001-03-00 will be treated as the day
246 * before 2001-03-01, 2000-13-32 will give the same result as
247 * 2001-02-01 and so on.
248 *
249 * 'rd' or 'RD' is used as an abbreviation for the latin 'rata die'
250 * (day number).  This is the number of days elapsed since 0000-12-31
251 * in the proleptic Gregorian calendar. The begin of the Christian Era
252 * (0001-01-01) is RD(1).
253 *
254 *
255 * Some notes on the implementation:
256 *
257 * Calendar algorithms thrive on the division operation, which is one of
258 * the slowest numerical operations in any CPU. What saves us here from
259 * abysmal performance is the fact that all divisions are divisions by
260 * constant numbers, and most compilers can do this by a multiplication
261 * operation.  But this might not work when using the div/ldiv/lldiv
262 * function family, because many compilers are not able to do inline
263 * expansion of the code with following optimisation for the
264 * constant-divider case.
265 *
266 * Also div/ldiv/lldiv are defined in terms of int/long/longlong, which
267 * are inherently target dependent. Nothing that could not be cured with
268 * autoconf, but still a mess...
269 *
270 * Furthermore, we need floor division while C demands truncation to
271 * zero, so additional steps are required to make sure the algorithms
272 * work.
273 *
274 * For all this, all divisions by constant are coded manually, even when
275 * there is a joined div/mod operation: The optimiser should sort that
276 * out, if possible.
277 *
278 * Finally, the functions do not check for overflow conditions. This
279 * is a sacrifice made for execution speed; since a 32-bit day counter
280 * covers +/- 5,879,610 years, this should not pose a problem here.
281 */
282
283
284/*
285 * ==================================================================
286 *
287 * General algorithmic stuff
288 *
289 * ==================================================================
290 */
291
292/*
293 *---------------------------------------------------------------------
294 * Do a periodic extension of 'value' around 'pivot' with a period of
295 * 'cycle'.
296 *
297 * The result 'res' is a number that holds to the following properties:
298 *
299 *   1)	 res MOD cycle == value MOD cycle
300 *   2)	 pivot <= res < pivot + cycle
301 *	 (replace </<= with >/>= for negative cycles)
302 *
303 * where 'MOD' denotes the modulo operator for FLOOR DIVISION, which
304 * is not the same as the '%' operator in C: C requires division to be
305 * a truncated division, where remainder and dividend have the same
306 * sign if the remainder is not zero, whereas floor division requires
307 * divider and modulus to have the same sign for a non-zero modulus.
308 *
309 * This function has some useful applications:
310 *
311 * + let Y be a calendar year and V a truncated 2-digit year: then
312 *	periodic_extend(Y-50, V, 100)
313 *   is the closest expansion of the truncated year with respect to
314 *   the full year, that is a 4-digit year with a difference of less
315 *   than 50 years to the year Y. ("century unfolding")
316 *
317 * + let T be a UN*X time stamp and V be seconds-of-day: then
318 *	perodic_extend(T-43200, V, 86400)
319 *   is a time stamp that has the same seconds-of-day as the input
320 *   value, with an absolute difference to T of <= 12hrs.  ("day
321 *   unfolding")
322 *
323 * + Wherever you have a truncated periodic value and a non-truncated
324 *   base value and you want to match them somehow...
325 *
326 * Basically, the function delivers 'pivot + (value - pivot) % cycle',
327 * but the implementation takes some pains to avoid internal signed
328 * integer overflows in the '(value - pivot) % cycle' part and adheres
329 * to the floor division convention.
330 *
331 * If 64bit scalars where available on all intended platforms, writing a
332 * version that uses 64 bit ops would be easy; writing a general
333 * division routine for 64bit ops on a platform that can only do
334 * 32/16bit divisions and is still performant is a bit more
335 * difficult. Since most usecases can be coded in a way that does only
336 * require the 32-bit version a 64bit version is NOT provided here.
337 * ---------------------------------------------------------------------
338 */
339int32_t
340ntpcal_periodic_extend(
341	int32_t pivot,
342	int32_t value,
343	int32_t cycle
344	)
345{
346	uint32_t diff;
347	char	 cpl = 0; /* modulo complement flag */
348	char	 neg = 0; /* sign change flag	    */
349
350	/* make the cycle positive and adjust the flags */
351	if (cycle < 0) {
352		cycle = - cycle;
353		neg ^= 1;
354		cpl ^= 1;
355	}
356	/* guard against div by zero or one */
357	if (cycle > 1) {
358		/*
359		 * Get absolute difference as unsigned quantity and
360		 * the complement flag. This is done by always
361		 * subtracting the smaller value from the bigger
362		 * one. This implementation works only on a two's
363		 * complement machine!
364		 */
365		if (value >= pivot) {
366			diff = (uint32_t)value - (uint32_t)pivot;
367		} else {
368			diff = (uint32_t)pivot - (uint32_t)value;
369			cpl ^= 1;
370		}
371		diff %= (uint32_t)cycle;
372		if (diff) {
373			if (cpl)
374				diff = cycle - diff;
375			if (neg)
376				diff = ~diff + 1;
377			pivot += diff;
378		}
379	}
380	return pivot;
381}
382
383/*
384 *-------------------------------------------------------------------
385 * Convert a timestamp in NTP scale to a 64bit seconds value in the UN*X
386 * scale with proper epoch unfolding around a given pivot or the current
387 * system time. This function happily accepts negative pivot values as
388 * timestamps befor 1970-01-01, so be aware of possible trouble on
389 * platforms with 32bit 'time_t'!
390 *
391 * This is also a periodic extension, but since the cycle is 2^32 and
392 * the shift is 2^31, we can do some *very* fast math without explicit
393 * divisions.
