xref: /freebsd/contrib/ntp/libntp/ntp_calendar.c (revision 7263c8c0998402e9860a0865013fbec4ece98cd4)
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 
22 static systime_func_ptr systime_func = &time;
23 static inline time_t now(void);
24 
25 
26 systime_func_ptr
27 ntpcal_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 
42 static inline time_t
43 now(void)
44 {
45 	return (*systime_func)(NULL);
46 }
47 
48 /*
49  *---------------------------------------------------------------------
50  * Convert between 'time_t' and 'vint64'
51  *---------------------------------------------------------------------
52  */
53 vint64
54 time_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 
99 time_t
100 vint64_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  */
128 int
129 ntpcal_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 #ifdef MKREPRO_DATE
157 	static const char build[] = MKREPRO_TIME "/" MKREPRO_DATE;
158 #else
159 	static const char build[] = __TIME__ "/" __DATE__;
160 #endif
161 	static const char mlist[] = "JanFebMarAprMayJunJulAugSepOctNovDec";
162 
163 	char		  monstr[4];
164 	const char *	  cp;
165 	unsigned short	  hour, minute, second, day, year;
166  	/* Note: The above quantities are used for sscanf 'hu' format,
167 	 * so using 'uint16_t' is contra-indicated!
168 	 */
169 
170 #ifdef DEBUG
171 	static int        ignore  = 0;
172 #endif
173 
174 	ZERO(*jd);
175 	jd->year     = 1970;
176 	jd->month    = 1;
177 	jd->monthday = 1;
178 
179 #ifdef DEBUG
180 	/* check environment if build date should be ignored */
181 	if (0 == ignore) {
182 	    const char * envstr;
183 	    envstr = getenv("NTPD_IGNORE_BUILD_DATE");
184 	    ignore = 1 + (envstr && (!*envstr || !strcasecmp(envstr, "yes")));
185 	}
186 	if (ignore > 1)
187 	    return FALSE;
188 #endif
189 
190 	if (6 == sscanf(build, "%hu:%hu:%hu/%3s %hu %hu",
191 			&hour, &minute, &second, monstr, &day, &year)) {
192 		cp = strstr(mlist, monstr);
193 		if (NULL != cp) {
194 			jd->year     = year;
195 			jd->month    = (uint8_t)((cp - mlist) / 3 + 1);
196 			jd->monthday = (uint8_t)day;
197 			jd->hour     = (uint8_t)hour;
198 			jd->minute   = (uint8_t)minute;
199 			jd->second   = (uint8_t)second;
200 
201 			return TRUE;
202 		}
203 	}
204 
205 	return FALSE;
206 }
207 
208 
209 /*
210  *---------------------------------------------------------------------
211  * basic calendar stuff
212  * --------------------------------------------------------------------
213  */
214 
215 /* month table for a year starting with March,1st */
216 static const uint16_t shift_month_table[13] = {
217 	0, 31, 61, 92, 122, 153, 184, 214, 245, 275, 306, 337, 366
218 };
219 
220 /* month tables for years starting with January,1st; regular & leap */
221 static const uint16_t real_month_table[2][13] = {
222 	/* -*- table for regular years -*- */
223 	{ 0, 31, 59, 90, 120, 151, 181, 212, 243, 273, 304, 334, 365 },
224 	/* -*- table for leap years -*- */
225 	{ 0, 31, 60, 91, 121, 152, 182, 213, 244, 274, 305, 335, 366 }
226 };
227 
228 /*
229  * Some notes on the terminology:
230  *
231  * We use the proleptic Gregorian calendar, which is the Gregorian
232  * calendar extended in both directions ad infinitum. This totally
233  * disregards the fact that this calendar was invented in 1582, and
234  * was adopted at various dates over the world; sometimes even after
235  * the start of the NTP epoch.
236  *
237  * Normally date parts are given as current cycles, while time parts
238  * are given as elapsed cycles:
239  *
240  * 1970-01-01/03:04:05 means 'IN the 1970st. year, IN the first month,
241  * ON the first day, with 3hrs, 4minutes and 5 seconds elapsed.
242  *
243  * The basic calculations for this calendar implementation deal with
244  * ELAPSED date units, which is the number of full years, full months
245  * and full days before a date: 1970-01-01 would be (1969, 0, 0) in
246  * that notation.
247  *
248  * To ease the numeric computations, month and day values outside the
249  * normal range are acceptable: 2001-03-00 will be treated as the day
250  * before 2001-03-01, 2000-13-32 will give the same result as
251  * 2001-02-01 and so on.
252  *
253  * 'rd' or 'RD' is used as an abbreviation for the latin 'rata die'
254  * (day number).  This is the number of days elapsed since 0000-12-31
255  * in the proleptic Gregorian calendar. The begin of the Christian Era
256  * (0001-01-01) is RD(1).
257  *
258  *
259  * Some notes on the implementation:
260  *
261  * Calendar algorithms thrive on the division operation, which is one of
262  * the slowest numerical operations in any CPU. What saves us here from
263  * abysmal performance is the fact that all divisions are divisions by
264  * constant numbers, and most compilers can do this by a multiplication
265  * operation.  But this might not work when using the div/ldiv/lldiv
266  * function family, because many compilers are not able to do inline
267  * expansion of the code with following optimisation for the
268  * constant-divider case.
269  *
270  * Also div/ldiv/lldiv are defined in terms of int/long/longlong, which
271  * are inherently target dependent. Nothing that could not be cured with
272  * autoconf, but still a mess...
273  *
274  * Furthermore, we need floor division while C demands truncation to
275  * zero, so additional steps are required to make sure the algorithms
276  * work.
277  *
278  * For all this, all divisions by constant are coded manually, even when
279  * there is a joined div/mod operation: The optimiser should sort that
280  * out, if possible.
281  *
282  * Finally, the functions do not check for overflow conditions. This
283  * is a sacrifice made for execution speed; since a 32-bit day counter
284  * covers +/- 5,879,610 years, this should not pose a problem here.