394 *-------------------------------------------------------------------
395 */
396vint64
397ntpcal_ntp_to_time(
398	uint32_t	ntp,
399	const time_t *	pivot
400	)
401{
402	vint64 res;
403
404#ifdef HAVE_INT64
405
406	res.q_s = (pivot != NULL)
407		      ? *pivot
408		      : now();
409	res.Q_s -= 0x80000000;		/* unshift of half range */
410	ntp	-= (uint32_t)JAN_1970;	/* warp into UN*X domain */
411	ntp	-= res.D_s.lo;		/* cycle difference	 */
412	res.Q_s += (uint64_t)ntp;	/* get expanded time	 */
413
414#else /* no 64bit scalars */
415
416	time_t tmp;
417
418	tmp = (pivot != NULL)
419		  ? *pivot
420		  : now();
421	res = time_to_vint64(&tmp);
422	M_SUB(res.D_s.hi, res.D_s.lo, 0, 0x80000000);
423	ntp -= (uint32_t)JAN_1970;	/* warp into UN*X domain */
424	ntp -= res.D_s.lo;		/* cycle difference	 */
425	M_ADD(res.D_s.hi, res.D_s.lo, 0, ntp);
426
427#endif /* no 64bit scalars */
428
429	return res;
430}
431
432/*
433 *-------------------------------------------------------------------
434 * Convert a timestamp in NTP scale to a 64bit seconds value in the NTP
435 * scale with proper epoch unfolding around a given pivot or the current
436 * system time.
437 *
438 * Note: The pivot must be given in the UN*X time domain!
439 *
440 * This is also a periodic extension, but since the cycle is 2^32 and
441 * the shift is 2^31, we can do some *very* fast math without explicit
442 * divisions.
443 *-------------------------------------------------------------------
444 */
445vint64
446ntpcal_ntp_to_ntp(
447	uint32_t      ntp,
448	const time_t *pivot
449	)
450{
451	vint64 res;
452
453#ifdef HAVE_INT64
454
455	res.q_s = (pivot)
456		      ? *pivot
457		      : now();
458	res.Q_s -= 0x80000000;		/* unshift of half range */
459	res.Q_s += (uint32_t)JAN_1970;	/* warp into NTP domain	 */
460	ntp	-= res.D_s.lo;		/* cycle difference	 */
461	res.Q_s += (uint64_t)ntp;	/* get expanded time	 */
462
463#else /* no 64bit scalars */
464
465	time_t tmp;
466
467	tmp = (pivot)
468		  ? *pivot
469		  : now();
470	res = time_to_vint64(&tmp);
471	M_SUB(res.D_s.hi, res.D_s.lo, 0, 0x80000000u);
472	M_ADD(res.D_s.hi, res.D_s.lo, 0, (uint32_t)JAN_1970);/*into NTP */
473	ntp -= res.D_s.lo;		/* cycle difference	 */
474	M_ADD(res.D_s.hi, res.D_s.lo, 0, ntp);
475
476#endif /* no 64bit scalars */
477
478	return res;
479}
480
481
482/*
483 * ==================================================================
484 *
485 * Splitting values to composite entities
486 *
487 * ==================================================================
488 */
489
490/*
491 *-------------------------------------------------------------------
492 * Split a 64bit seconds value into elapsed days in 'res.hi' and
493 * elapsed seconds since midnight in 'res.lo' using explicit floor
494 * division. This function happily accepts negative time values as
495 * timestamps before the respective epoch start.
496 * -------------------------------------------------------------------
497 */
498ntpcal_split
499ntpcal_daysplit(
500	const vint64 *ts
501	)
502{
503	ntpcal_split res;
504
505#ifdef HAVE_INT64
506
507	/* manual floor division by SECSPERDAY */
508	res.hi = (int32_t)(ts->q_s / SECSPERDAY);
509	res.lo = (int32_t)(ts->q_s % SECSPERDAY);
510	if (res.lo < 0) {
511		res.hi -= 1;
512		res.lo += SECSPERDAY;
513	}
514
515#else
516
517	/*
518	 * since we do not have 64bit ops, we have to this by hand.
519	 * Luckily SECSPERDAY is 86400 is 675*128, so we do the division
520	 * using chained 32/16 bit divisions and shifts.
521	 */
522	vint64	 op;
523	uint32_t q, r, a;
524	int	 isneg;
525
526	memcpy(&op, ts, sizeof(op));
527	/* fix sign */
528	isneg = M_ISNEG(op.D_s.hi);
529	if (isneg)
530		M_NEG(op.D_s.hi, op.D_s.lo);
531
532	/* save remainder of DIV 128, shift for divide */
533	r  = op.D_s.lo & 127; /* save remainder bits */
534	op.D_s.lo = (op.D_s.lo >> 7) | (op.D_s.hi << 25);
535	op.D_s.hi = (op.D_s.hi >> 7);
536
537	/* now do a mnual division, trying to remove as many ops as
538	 * possible -- division is always slow! An since we do not have
539	 * the advantage of a specific 64/32 bit or even a specific 32/16
540	 * bit division op, but must use the general 32/32bit division
541	 * even if we *know* the divider fits into unsigned 16 bits, the
542	 * exra code pathes should pay off.
543	 */
544	a = op.D_s.hi;
545	if (a > 675u)
546		a = a % 675u;
547	if (a) {
548		a = (a << 16) | op.W_s.lh;
549		q = a / 675u;
550		a = a % 675u;
551
552		a = (a << 16) | op.W_s.ll;
553		q = (q << 16) | (a / 675u);
554	} else {
555		a = op.D_s.lo;
556		q = a / 675u;
557	}
558	a = a % 675u;
559
560	/* assemble remainder */
561	r |= a << 7;
562
563	/* fix sign of result */
564	if (isneg) {
565		if (r) {
566			r = SECSPERDAY - r;
567			q = ~q;
568		} else
569			q = ~q + 1;
570	}
571
572	res.hi = q;
573	res.lo = r;
574
575#endif
576	return res;
577}
578
579/*
580 *-------------------------------------------------------------------
581 * Split a 32bit seconds value into h/m/s and excessive days.  This
582 * function happily accepts negative time values as timestamps before
583 * midnight.
584 * -------------------------------------------------------------------
585 */
586static int32_t
587priv_timesplit(
588	int32_t split[3],
589	int32_t ts
590	)
591{
592	int32_t days = 0;
593
594	/* make sure we have a positive offset into a day */
595	if (ts < 0 || ts >= SECSPERDAY) {
596		days = ts / SECSPERDAY;
597		ts   = ts % SECSPERDAY;
598		if (ts < 0) {
599			days -= 1;
600			ts   += SECSPERDAY;
601		}
602	}
603
604	/* get secs, mins, hours */
605	split[2] = (uint8_t)(ts % SECSPERMIN);
606	ts /= SECSPERMIN;
607	split[1] = (uint8_t)(ts % MINSPERHR);
608	split[0] = (uint8_t)(ts / MINSPERHR);
609
610	return days;
611}
612
613/*
614 * ---------------------------------------------------------------------
615 * Given the number of elapsed days in the calendar era, split this
616 * number into the number of elapsed years in 'res.hi' and the number
617 * of elapsed days of that year in 'res.lo'.
618 *
619 * if 'isleapyear' is not NULL, it will receive an integer that is 0 for
620 * regular years and a non-zero value for leap years.
621 *---------------------------------------------------------------------
622 */
623ntpcal_split
624ntpcal_split_eradays(
625	int32_t days,
626	int  *isleapyear
627	)
628{
629	ntpcal_split res;
630	int32_t	     n400, n100, n004, n001, yday; /* calendar year cycles */
631
632	/*
633	 * Split off calendar cycles, using floor division in the first
634	 * step. After that first step, simple division does it because
635	 * all operands are positive; alas, we have to be aware of the
636	 * possibe cycle overflows for 100 years and 1 year, caused by
637	 * the additional leap day.
638	 */
639	n400 = days / GREGORIAN_CYCLE_DAYS;
640	yday = days % GREGORIAN_CYCLE_DAYS;
641	if (yday < 0) {
642		n400 -= 1;
643		yday += GREGORIAN_CYCLE_DAYS;
644	}
645	n100 = yday / GREGORIAN_NORMAL_CENTURY_DAYS;
646	yday = yday % GREGORIAN_NORMAL_CENTURY_DAYS;
647	n004 = yday / GREGORIAN_NORMAL_LEAP_CYCLE_DAYS;
648	yday = yday % GREGORIAN_NORMAL_LEAP_CYCLE_DAYS;
649	n001 = yday / DAYSPERYEAR;
650	yday = yday % DAYSPERYEAR;
651
652	/*
653	 * check for leap cycle overflows and calculate the leap flag
654	 * if needed
655	 */
656	if ((n001 | n100) > 3) {
657		/* hit last day of leap year */
658		n001 -= 1;
659		yday += DAYSPERYEAR;
660		if (isleapyear)
661			*isleapyear = 1;
662	} else if (isleapyear)
663		*isleapyear = (n001 == 3) && ((n004 != 24) || (n100 == 3));
664
665	/* now merge the cycles to elapsed years, using horner scheme */
666	res.hi = ((4*n400 + n100)*25 + n004)*4 + n001;
667	res.lo = yday;
668
669	return res;
670}
671
672/*
673 *---------------------------------------------------------------------
674 * Given a number of elapsed days in a year and a leap year indicator,
675 * split the number of elapsed days into the number of elapsed months in
676 * 'res.hi' and the number of elapsed days of that month in 'res.lo'.
677 *
678 * This function will fail and return {-1,-1} if the number of elapsed
679 * days is not in the valid range!
680 *---------------------------------------------------------------------
681 */
682ntpcal_split
683ntpcal_split_yeardays(
684	int32_t eyd,
685	int     isleapyear
686	)
687{
688	ntpcal_split    res;
689	const uint16_t *lt;	/* month length table	*/
690
691	/* check leap year flag and select proper table */
692	lt = real_month_table[(isleapyear != 0)];
693	if (0 <= eyd && eyd < lt[12]) {
694		/* get zero-based month by approximation & correction step */
695		res.hi = eyd >> 5;	   /* approx month; might be 1 too low */
696		if (lt[res.hi + 1] <= eyd) /* fixup approximative month value  */
697			res.hi += 1;
698		res.lo = eyd - lt[res.hi];
699	} else {
700		res.lo = res.hi = -1;
701	}
702
703	return res;
704}
705
706/*
707 *---------------------------------------------------------------------
708 * Convert a RD into the date part of a 'struct calendar'.