285  */
286 
287 
288 /*
289  * ==================================================================
290  *
291  * General algorithmic stuff
292  *
293  * ==================================================================
294  */
295 
296 /*
297  *---------------------------------------------------------------------
298  * Do a periodic extension of 'value' around 'pivot' with a period of
299  * 'cycle'.
300  *
301  * The result 'res' is a number that holds to the following properties:
302  *
303  *   1)	 res MOD cycle == value MOD cycle
304  *   2)	 pivot <= res < pivot + cycle
305  *	 (replace </<= with >/>= for negative cycles)
306  *
307  * where 'MOD' denotes the modulo operator for FLOOR DIVISION, which
308  * is not the same as the '%' operator in C: C requires division to be
309  * a truncated division, where remainder and dividend have the same
310  * sign if the remainder is not zero, whereas floor division requires
311  * divider and modulus to have the same sign for a non-zero modulus.
312  *
313  * This function has some useful applications:
314  *
315  * + let Y be a calendar year and V a truncated 2-digit year: then
316  *	periodic_extend(Y-50, V, 100)
317  *   is the closest expansion of the truncated year with respect to
318  *   the full year, that is a 4-digit year with a difference of less
319  *   than 50 years to the year Y. ("century unfolding")
320  *
321  * + let T be a UN*X time stamp and V be seconds-of-day: then
322  *	perodic_extend(T-43200, V, 86400)
323  *   is a time stamp that has the same seconds-of-day as the input
324  *   value, with an absolute difference to T of <= 12hrs.  ("day
325  *   unfolding")
326  *
327  * + Wherever you have a truncated periodic value and a non-truncated
328  *   base value and you want to match them somehow...
329  *
330  * Basically, the function delivers 'pivot + (value - pivot) % cycle',
331  * but the implementation takes some pains to avoid internal signed
332  * integer overflows in the '(value - pivot) % cycle' part and adheres
333  * to the floor division convention.
334  *
335  * If 64bit scalars where available on all intended platforms, writing a
336  * version that uses 64 bit ops would be easy; writing a general
337  * division routine for 64bit ops on a platform that can only do
338  * 32/16bit divisions and is still performant is a bit more
339  * difficult. Since most usecases can be coded in a way that does only
340  * require the 32-bit version a 64bit version is NOT provided here.
341  * ---------------------------------------------------------------------
342  */
343 int32_t
344 ntpcal_periodic_extend(
345 	int32_t pivot,
346 	int32_t value,
347 	int32_t cycle
348 	)
349 {
350 	uint32_t diff;
351 	char	 cpl = 0; /* modulo complement flag */
352 	char	 neg = 0; /* sign change flag	    */
353 
354 	/* make the cycle positive and adjust the flags */
355 	if (cycle < 0) {
356 		cycle = - cycle;
357 		neg ^= 1;
358 		cpl ^= 1;
359 	}
360 	/* guard against div by zero or one */
361 	if (cycle > 1) {
362 		/*
363 		 * Get absolute difference as unsigned quantity and
364 		 * the complement flag. This is done by always
365 		 * subtracting the smaller value from the bigger
366 		 * one. This implementation works only on a two's
367 		 * complement machine!
368 		 */
369 		if (value >= pivot) {
370 			diff = (uint32_t)value - (uint32_t)pivot;
371 		} else {
372 			diff = (uint32_t)pivot - (uint32_t)value;
373 			cpl ^= 1;
374 		}
375 		diff %= (uint32_t)cycle;
376 		if (diff) {
377 			if (cpl)
378 				diff = cycle - diff;
379 			if (neg)
380 				diff = ~diff + 1;
381 			pivot += diff;
382 		}
383 	}
384 	return pivot;
385 }
386 
387 /*
388  *-------------------------------------------------------------------
389  * Convert a timestamp in NTP scale to a 64bit seconds value in the UN*X
390  * scale with proper epoch unfolding around a given pivot or the current
391  * system time. This function happily accepts negative pivot values as
392  * timestamps befor 1970-01-01, so be aware of possible trouble on
393  * platforms with 32bit 'time_t'!
394  *
395  * This is also a periodic extension, but since the cycle is 2^32 and
396  * the shift is 2^31, we can do some *very* fast math without explicit
397  * divisions.
398  *-------------------------------------------------------------------
399  */
400 vint64
401 ntpcal_ntp_to_time(
402 	uint32_t	ntp,
403 	const time_t *	pivot
404 	)
405 {
406 	vint64 res;
407 
408 #ifdef HAVE_INT64
409 
410 	res.q_s = (pivot != NULL)
411 		      ? *pivot
412 		      : now();
413 	res.Q_s -= 0x80000000;		/* unshift of half range */
414 	ntp	-= (uint32_t)JAN_1970;	/* warp into UN*X domain */
415 	ntp	-= res.D_s.lo;		/* cycle difference	 */
416 	res.Q_s += (uint64_t)ntp;	/* get expanded time	 */
417 
418 #else /* no 64bit scalars */
419 
420 	time_t tmp;
421 
422 	tmp = (pivot != NULL)
423 		  ? *pivot
424 		  : now();
425 	res = time_to_vint64(&tmp);
426 	M_SUB(res.D_s.hi, res.D_s.lo, 0, 0x80000000);
427 	ntp -= (uint32_t)JAN_1970;	/* warp into UN*X domain */
428 	ntp -= res.D_s.lo;		/* cycle difference	 */
429 	M_ADD(res.D_s.hi, res.D_s.lo, 0, ntp);
430 
431 #endif /* no 64bit scalars */
432 
433 	return res;
434 }
435 
436 /*
437  *-------------------------------------------------------------------
438  * Convert a timestamp in NTP scale to a 64bit seconds value in the NTP
439  * scale with proper epoch unfolding around a given pivot or the current
440  * system time.
441  *
442  * Note: The pivot must be given in the UN*X time domain!
443  *
444  * This is also a periodic extension, but since the cycle is 2^32 and
445  * the shift is 2^31, we can do some *very* fast math without explicit
446  * divisions.