709 *---------------------------------------------------------------------
710 */
711int
712ntpcal_rd_to_date(
713	struct calendar *jd,
714	int32_t		 rd
715	)
716{
717	ntpcal_split split;
718	int	     leaps;
719	int	     retv;
720
721	leaps = 0;
722	retv = 0;
723	/* get day-of-week first */
724	jd->weekday = rd % 7;
725	if (jd->weekday >= 7)	/* unsigned! */
726		jd->weekday += 7;
727
728	split = ntpcal_split_eradays(rd - 1, &leaps);
729	retv  = leaps;
730	/* get year and day-of-year */
731	jd->year = (uint16_t)split.hi + 1;
732	if (jd->year != split.hi + 1) {
733		jd->year = 0;
734		retv	 = -1;	/* bletch. overflow trouble. */
735	}
736	jd->yearday = (uint16_t)split.lo + 1;
737
738	/* convert to month and mday */
739	split = ntpcal_split_yeardays(split.lo, leaps);
740	jd->month    = (uint8_t)split.hi + 1;
741	jd->monthday = (uint8_t)split.lo + 1;
742
743	return retv ? retv : leaps;
744}
745
746/*
747 *---------------------------------------------------------------------
748 * Convert a RD into the date part of a 'struct tm'.
749 *---------------------------------------------------------------------
750 */
751int
752ntpcal_rd_to_tm(
753	struct tm  *utm,
754	int32_t	    rd
755	)
756{
757	ntpcal_split split;
758	int	     leaps;
759
760	leaps = 0;
761	/* get day-of-week first */
762	utm->tm_wday = rd % 7;
763	if (utm->tm_wday < 0)
764		utm->tm_wday += 7;
765
766	/* get year and day-of-year */
767	split = ntpcal_split_eradays(rd - 1, &leaps);
768	utm->tm_year = split.hi - 1899;
769	utm->tm_yday = split.lo;	/* 0-based */
770
771	/* convert to month and mday */
772	split = ntpcal_split_yeardays(split.lo, leaps);
773	utm->tm_mon  = split.hi;	/* 0-based */
774	utm->tm_mday = split.lo + 1;	/* 1-based */
775
776	return leaps;
777}
778
779/*
780 *---------------------------------------------------------------------
781 * Take a value of seconds since midnight and split it into hhmmss in a
782 * 'struct calendar'.
783 *---------------------------------------------------------------------
784 */
785int32_t
786ntpcal_daysec_to_date(
787	struct calendar *jd,
788	int32_t		sec
789	)
790{
791	int32_t days;
792	int   ts[3];
793
794	days = priv_timesplit(ts, sec);
795	jd->hour   = (uint8_t)ts[0];
796	jd->minute = (uint8_t)ts[1];
797	jd->second = (uint8_t)ts[2];
798
799	return days;
800}
801
802/*
803 *---------------------------------------------------------------------
804 * Take a value of seconds since midnight and split it into hhmmss in a
805 * 'struct tm'.
806 *---------------------------------------------------------------------
807 */
808int32_t
809ntpcal_daysec_to_tm(
810	struct tm *utm,
811	int32_t	   sec
812	)
813{
814	int32_t days;
815	int32_t ts[3];
816
817	days = priv_timesplit(ts, sec);
818	utm->tm_hour = ts[0];
819	utm->tm_min  = ts[1];
820	utm->tm_sec  = ts[2];
821
822	return days;
823}
824
825/*
826 *---------------------------------------------------------------------
827 * take a split representation for day/second-of-day and day offset
828 * and convert it to a 'struct calendar'. The seconds will be normalised
829 * into the range of a day, and the day will be adjusted accordingly.
830 *
831 * returns >0 if the result is in a leap year, 0 if in a regular
832 * year and <0 if the result did not fit into the calendar struct.
833 *---------------------------------------------------------------------
834 */
835int
836ntpcal_daysplit_to_date(
837	struct calendar	   *jd,
838	const ntpcal_split *ds,
839	int32_t		    dof
840	)
841{
842	dof += ntpcal_daysec_to_date(jd, ds->lo);
843	return ntpcal_rd_to_date(jd, ds->hi + dof);
844}
845
846/*
847 *---------------------------------------------------------------------
848 * take a split representation for day/second-of-day and day offset
849 * and convert it to a 'struct tm'. The seconds will be normalised
850 * into the range of a day, and the day will be adjusted accordingly.
851 *
852 * returns 1 if the result is in a leap year and zero if in a regular
853 * year.
854 *---------------------------------------------------------------------
855 */
856int
857ntpcal_daysplit_to_tm(
858	struct tm	   *utm,
859	const ntpcal_split *ds ,
860	int32_t		    dof
861	)
862{
863	dof += ntpcal_daysec_to_tm(utm, ds->lo);
864
865	return ntpcal_rd_to_tm(utm, ds->hi + dof);
866}
867
868/*
869 *---------------------------------------------------------------------
870 * Take a UN*X time and convert to a calendar structure.
871 *---------------------------------------------------------------------
872 */
873int
874ntpcal_time_to_date(
875	struct calendar	*jd,
876	const vint64	*ts
877	)
878{
879	ntpcal_split ds;
880
881	ds = ntpcal_daysplit(ts);
882	ds.hi += ntpcal_daysec_to_date(jd, ds.lo);
883	ds.hi += DAY_UNIX_STARTS;
884
885	return ntpcal_rd_to_date(jd, ds.hi);
886}
887
888
889/*
890 * ==================================================================
891 *
892 * merging composite entities
893 *
894 * ==================================================================
895 */
896
897/*
898 *---------------------------------------------------------------------
899 * Merge a number of days and a number of seconds into seconds,
900 * expressed in 64 bits to avoid overflow.
901 *---------------------------------------------------------------------
902 */
903vint64
904ntpcal_dayjoin(
905	int32_t days,
906	int32_t secs
907	)
908{
909	vint64 res;
910
911#ifdef HAVE_INT64
912
913	res.q_s	 = days;
914	res.q_s *= SECSPERDAY;
915	res.q_s += secs;
916
917#else
918
919	uint32_t p1, p2;
920	int	 isneg;
921
922	/*
923	 * res = days *86400 + secs, using manual 16/32 bit
924	 * multiplications and shifts.