447  *-------------------------------------------------------------------
448  */
449 vint64
450 ntpcal_ntp_to_ntp(
451 	uint32_t      ntp,
452 	const time_t *pivot
453 	)
454 {
455 	vint64 res;
456 
457 #ifdef HAVE_INT64
458 
459 	res.q_s = (pivot)
460 		      ? *pivot
461 		      : now();
462 	res.Q_s -= 0x80000000;		/* unshift of half range */
463 	res.Q_s += (uint32_t)JAN_1970;	/* warp into NTP domain	 */
464 	ntp	-= res.D_s.lo;		/* cycle difference	 */
465 	res.Q_s += (uint64_t)ntp;	/* get expanded time	 */
466 
467 #else /* no 64bit scalars */
468 
469 	time_t tmp;
470 
471 	tmp = (pivot)
472 		  ? *pivot
473 		  : now();
474 	res = time_to_vint64(&tmp);
475 	M_SUB(res.D_s.hi, res.D_s.lo, 0, 0x80000000u);
476 	M_ADD(res.D_s.hi, res.D_s.lo, 0, (uint32_t)JAN_1970);/*into NTP */
477 	ntp -= res.D_s.lo;		/* cycle difference	 */
478 	M_ADD(res.D_s.hi, res.D_s.lo, 0, ntp);
479 
480 #endif /* no 64bit scalars */
481 
482 	return res;
483 }
484 
485 
486 /*
487  * ==================================================================
488  *
489  * Splitting values to composite entities
490  *
491  * ==================================================================
492  */
493 
494 /*
495  *-------------------------------------------------------------------
496  * Split a 64bit seconds value into elapsed days in 'res.hi' and
497  * elapsed seconds since midnight in 'res.lo' using explicit floor
498  * division. This function happily accepts negative time values as
499  * timestamps before the respective epoch start.
500  * -------------------------------------------------------------------
501  */
502 ntpcal_split
503 ntpcal_daysplit(
504 	const vint64 *ts
505 	)
506 {
507 	ntpcal_split res;
508 
509 #ifdef HAVE_INT64
510 
511 	/* manual floor division by SECSPERDAY */
512 	res.hi = (int32_t)(ts->q_s / SECSPERDAY);
513 	res.lo = (int32_t)(ts->q_s % SECSPERDAY);
514 	if (res.lo < 0) {
515 		res.hi -= 1;
516 		res.lo += SECSPERDAY;
517 	}
518 
519 #else
520 
521 	/*
522 	 * since we do not have 64bit ops, we have to this by hand.
523 	 * Luckily SECSPERDAY is 86400 is 675*128, so we do the division
524 	 * using chained 32/16 bit divisions and shifts.
525 	 */
526 	vint64	 op;
527 	uint32_t q, r, a;
528 	int	 isneg;
529 
530 	memcpy(&op, ts, sizeof(op));
531 	/* fix sign */
532 	isneg = M_ISNEG(op.D_s.hi);
533 	if (isneg)
534 		M_NEG(op.D_s.hi, op.D_s.lo);
535 
536 	/* save remainder of DIV 128, shift for divide */
537 	r  = op.D_s.lo & 127; /* save remainder bits */
538 	op.D_s.lo = (op.D_s.lo >> 7) | (op.D_s.hi << 25);
539 	op.D_s.hi = (op.D_s.hi >> 7);
540 
541 	/* now do a mnual division, trying to remove as many ops as
542 	 * possible -- division is always slow! An since we do not have
543 	 * the advantage of a specific 64/32 bit or even a specific 32/16
544 	 * bit division op, but must use the general 32/32bit division
545 	 * even if we *know* the divider fits into unsigned 16 bits, the
546 	 * exra code pathes should pay off.
547 	 */
548 	a = op.D_s.hi;
549 	if (a > 675u)
550 		a = a % 675u;
551 	if (a) {
552 		a = (a << 16) | op.W_s.lh;
553 		q = a / 675u;
554 		a = a % 675u;
555 
556 		a = (a << 16) | op.W_s.ll;
557 		q = (q << 16) | (a / 675u);
558 	} else {
559 		a = op.D_s.lo;
560 		q = a / 675u;
561 	}
562 	a = a % 675u;
563 
564 	/* assemble remainder */
565 	r |= a << 7;
566 
567 	/* fix sign of result */
568 	if (isneg) {
569 		if (r) {
570 			r = SECSPERDAY - r;
571 			q = ~q;
572 		} else
573 			q = ~q + 1;
574 	}
575 
576 	res.hi = q;
577 	res.lo = r;
578 
579 #endif
580 	return res;
581 }
582 
583 /*
584  *-------------------------------------------------------------------
585  * Split a 32bit seconds value into h/m/s and excessive days.  This
586  * function happily accepts negative time values as timestamps before
587  * midnight.
588  * -------------------------------------------------------------------
589  */
590 static int32_t
591 priv_timesplit(
592 	int32_t split[3],
593 	int32_t ts
594 	)
595 {
596 	int32_t days = 0;
597 
598 	/* make sure we have a positive offset into a day */
599 	if (ts < 0 || ts >= SECSPERDAY) {
600 		days = ts / SECSPERDAY;
601 		ts   = ts % SECSPERDAY;
602 		if (ts < 0) {
603 			days -= 1;
604 			ts   += SECSPERDAY;
605 		}
606 	}
607 
608 	/* get secs, mins, hours */
609 	split[2] = (uint8_t)(ts % SECSPERMIN);
610 	ts /= SECSPERMIN;
611 	split[1] = (uint8_t)(ts % MINSPERHR);
612 	split[0] = (uint8_t)(ts / MINSPERHR);
613 
614 	return days;
615 }
616 
617 /*
618  * ---------------------------------------------------------------------
619  * Given the number of elapsed days in the calendar era, split this
620  * number into the number of elapsed years in 'res.hi' and the number
621  * of elapsed days of that year in 'res.lo'.