925	 */
926	isneg = (days < 0);
927	if (isneg)
928		days = -days;
929
930	/* assemble days * 675 */
931	res.D_s.lo = (days & 0xFFFF) * 675u;
932	res.D_s.hi = 0;
933	p1 = (days >> 16) * 675u;
934	p2 = p1 >> 16;
935	p1 = p1 << 16;
936	M_ADD(res.D_s.hi, res.D_s.lo, p2, p1);
937
938	/* mul by 128, using shift */
939	res.D_s.hi = (res.D_s.hi << 7) | (res.D_s.lo >> 25);
940	res.D_s.lo = (res.D_s.lo << 7);
941
942	/* fix sign */
943	if (isneg)
944		M_NEG(res.D_s.hi, res.D_s.lo);
945
946	/* properly add seconds */
947	p2 = 0;
948	if (secs < 0) {
949		p1 = (uint32_t)-secs;
950		M_NEG(p2, p1);
951	} else {
952		p1 = (uint32_t)secs;
953	}
954	M_ADD(res.D_s.hi, res.D_s.lo, p2, p1);
955
956#endif
957
958	return res;
959}
960
961/*
962 *---------------------------------------------------------------------
963 * Convert elapsed years in Era into elapsed days in Era.
964 *
965 * To accomodate for negative values of years, floor division would be
966 * required for all division operations. This can be eased by first
967 * splitting the years into full 400-year cycles and years in the
968 * cycle. Only this operation must be coded as a full floor division; as
969 * the years in the cycle is a non-negative number, all other divisions
970 * can be regular truncated divisions.
971 *---------------------------------------------------------------------
972 */
973int32_t
974ntpcal_days_in_years(
975	int32_t years
976	)
977{
978	int32_t cycle; /* full gregorian cycle */
979
980	/* split off full calendar cycles, using floor division */
981	cycle = years / 400;
982	years = years % 400;
983	if (years < 0) {
984		cycle -= 1;
985		years += 400;
986	}
987
988	/*
989	 * Calculate days in cycle. years now is a non-negative number,
990	 * holding the number of years in the 400-year cycle.
991	 */
992	return cycle * GREGORIAN_CYCLE_DAYS
993	     + years * DAYSPERYEAR	/* days inregular years	*/
994	     + years / 4		/* 4 year leap rule	*/
995	     - years / 100;		/* 100 year leap rule	*/
996	/* the 400-year rule does not apply due to full-cycle split-off */
997}
998
999/*
1000 *---------------------------------------------------------------------
1001 * Convert a number of elapsed month in a year into elapsed days in year.
1002 *
1003 * The month will be normalized, and 'res.hi' will contain the
1004 * excessive years that must be considered when converting the years,
1005 * while 'res.lo' will contain the number of elapsed days since start
1006 * of the year.
1007 *
1008 * This code uses the shifted-month-approach to convert month to days,
1009 * because then there is no need to have explicit leap year
1010 * information.	 The slight disadvantage is that for most month values
1011 * the result is a negative value, and the year excess is one; the
1012 * conversion is then simply based on the start of the following year.
1013 *---------------------------------------------------------------------
1014 */
1015ntpcal_split
1016ntpcal_days_in_months(
1017	int32_t m
1018	)
1019{
1020	ntpcal_split res;
1021
1022	/* normalize month into range */
1023	res.hi = 0;
1024	res.lo = m;
1025	if (res.lo < 0 || res.lo >= 12) {
1026		res.hi = res.lo / 12;
1027		res.lo = res.lo % 12;
1028		if (res.lo < 0) {
1029			res.hi -= 1;
1030			res.lo += 12;
1031		}
1032	}
1033
1034	/* add 10 month for year starting with march */
1035	if (res.lo < 2)
1036		res.lo += 10;
1037	else {
1038		res.hi += 1;
1039		res.lo -= 2;
1040	}
1041
1042	/* get cummulated days in year with unshift */
1043	res.lo = shift_month_table[res.lo] - 306;
1044
1045	return res;
1046}
1047
1048/*
1049 *---------------------------------------------------------------------
1050 * Convert ELAPSED years/months/days of gregorian calendar to elapsed
1051 * days in Gregorian epoch.
1052 *
1053 * If you want to convert years and days-of-year, just give a month of
1054 * zero.
1055 *---------------------------------------------------------------------
1056 */
1057int32_t
1058ntpcal_edate_to_eradays(
1059	int32_t years,
1060	int32_t mons,
1061	int32_t mdays
1062	)
1063{
1064	ntpcal_split tmp;
1065	int32_t	     res;
1066
1067	if (mons) {
1068		tmp = ntpcal_days_in_months(mons);
1069		res = ntpcal_days_in_years(years + tmp.hi) + tmp.lo;
1070	} else
1071		res = ntpcal_days_in_years(years);
1072	res += mdays;
1073
1074	return res;
1075}
1076
1077/*
1078 *---------------------------------------------------------------------
1079 * Convert ELAPSED years/months/days of gregorian calendar to elapsed
1080 * days in year.
1081 *
1082 * Note: This will give the true difference to the start of the given year,
1083 * even if months & days are off-scale.
1084 *---------------------------------------------------------------------
1085 */
1086int32_t
1087ntpcal_edate_to_yeardays(
1088	int32_t years,
1089	int32_t mons,
1090	int32_t mdays
1091	)
1092{
1093	ntpcal_split tmp;
1094
1095	if (0 <= mons && mons < 12) {
1096		years += 1;
1097		mdays += real_month_table[is_leapyear(years)][mons];
1098	} else {
1099		tmp = ntpcal_days_in_months(mons);
1100		mdays += tmp.lo
1101		       + ntpcal_days_in_years(years + tmp.hi)
1102		       - ntpcal_days_in_years(years);
1103	}
1104
1105	return mdays;
1106}
1107
1108/*
1109 *---------------------------------------------------------------------
1110 * Convert elapsed days and the hour/minute/second information into
1111 * total seconds.
1112 *
1113 * If 'isvalid' is not NULL, do a range check on the time specification
1114 * and tell if the time input is in the normal range, permitting for a
1115 * single leapsecond.
1116 *---------------------------------------------------------------------
1117 */
1118int32_t
1119ntpcal_etime_to_seconds(
1120	int32_t hours,
1121	int32_t minutes,
1122	int32_t seconds
1123	)
1124{
1125	int32_t res;
1126
1127	res = (hours * MINSPERHR + minutes) * SECSPERMIN + seconds;
1128
1129	return res;
1130}
1131
1132/*
1133 *---------------------------------------------------------------------
1134 * Convert the date part of a 'struct tm' (that is, year, month,
1135 * day-of-month) into the RD of that day.
1136 *---------------------------------------------------------------------
1137 */
1138int32_t
1139ntpcal_tm_to_rd(
1140	const struct tm *utm
1141	)
1142{
1143	return ntpcal_edate_to_eradays(utm->tm_year + 1899,
1144				       utm->tm_mon,
1145				       utm->tm_mday - 1) + 1;
1146}
1147
1148/*
1149 *---------------------------------------------------------------------
1150 * Convert the date part of a 'struct calendar' (that is, year, month,
1151 * day-of-month) into the RD of that day.
1152 *---------------------------------------------------------------------
1153 */
1154int32_t
1155ntpcal_date_to_rd(
1156	const struct calendar *jd
1157	)
1158{
1159	return ntpcal_edate_to_eradays((int32_t)jd->year - 1,
1160				       (int32_t)jd->month - 1,
1161				       (int32_t)jd->monthday - 1) + 1;
1162}
1163
1164/*
1165 *---------------------------------------------------------------------
1166 * convert a year number to rata die of year start
1167 *---------------------------------------------------------------------
1168 */
1169int32_t
1170ntpcal_year_to_ystart(
1171	int32_t year
1172	)
1173{
1174	return ntpcal_days_in_years(year - 1) + 1;
1175}
1176
1177/*
1178 *---------------------------------------------------------------------
1179 * For a given RD, get the RD of the associated year start,
1180 * that is, the RD of the last January,1st on or before that day.
1181 *---------------------------------------------------------------------
1182 */
1183int32_t
1184ntpcal_rd_to_ystart(
1185	int32_t rd
1186	)
1187{
1188	/*
1189	 * Rather simple exercise: split the day number into elapsed
1190	 * years and elapsed days, then remove the elapsed days from the
1191	 * input value. Nice'n sweet...
1192	 */
1193	return rd - ntpcal_split_eradays(rd - 1, NULL).lo;
1194}
1195
1196/*
1197 *---------------------------------------------------------------------
1198 * For a given RD, get the RD of the associated month start.
1199 *---------------------------------------------------------------------
1200 */
1201int32_t
1202ntpcal_rd_to_mstart(
1203	int32_t rd
1204	)
1205{
1206	ntpcal_split split;
1207	int	     leaps;
1208
1209	split = ntpcal_split_eradays(rd - 1, &leaps);
1210	split = ntpcal_split_yeardays(split.lo, leaps);
1211
1212	return rd - split.lo;
1213}
1214
1215/*
1216 *---------------------------------------------------------------------
1217 * take a 'struct calendar' and get the seconds-of-day from it.
1218 *---------------------------------------------------------------------
1219 */
1220int32_t
1221ntpcal_date_to_daysec(
1222	const struct calendar *jd
1223	)
1224{
1225	return ntpcal_etime_to_seconds(jd->hour, jd->minute,
1226				       jd->second);
1227}
1228
1229/*
1230 *---------------------------------------------------------------------
1231 * take a 'struct tm' and get the seconds-of-day from it.
1232 *---------------------------------------------------------------------
1233 */
1234int32_t
1235ntpcal_tm_to_daysec(
1236	const struct tm *utm
1237	)
1238{
1239	return ntpcal_etime_to_seconds(utm->tm_hour, utm->tm_min,
1240				       utm->tm_sec);
1241}
1242
1243/*
1244 *---------------------------------------------------------------------
1245 * take a 'struct calendar' and convert it to a 'time_t'
1246 *---------------------------------------------------------------------
1247 */
1248time_t
1249ntpcal_date_to_time(
1250	const struct calendar *jd
1251	)
1252{
1253	vint64  join;
1254	int32_t days, secs;
1255
1256	days = ntpcal_date_to_rd(jd) - DAY_UNIX_STARTS;
1257	secs = ntpcal_date_to_daysec(jd);
1258	join = ntpcal_dayjoin(days, secs);
1259
1260	return vint64_to_time(&join);
1261}
1262
1263
1264/*
1265 * ==================================================================
1266 *
1267 * extended and unchecked variants of caljulian/caltontp
1268 *
1269 * ==================================================================
1270 */
1271int
1272ntpcal_ntp64_to_date(
1273	struct calendar *jd,
1274	const vint64    *ntp
1275	)
1276{
1277	ntpcal_split ds;
1278
1279	ds = ntpcal_daysplit(ntp);
1280	ds.hi += ntpcal_daysec_to_date(jd, ds.lo);
1281
1282	return ntpcal_rd_to_date(jd, ds.hi + DAY_NTP_STARTS);
1283}
1284
1285int
1286ntpcal_ntp_to_date(
1287	struct calendar *jd,
1288	uint32_t	 ntp,
1289	const time_t	*piv
1290	)
1291{
1292	vint64	ntp64;
1293
1294	/*
1295	 * Unfold ntp time around current time into NTP domain. Split
1296	 * into days and seconds, shift days into CE domain and
1297	 * process the parts.