622  *
623  * if 'isleapyear' is not NULL, it will receive an integer that is 0 for
624  * regular years and a non-zero value for leap years.
625  *---------------------------------------------------------------------
626  */
627 ntpcal_split
628 ntpcal_split_eradays(
629 	int32_t days,
630 	int  *isleapyear
631 	)
632 {
633 	ntpcal_split res;
634 	int32_t	     n400, n100, n004, n001, yday; /* calendar year cycles */
635 
636 	/*
637 	 * Split off calendar cycles, using floor division in the first
638 	 * step. After that first step, simple division does it because
639 	 * all operands are positive; alas, we have to be aware of the
640 	 * possibe cycle overflows for 100 years and 1 year, caused by
641 	 * the additional leap day.
642 	 */
643 	n400 = days / GREGORIAN_CYCLE_DAYS;
644 	yday = days % GREGORIAN_CYCLE_DAYS;
645 	if (yday < 0) {
646 		n400 -= 1;
647 		yday += GREGORIAN_CYCLE_DAYS;
648 	}
649 	n100 = yday / GREGORIAN_NORMAL_CENTURY_DAYS;
650 	yday = yday % GREGORIAN_NORMAL_CENTURY_DAYS;
651 	n004 = yday / GREGORIAN_NORMAL_LEAP_CYCLE_DAYS;
652 	yday = yday % GREGORIAN_NORMAL_LEAP_CYCLE_DAYS;
653 	n001 = yday / DAYSPERYEAR;
654 	yday = yday % DAYSPERYEAR;
655 
656 	/*
657 	 * check for leap cycle overflows and calculate the leap flag
658 	 * if needed
659 	 */
660 	if ((n001 | n100) > 3) {
661 		/* hit last day of leap year */
662 		n001 -= 1;
663 		yday += DAYSPERYEAR;
664 		if (isleapyear)
665 			*isleapyear = 1;
666 	} else if (isleapyear)
667 		*isleapyear = (n001 == 3) && ((n004 != 24) || (n100 == 3));
668 
669 	/* now merge the cycles to elapsed years, using horner scheme */
670 	res.hi = ((4*n400 + n100)*25 + n004)*4 + n001;
671 	res.lo = yday;
672 
673 	return res;
674 }
675 
676 /*
677  *---------------------------------------------------------------------
678  * Given a number of elapsed days in a year and a leap year indicator,
679  * split the number of elapsed days into the number of elapsed months in
680  * 'res.hi' and the number of elapsed days of that month in 'res.lo'.
681  *
682  * This function will fail and return {-1,-1} if the number of elapsed
683  * days is not in the valid range!
684  *---------------------------------------------------------------------
685  */
686 ntpcal_split
687 ntpcal_split_yeardays(
688 	int32_t eyd,
689 	int     isleapyear
690 	)
691 {
692 	ntpcal_split    res;
693 	const uint16_t *lt;	/* month length table	*/
694 
695 	/* check leap year flag and select proper table */
696 	lt = real_month_table[(isleapyear != 0)];
697 	if (0 <= eyd && eyd < lt[12]) {
698 		/* get zero-based month by approximation & correction step */
699 		res.hi = eyd >> 5;	   /* approx month; might be 1 too low */
700 		if (lt[res.hi + 1] <= eyd) /* fixup approximative month value  */
701 			res.hi += 1;
702 		res.lo = eyd - lt[res.hi];
703 	} else {
704 		res.lo = res.hi = -1;
705 	}
706 
707 	return res;
708 }
709 
710 /*
711  *---------------------------------------------------------------------
712  * Convert a RD into the date part of a 'struct calendar'.
713  *---------------------------------------------------------------------
714  */
715 int
716 ntpcal_rd_to_date(
717 	struct calendar *jd,
718 	int32_t		 rd
719 	)
720 {
721 	ntpcal_split split;
722 	int	     leaps;
723 	int	     retv;
724 
725 	leaps = 0;
726 	retv = 0;
727 	/* get day-of-week first */
728 	jd->weekday = rd % 7;
729 	if (jd->weekday >= 7)	/* unsigned! */
730 		jd->weekday += 7;
731 
732 	split = ntpcal_split_eradays(rd - 1, &leaps);
733 	retv  = leaps;
734 	/* get year and day-of-year */
735 	jd->year = (uint16_t)split.hi + 1;
736 	if (jd->year != split.hi + 1) {
737 		jd->year = 0;
738 		retv	 = -1;	/* bletch. overflow trouble. */
739 	}
740 	jd->yearday = (uint16_t)split.lo + 1;
741 
742 	/* convert to month and mday */
743 	split = ntpcal_split_yeardays(split.lo, leaps);
744 	jd->month    = (uint8_t)split.hi + 1;
745 	jd->monthday = (uint8_t)split.lo + 1;
746 
747 	return retv ? retv : leaps;
748 }
749 
750 /*
751  *---------------------------------------------------------------------
752  * Convert a RD into the date part of a 'struct tm'.
753  *---------------------------------------------------------------------
754  */
755 int
756 ntpcal_rd_to_tm(
757 	struct tm  *utm,
758 	int32_t	    rd
759 	)
760 {
761 	ntpcal_split split;
762 	int	     leaps;
763 
764 	leaps = 0;
765 	/* get day-of-week first */
766 	utm->tm_wday = rd % 7;
767 	if (utm->tm_wday < 0)
768 		utm->tm_wday += 7;
769 
770 	/* get year and day-of-year */
771 	split = ntpcal_split_eradays(rd - 1, &leaps);
772 	utm->tm_year = split.hi - 1899;
773 	utm->tm_yday = split.lo;	/* 0-based */
774 
775 	/* convert to month and mday */
776 	split = ntpcal_split_yeardays(split.lo, leaps);
777 	utm->tm_mon  = split.hi;	/* 0-based */
778 	utm->tm_mday = split.lo + 1;	/* 1-based */
779 
780 	return leaps;
781 }
782 
783 /*
784  *---------------------------------------------------------------------
785  * Take a value of seconds since midnight and split it into hhmmss in a
786  * 'struct calendar'.