1298	 */
1299	ntp64 = ntpcal_ntp_to_ntp(ntp, piv);
1300	return ntpcal_ntp64_to_date(jd, &ntp64);
1301}
1302
1303
1304vint64
1305ntpcal_date_to_ntp64(
1306	const struct calendar *jd
1307	)
1308{
1309	/*
1310	 * Convert date to NTP. Ignore yearday, use d/m/y only.
1311	 */
1312	return ntpcal_dayjoin(ntpcal_date_to_rd(jd) - DAY_NTP_STARTS,
1313			      ntpcal_date_to_daysec(jd));
1314}
1315
1316
1317uint32_t
1318ntpcal_date_to_ntp(
1319	const struct calendar *jd
1320	)
1321{
1322	/*
1323	 * Get lower half of 64-bit NTP timestamp from date/time.
1324	 */
1325	return ntpcal_date_to_ntp64(jd).d_s.lo;
1326}
1327
1328
1329
1330/*
1331 * ==================================================================
1332 *
1333 * day-of-week calculations
1334 *
1335 * ==================================================================
1336 */
1337/*
1338 * Given a RataDie and a day-of-week, calculate a RDN that is reater-than,
1339 * greater-or equal, closest, less-or-equal or less-than the given RDN
1340 * and denotes the given day-of-week
1341 */
1342int32_t
1343ntpcal_weekday_gt(
1344	int32_t rdn,
1345	int32_t dow
1346	)
1347{
1348	return ntpcal_periodic_extend(rdn+1, dow, 7);
1349}
1350
1351int32_t
1352ntpcal_weekday_ge(
1353	int32_t rdn,
1354	int32_t dow
1355	)
1356{
1357	return ntpcal_periodic_extend(rdn, dow, 7);
1358}
1359
1360int32_t
1361ntpcal_weekday_close(
1362	int32_t rdn,
1363	int32_t dow
1364	)
1365{
1366	return ntpcal_periodic_extend(rdn-3, dow, 7);
1367}
1368
1369int32_t
1370ntpcal_weekday_le(
1371	int32_t rdn,
1372	int32_t dow
1373	)
1374{
1375	return ntpcal_periodic_extend(rdn, dow, -7);
1376}
1377
1378int32_t
1379ntpcal_weekday_lt(
1380	int32_t rdn,
1381	int32_t dow
1382	)
1383{
1384	return ntpcal_periodic_extend(rdn-1, dow, -7);
1385}
1386
1387/*
1388 * ==================================================================
1389 *
1390 * ISO week-calendar conversions
1391 *
1392 * The ISO8601 calendar defines a calendar of years, weeks and weekdays.
1393 * It is related to the Gregorian calendar, and a ISO year starts at the
1394 * Monday closest to Jan,1st of the corresponding Gregorian year.  A ISO
1395 * calendar year has always 52 or 53 weeks, and like the Grogrian
1396 * calendar the ISO8601 calendar repeats itself every 400 years, or
1397 * 146097 days, or 20871 weeks.
1398 *
1399 * While it is possible to write ISO calendar functions based on the
1400 * Gregorian calendar functions, the following implementation takes a
1401 * different approach, based directly on years and weeks.
1402 *
1403 * Analysis of the tabulated data shows that it is not possible to
1404 * interpolate from years to weeks over a full 400 year range; cyclic
1405 * shifts over 400 years do not provide a solution here. But it *is*
1406 * possible to interpolate over every single century of the 400-year
1407 * cycle. (The centennial leap year rule seems to be the culprit here.)
1408 *
1409 * It can be shown that a conversion from years to weeks can be done
1410 * using a linear transformation of the form
1411 *
1412 *   w = floor( y * a + b )
1413 *
1414 * where the slope a must hold to
1415 *
1416 *  52.1780821918 <= a < 52.1791044776
1417 *
1418 * and b must be chosen according to the selected slope and the number
1419 * of the century in a 400-year period.
1420 *
1421 * The inverse calculation can also be done in this way. Careful scaling
1422 * provides an unlimited set of integer coefficients a,k,b that enable
1423 * us to write the calulation in the form
1424 *
1425 *   w = (y * a	 + b ) / k
1426 *   y = (w * a' + b') / k'
1427 *
1428 * In this implementation the values of k and k' are chosen to be
1429 * smallest possible powers of two, so the division can be implemented
1430 * as shifts if the optimiser chooses to do so.
1431 *
1432 * ==================================================================
1433 */
1434
1435/*
1436 * Given a number of elapsed (ISO-)years since the begin of the
1437 * christian era, return the number of elapsed weeks corresponding to
1438 * the number of years.
1439 */
1440int32_t
1441isocal_weeks_in_years(
1442	int32_t years
1443	)
1444{
1445	/*
1446	 * use: w = (y * 53431 + b[c]) / 1024 as interpolation
1447	 */
1448	static const int32_t bctab[4] = { 449, 157, 889, 597 };
1449	int32_t cycle; /* full gregorian cycle */
1450	int32_t cents; /* full centuries	   */
1451	int32_t weeks; /* accumulated weeks	   */
1452
1453	/* split off full calendar cycles, using floor division */
1454	cycle = years / 400;
1455	years = years % 400;
1456	if (years < 0) {
1457		cycle -= 1;
1458		years += 400;
1459	}
1460
1461	/* split off full centuries */
1462	cents = years / 100;
1463	years = years % 100;
1464
1465	/*
1466	 * calculate elapsed weeks, taking into account that the
1467	 * first, third and fourth century have 5218 weeks but the
1468	 * second century falls short by one week.