787  *---------------------------------------------------------------------
788  */
789 int32_t
790 ntpcal_daysec_to_date(
791 	struct calendar *jd,
792 	int32_t		sec
793 	)
794 {
795 	int32_t days;
796 	int   ts[3];
797 
798 	days = priv_timesplit(ts, sec);
799 	jd->hour   = (uint8_t)ts[0];
800 	jd->minute = (uint8_t)ts[1];
801 	jd->second = (uint8_t)ts[2];
802 
803 	return days;
804 }
805 
806 /*
807  *---------------------------------------------------------------------
808  * Take a value of seconds since midnight and split it into hhmmss in a
809  * 'struct tm'.
810  *---------------------------------------------------------------------
811  */
812 int32_t
813 ntpcal_daysec_to_tm(
814 	struct tm *utm,
815 	int32_t	   sec
816 	)
817 {
818 	int32_t days;
819 	int32_t ts[3];
820 
821 	days = priv_timesplit(ts, sec);
822 	utm->tm_hour = ts[0];
823 	utm->tm_min  = ts[1];
824 	utm->tm_sec  = ts[2];
825 
826 	return days;
827 }
828 
829 /*
830  *---------------------------------------------------------------------
831  * take a split representation for day/second-of-day and day offset
832  * and convert it to a 'struct calendar'. The seconds will be normalised
833  * into the range of a day, and the day will be adjusted accordingly.
834  *
835  * returns >0 if the result is in a leap year, 0 if in a regular
836  * year and <0 if the result did not fit into the calendar struct.
837  *---------------------------------------------------------------------
838  */
839 int
840 ntpcal_daysplit_to_date(
841 	struct calendar	   *jd,
842 	const ntpcal_split *ds,
843 	int32_t		    dof
844 	)
845 {
846 	dof += ntpcal_daysec_to_date(jd, ds->lo);
847 	return ntpcal_rd_to_date(jd, ds->hi + dof);
848 }
849 
850 /*
851  *---------------------------------------------------------------------
852  * take a split representation for day/second-of-day and day offset
853  * and convert it to a 'struct tm'. The seconds will be normalised
854  * into the range of a day, and the day will be adjusted accordingly.
855  *
856  * returns 1 if the result is in a leap year and zero if in a regular
857  * year.
858  *---------------------------------------------------------------------
859  */
860 int
861 ntpcal_daysplit_to_tm(
862 	struct tm	   *utm,
863 	const ntpcal_split *ds ,
864 	int32_t		    dof
865 	)
866 {
867 	dof += ntpcal_daysec_to_tm(utm, ds->lo);
868 
869 	return ntpcal_rd_to_tm(utm, ds->hi + dof);
870 }
871 
872 /*
873  *---------------------------------------------------------------------
874  * Take a UN*X time and convert to a calendar structure.
875  *---------------------------------------------------------------------
876  */
877 int
878 ntpcal_time_to_date(
879 	struct calendar	*jd,
880 	const vint64	*ts
881 	)
882 {
883 	ntpcal_split ds;
884 
885 	ds = ntpcal_daysplit(ts);
886 	ds.hi += ntpcal_daysec_to_date(jd, ds.lo);
887 	ds.hi += DAY_UNIX_STARTS;
888 
889 	return ntpcal_rd_to_date(jd, ds.hi);
890 }
891 
892 
893 /*
894  * ==================================================================
895  *
896  * merging composite entities
897  *
898  * ==================================================================
899  */
900 
901 /*
902  *---------------------------------------------------------------------
903  * Merge a number of days and a number of seconds into seconds,
904  * expressed in 64 bits to avoid overflow.
905  *---------------------------------------------------------------------
906  */
907 vint64
908 ntpcal_dayjoin(
909 	int32_t days,
910 	int32_t secs
911 	)
912 {
913 	vint64 res;
914 
915 #ifdef HAVE_INT64
916 
917 	res.q_s	 = days;
918 	res.q_s *= SECSPERDAY;
919 	res.q_s += secs;
920 
921 #else
922 
923 	uint32_t p1, p2;
924 	int	 isneg;
925 
926 	/*
927 	 * res = days *86400 + secs, using manual 16/32 bit
928 	 * multiplications and shifts.
929 	 */
930 	isneg = (days < 0);
931 	if (isneg)
932 		days = -days;
933 
934 	/* assemble days * 675 */
935 	res.D_s.lo = (days & 0xFFFF) * 675u;
936 	res.D_s.hi = 0;
937 	p1 = (days >> 16) * 675u;
938 	p2 = p1 >> 16;
939 	p1 = p1 << 16;
940 	M_ADD(res.D_s.hi, res.D_s.lo, p2, p1);
941 
942 	/* mul by 128, using shift */
943 	res.D_s.hi = (res.D_s.hi << 7) | (res.D_s.lo >> 25);
944 	res.D_s.lo = (res.D_s.lo << 7);
945 
946 	/* fix sign */
947 	if (isneg)
948 		M_NEG(res.D_s.hi, res.D_s.lo);
949 
950 	/* properly add seconds */
951 	p2 = 0;
952 	if (secs < 0) {
953 		p1 = (uint32_t)-secs;
954 		M_NEG(p2, p1);
955 	} else {
956 		p1 = (uint32_t)secs;
957 	}
958 	M_ADD(res.D_s.hi, res.D_s.lo, p2, p1);
959 
960 #endif
961 
962 	return res;
963 }
964 
965 /*
966  *---------------------------------------------------------------------
967  * Convert elapsed years in Era into elapsed days in Era.
968  *
969  * To accomodate for negative values of years, floor division would be
970  * required for all division operations. This can be eased by first
971  * splitting the years into full 400-year cycles and years in the
972  * cycle. Only this operation must be coded as a full floor division; as
973  * the years in the cycle is a non-negative number, all other divisions
974  * can be regular truncated divisions.