1469	 */
1470	weeks = (years * 53431 + bctab[cents]) / 1024;
1471
1472	return cycle * GREGORIAN_CYCLE_WEEKS
1473	     + cents * 5218 - (cents > 1)
1474	     + weeks;
1475}
1476
1477/*
1478 * Given a number of elapsed weeks since the begin of the christian
1479 * era, split this number into the number of elapsed years in res.hi
1480 * and the excessive number of weeks in res.lo. (That is, res.lo is
1481 * the number of elapsed weeks in the remaining partial year.)
1482 */
1483ntpcal_split
1484isocal_split_eraweeks(
1485	int32_t weeks
1486	)
1487{
1488	/*
1489	 * use: y = (w * 157 + b[c]) / 8192 as interpolation
1490	 */
1491	static const int32_t bctab[4] = { 85, 131, 17, 62 };
1492	ntpcal_split res;
1493	int32_t	     cents;
1494
1495	/*
1496	 * split off 400-year cycles, using the fact that a 400-year
1497	 * cycle has 146097 days, which is exactly 20871 weeks.
1498	 */
1499	res.hi = weeks / GREGORIAN_CYCLE_WEEKS;
1500	res.lo = weeks % GREGORIAN_CYCLE_WEEKS;
1501	if (res.lo < 0) {
1502		res.hi -= 1;
1503		res.lo += GREGORIAN_CYCLE_WEEKS;
1504	}
1505	res.hi *= 400;
1506
1507	/*
1508	 * split off centuries, taking into account that the first,
1509	 * third and fourth century have 5218 weeks but that the
1510	 * second century falls short by one week.
1511	 */
1512	res.lo += (res.lo >= 10435);
1513	cents	= res.lo / 5218;
1514	res.lo %= 5218;		/* res.lo is weeks in century now */
1515
1516	/* convert elapsed weeks in century to elapsed years and weeks */
1517	res.lo	= res.lo * 157 + bctab[cents];
1518	res.hi += cents * 100 + res.lo / 8192;
1519	res.lo	= (res.lo % 8192) / 157;
1520
1521	return res;
1522}
1523
1524/*
1525 * Given a second in the NTP time scale and a pivot, expand the NTP
1526 * time stamp around the pivot and convert into an ISO calendar time
1527 * stamp.
1528 */
1529int
1530isocal_ntp64_to_date(
1531	struct isodate *id,
1532	const vint64   *ntp
1533	)
1534{
1535	ntpcal_split ds;
1536	int32_t      ts[3];
1537
1538	/*
1539	 * Split NTP time into days and seconds, shift days into CE
1540	 * domain and process the parts.
1541	 */
1542	ds = ntpcal_daysplit(ntp);
1543
1544	/* split time part */
1545	ds.hi += priv_timesplit(ts, ds.lo);
1546	id->hour   = (uint8_t)ts[0];
1547	id->minute = (uint8_t)ts[1];
1548	id->second = (uint8_t)ts[2];
1549
1550	/* split date part */
1551	ds.lo = ds.hi + DAY_NTP_STARTS - 1;	/* elapsed era days  */
1552	ds.hi = ds.lo / 7;			/* elapsed era weeks */
1553	ds.lo = ds.lo % 7;			/* elapsed week days */
1554	if (ds.lo < 0) {			/* floor division!   */
1555		ds.hi -= 1;
1556		ds.lo += 7;
1557	}
1558	id->weekday = (uint8_t)ds.lo + 1;	/* weekday result    */
1559
1560	ds = isocal_split_eraweeks(ds.hi);	/* elapsed years&week*/
1561	id->year = (uint16_t)ds.hi + 1;		/* shift to current  */
1562	id->week = (uint8_t )ds.lo + 1;
1563
1564	return (ds.hi >= 0 && ds.hi < 0xFFFFU);
1565}
1566
1567int
1568isocal_ntp_to_date(
1569	struct isodate *id,
1570	uint32_t	ntp,
1571	const time_t   *piv
1572	)
1573{
1574	vint64	ntp64;
1575
1576	/*
1577	 * Unfold ntp time around current time into NTP domain, then
1578	 * convert the full time stamp.
1579	 */
1580	ntp64 = ntpcal_ntp_to_ntp(ntp, piv);
1581	return isocal_ntp64_to_date(id, &ntp64);
1582}
1583
1584/*
1585 * Convert a ISO date spec into a second in the NTP time scale,
1586 * properly truncated to 32 bit.
1587 */
1588vint64
1589isocal_date_to_ntp64(
1590	const struct isodate *id
1591	)
1592{
1593	int32_t weeks, days, secs;
1594
1595	weeks = isocal_weeks_in_years((int32_t)id->year - 1)
1596	      + (int32_t)id->week - 1;
1597	days = weeks * 7 + (int32_t)id->weekday;
1598	/* days is RDN of ISO date now */
1599	secs = ntpcal_etime_to_seconds(id->hour, id->minute, id->second);
1600
1601	return ntpcal_dayjoin(days - DAY_NTP_STARTS, secs);
1602}
1603
1604uint32_t
1605isocal_date_to_ntp(
1606	const struct isodate *id
1607	)
1608{
1609	/*
1610	 * Get lower half of 64-bit NTP timestamp from date/time.
1611	 */
1612	return isocal_date_to_ntp64(id).d_s.lo;
1613}
1614
1615/* -*-EOF-*- */
1616