975  *---------------------------------------------------------------------
976  */
977 int32_t
978 ntpcal_days_in_years(
979 	int32_t years
980 	)
981 {
982 	int32_t cycle; /* full gregorian cycle */
983 
984 	/* split off full calendar cycles, using floor division */
985 	cycle = years / 400;
986 	years = years % 400;
987 	if (years < 0) {
988 		cycle -= 1;
989 		years += 400;
990 	}
991 
992 	/*
993 	 * Calculate days in cycle. years now is a non-negative number,
994 	 * holding the number of years in the 400-year cycle.
995 	 */
996 	return cycle * GREGORIAN_CYCLE_DAYS
997 	     + years * DAYSPERYEAR	/* days inregular years	*/
998 	     + years / 4		/* 4 year leap rule	*/
999 	     - years / 100;		/* 100 year leap rule	*/
1000 	/* the 400-year rule does not apply due to full-cycle split-off */
1001 }
1002 
1003 /*
1004  *---------------------------------------------------------------------
1005  * Convert a number of elapsed month in a year into elapsed days in year.
1006  *
1007  * The month will be normalized, and 'res.hi' will contain the
1008  * excessive years that must be considered when converting the years,
1009  * while 'res.lo' will contain the number of elapsed days since start
1010  * of the year.
1011  *
1012  * This code uses the shifted-month-approach to convert month to days,
1013  * because then there is no need to have explicit leap year
1014  * information.	 The slight disadvantage is that for most month values
1015  * the result is a negative value, and the year excess is one; the
1016  * conversion is then simply based on the start of the following year.
1017  *---------------------------------------------------------------------
1018  */
1019 ntpcal_split
1020 ntpcal_days_in_months(
1021 	int32_t m
1022 	)
1023 {
1024 	ntpcal_split res;
1025 
1026 	/* normalize month into range */
1027 	res.hi = 0;
1028 	res.lo = m;
1029 	if (res.lo < 0 || res.lo >= 12) {
1030 		res.hi = res.lo / 12;
1031 		res.lo = res.lo % 12;
1032 		if (res.lo < 0) {
1033 			res.hi -= 1;
1034 			res.lo += 12;
1035 		}
1036 	}
1037 
1038 	/* add 10 month for year starting with march */
1039 	if (res.lo < 2)
1040 		res.lo += 10;
1041 	else {
1042 		res.hi += 1;
1043 		res.lo -= 2;
1044 	}
1045 
1046 	/* get cummulated days in year with unshift */
1047 	res.lo = shift_month_table[res.lo] - 306;
1048 
1049 	return res;
1050 }
1051 
1052 /*
1053  *---------------------------------------------------------------------
1054  * Convert ELAPSED years/months/days of gregorian calendar to elapsed
1055  * days in Gregorian epoch.
1056  *
1057  * If you want to convert years and days-of-year, just give a month of
1058  * zero.
1059  *---------------------------------------------------------------------
1060  */
1061 int32_t
1062 ntpcal_edate_to_eradays(
1063 	int32_t years,
1064 	int32_t mons,
1065 	int32_t mdays
1066 	)
1067 {
1068 	ntpcal_split tmp;
1069 	int32_t	     res;
1070 
1071 	if (mons) {
1072 		tmp = ntpcal_days_in_months(mons);
1073 		res = ntpcal_days_in_years(years + tmp.hi) + tmp.lo;
1074 	} else
1075 		res = ntpcal_days_in_years(years);
1076 	res += mdays;
1077 
1078 	return res;
1079 }
1080 
1081 /*
1082  *---------------------------------------------------------------------
1083  * Convert ELAPSED years/months/days of gregorian calendar to elapsed
1084  * days in year.
1085  *
1086  * Note: This will give the true difference to the start of the given year,
1087  * even if months & days are off-scale.
1088  *---------------------------------------------------------------------
1089  */
1090 int32_t
1091 ntpcal_edate_to_yeardays(
1092 	int32_t years,
1093 	int32_t mons,
1094 	int32_t mdays
1095 	)
1096 {
1097 	ntpcal_split tmp;
1098 
1099 	if (0 <= mons && mons < 12) {
1100 		years += 1;
1101 		mdays += real_month_table[is_leapyear(years)][mons];
1102 	} else {
1103 		tmp = ntpcal_days_in_months(mons);
1104 		mdays += tmp.lo
1105 		       + ntpcal_days_in_years(years + tmp.hi)
1106 		       - ntpcal_days_in_years(years);
1107 	}
1108 
1109 	return mdays;
1110 }
1111 
1112 /*
1113  *---------------------------------------------------------------------
1114  * Convert elapsed days and the hour/minute/second information into
1115  * total seconds.
1116  *
1117  * If 'isvalid' is not NULL, do a range check on the time specification
1118  * and tell if the time input is in the normal range, permitting for a
1119  * single leapsecond.
1120  *---------------------------------------------------------------------
1121  */
1122 int32_t
1123 ntpcal_etime_to_seconds(
1124 	int32_t hours,
1125 	int32_t minutes,
1126 	int32_t seconds
1127 	)
1128 {
1129 	int32_t res;
1130 
1131 	res = (hours * MINSPERHR + minutes) * SECSPERMIN + seconds;
1132 
1133 	return res;
1134 }
1135 
1136 /*
1137  *---------------------------------------------------------------------
1138  * Convert the date part of a 'struct tm' (that is, year, month,
1139  * day-of-month) into the RD of that day.
1140  *---------------------------------------------------------------------
1141  */
1142 int32_t
1143 ntpcal_tm_to_rd(
1144 	const struct tm *utm
1145 	)
1146 {
1147 	return ntpcal_edate_to_eradays(utm->tm_year + 1899,
1148 				       utm->tm_mon,
1149 				       utm->tm_mday - 1) + 1;
1150 }
1151 
1152 /*
1153  *---------------------------------------------------------------------
1154  * Convert the date part of a 'struct calendar' (that is, year, month,
1155  * day-of-month) into the RD of that day.
1156  *---------------------------------------------------------------------
1157  */
1158 int32_t
1159 ntpcal_date_to_rd(
1160 	const struct calendar *jd
1161 	)
1162 {
1163 	return ntpcal_edate_to_eradays((int32_t)jd->year - 1,
1164 				       (int32_t)jd->month - 1,
1165 				       (int32_t)jd->monthday - 1) + 1;
1166 }
1167 
1168 /*
1169  *---------------------------------------------------------------------
1170  * convert a year number to rata die of year start
1171  *---------------------------------------------------------------------
1172  */
1173 int32_t
1174 ntpcal_year_to_ystart(
1175 	int32_t year
1176 	)
1177 {
1178 	return ntpcal_days_in_years(year - 1) + 1;
1179 }
1180 
1181 /*
1182  *---------------------------------------------------------------------
1183  * For a given RD, get the RD of the associated year start,
1184  * that is, the RD of the last January,1st on or before that day.
1185  *---------------------------------------------------------------------
1186  */
1187 int32_t
1188 ntpcal_rd_to_ystart(
1189 	int32_t rd
1190 	)
1191 {
1192 	/*
1193 	 * Rather simple exercise: split the day number into elapsed
1194 	 * years and elapsed days, then remove the elapsed days from the
1195 	 * input value. Nice'n sweet...
1196 	 */
1197 	return rd - ntpcal_split_eradays(rd - 1, NULL).lo;
1198 }
1199 
1200 /*
1201  *---------------------------------------------------------------------
1202  * For a given RD, get the RD of the associated month start.
1203  *---------------------------------------------------------------------
1204  */
1205 int32_t
1206 ntpcal_rd_to_mstart(
1207 	int32_t rd
1208 	)
1209 {
1210 	ntpcal_split split;
1211 	int	     leaps;
1212 
1213 	split = ntpcal_split_eradays(rd - 1, &leaps);
1214 	split = ntpcal_split_yeardays(split.lo, leaps);
1215 
1216 	return rd - split.lo;
1217 }
1218 
1219 /*
1220  *---------------------------------------------------------------------
1221  * take a 'struct calendar' and get the seconds-of-day from it.
1222  *---------------------------------------------------------------------
1223  */
1224 int32_t
1225 ntpcal_date_to_daysec(
1226 	const struct calendar *jd
1227 	)
1228 {
1229 	return ntpcal_etime_to_seconds(jd->hour, jd->minute,
1230 				       jd->second);
1231 }
1232 
1233 /*
1234  *---------------------------------------------------------------------
1235  * take a 'struct tm' and get the seconds-of-day from it.
1236  *---------------------------------------------------------------------
1237  */
1238 int32_t
1239 ntpcal_tm_to_daysec(
1240 	const struct tm *utm
1241 	)
1242 {
1243 	return ntpcal_etime_to_seconds(utm->tm_hour, utm->tm_min,
1244 				       utm->tm_sec);
1245 }
1246 
1247 /*
1248  *---------------------------------------------------------------------
1249  * take a 'struct calendar' and convert it to a 'time_t'
1250  *---------------------------------------------------------------------
1251  */
1252 time_t
1253 ntpcal_date_to_time(
1254 	const struct calendar *jd
1255 	)
1256 {
1257 	vint64  join;
1258 	int32_t days, secs;
1259 
1260 	days = ntpcal_date_to_rd(jd) - DAY_UNIX_STARTS;
1261 	secs = ntpcal_date_to_daysec(jd);
1262 	join = ntpcal_dayjoin(days, secs);
1263 
1264 	return vint64_to_time(&join);
1265 }
1266 
1267 
1268 /*
1269  * ==================================================================
1270  *
1271  * extended and unchecked variants of caljulian/caltontp
1272  *
1273  * ==================================================================
1274  */
1275 int
1276 ntpcal_ntp64_to_date(
1277 	struct calendar *jd,
1278 	const vint64    *ntp
1279 	)
1280 {
1281 	ntpcal_split ds;
1282 
1283 	ds = ntpcal_daysplit(ntp);
1284 	ds.hi += ntpcal_daysec_to_date(jd, ds.lo);
1285 
1286 	return ntpcal_rd_to_date(jd, ds.hi + DAY_NTP_STARTS);
1287 }
1288 
1289 int
1290 ntpcal_ntp_to_date(
1291 	struct calendar *jd,
1292 	uint32_t	 ntp,
1293 	const time_t	*piv
1294 	)
1295 {
1296 	vint64	ntp64;
1297 
1298 	/*
1299 	 * Unfold ntp time around current time into NTP domain. Split
1300 	 * into days and seconds, shift days into CE domain and
1301 	 * process the parts.
1302 	 */
1303 	ntp64 = ntpcal_ntp_to_ntp(ntp, piv);
1304 	return ntpcal_ntp64_to_date(jd, &ntp64);
1305 }
1306 
1307 
1308 vint64
1309 ntpcal_date_to_ntp64(
1310 	const struct calendar *jd
1311 	)
1312 {
1313 	/*
1314 	 * Convert date to NTP. Ignore yearday, use d/m/y only.
1315 	 */
1316 	return ntpcal_dayjoin(ntpcal_date_to_rd(jd) - DAY_NTP_STARTS,
1317 			      ntpcal_date_to_daysec(jd));
1318 }
1319 
1320 
1321 uint32_t
1322 ntpcal_date_to_ntp(
1323 	const struct calendar *jd
1324 	)
1325 {
1326 	/*
1327 	 * Get lower half of 64-bit NTP timestamp from date/time.
1328 	 */
1329 	return ntpcal_date_to_ntp64(jd).d_s.lo;
1330 }
1331 
1332 
1333 
1334 /*
1335  * ==================================================================
1336  *
1337  * day-of-week calculations
1338  *
1339  * ==================================================================
1340  */
1341 /*
1342  * Given a RataDie and a day-of-week, calculate a RDN that is reater-than,
1343  * greater-or equal, closest, less-or-equal or less-than the given RDN
1344  * and denotes the given day-of-week
1345  */
1346 int32_t
1347 ntpcal_weekday_gt(
1348 	int32_t rdn,
1349 	int32_t dow
1350 	)
1351 {
1352 	return ntpcal_periodic_extend(rdn+1, dow, 7);
1353 }
1354 
1355 int32_t
1356 ntpcal_weekday_ge(
1357 	int32_t rdn,
1358 	int32_t dow
1359 	)
1360 {
1361 	return ntpcal_periodic_extend(rdn, dow, 7);
1362 }
1363 
1364 int32_t
1365 ntpcal_weekday_close(
1366 	int32_t rdn,
1367 	int32_t dow
1368 	)
1369 {
1370 	return ntpcal_periodic_extend(rdn-3, dow, 7);
1371 }
1372 
1373 int32_t
1374 ntpcal_weekday_le(
1375 	int32_t rdn,
1376 	int32_t dow
1377 	)
1378 {
1379 	return ntpcal_periodic_extend(rdn, dow, -7);
1380 }
1381 
1382 int32_t
1383 ntpcal_weekday_lt(
1384 	int32_t rdn,
1385 	int32_t dow
1386 	)
1387 {
1388 	return ntpcal_periodic_extend(rdn-1, dow, -7);
1389 }
1390 
1391 /*
1392  * ==================================================================
1393  *
1394  * ISO week-calendar conversions
1395  *
1396  * The ISO8601 calendar defines a calendar of years, weeks and weekdays.
1397  * It is related to the Gregorian calendar, and a ISO year starts at the
1398  * Monday closest to Jan,1st of the corresponding Gregorian year.  A ISO
1399  * calendar year has always 52 or 53 weeks, and like the Grogrian
1400  * calendar the ISO8601 calendar repeats itself every 400 years, or
1401  * 146097 days, or 20871 weeks.
1402  *
1403  * While it is possible to write ISO calendar functions based on the
1404  * Gregorian calendar functions, the following implementation takes a
1405  * different approach, based directly on years and weeks.
1406  *
1407  * Analysis of the tabulated data shows that it is not possible to
1408  * interpolate from years to weeks over a full 400 year range; cyclic
1409  * shifts over 400 years do not provide a solution here. But it *is*
1410  * possible to interpolate over every single century of the 400-year
1411  * cycle. (The centennial leap year rule seems to be the culprit here.)
1412  *
1413  * It can be shown that a conversion from years to weeks can be done
1414  * using a linear transformation of the form
1415  *
1416  *   w = floor( y * a + b )
1417  *
1418  * where the slope a must hold to
1419  *
1420  *  52.1780821918 <= a < 52.1791044776
1421  *
1422  * and b must be chosen according to the selected slope and the number
1423  * of the century in a 400-year period.
1424  *
1425  * The inverse calculation can also be done in this way. Careful scaling
1426  * provides an unlimited set of integer coefficients a,k,b that enable
1427  * us to write the calulation in the form
1428  *
1429  *   w = (y * a	 + b ) / k
1430  *   y = (w * a' + b') / k'
1431  *
1432  * In this implementation the values of k and k' are chosen to be
1433  * smallest possible powers of two, so the division can be implemented
1434  * as shifts if the optimiser chooses to do so.
1435  *
1436  * ==================================================================
1437  */
1438 
1439 /*
1440  * Given a number of elapsed (ISO-)years since the begin of the
1441  * christian era, return the number of elapsed weeks corresponding to
1442  * the number of years.
1443  */
1444 int32_t
1445 isocal_weeks_in_years(
1446 	int32_t years
1447 	)
1448 {
1449 	/*
1450 	 * use: w = (y * 53431 + b[c]) / 1024 as interpolation
1451 	 */
1452 	static const int32_t bctab[4] = { 449, 157, 889, 597 };
1453 	int32_t cycle; /* full gregorian cycle */
1454 	int32_t cents; /* full centuries	   */
1455 	int32_t weeks; /* accumulated weeks	   */
1456 
1457 	/* split off full calendar cycles, using floor division */
1458 	cycle = years / 400;
1459 	years = years % 400;
1460 	if (years < 0) {
1461 		cycle -= 1;
1462 		years += 400;
1463 	}
1464 
1465 	/* split off full centuries */
1466 	cents = years / 100;
1467 	years = years % 100;
1468 
1469 	/*
1470 	 * calculate elapsed weeks, taking into account that the
1471 	 * first, third and fourth century have 5218 weeks but the
1472 	 * second century falls short by one week.
1473 	 */
1474 	weeks = (years * 53431 + bctab[cents]) / 1024;
1475 
1476 	return cycle * GREGORIAN_CYCLE_WEEKS
1477 	     + cents * 5218 - (cents > 1)
1478 	     + weeks;
1479 }
1480 
1481 /*
1482  * Given a number of elapsed weeks since the begin of the christian
1483  * era, split this number into the number of elapsed years in res.hi
1484  * and the excessive number of weeks in res.lo. (That is, res.lo is
1485  * the number of elapsed weeks in the remaining partial year.)
1486  */
1487 ntpcal_split
1488 isocal_split_eraweeks(
1489 	int32_t weeks
1490 	)
1491 {
1492 	/*
1493 	 * use: y = (w * 157 + b[c]) / 8192 as interpolation
1494 	 */
1495 	static const int32_t bctab[4] = { 85, 131, 17, 62 };
1496 	ntpcal_split res;
1497 	int32_t	     cents;
1498 
1499 	/*
1500 	 * split off 400-year cycles, using the fact that a 400-year
1501 	 * cycle has 146097 days, which is exactly 20871 weeks.
1502 	 */
1503 	res.hi = weeks / GREGORIAN_CYCLE_WEEKS;
1504 	res.lo = weeks % GREGORIAN_CYCLE_WEEKS;
1505 	if (res.lo < 0) {
1506 		res.hi -= 1;
1507 		res.lo += GREGORIAN_CYCLE_WEEKS;
1508 	}
1509 	res.hi *= 400;
1510 
1511 	/*
1512 	 * split off centuries, taking into account that the first,
1513 	 * third and fourth century have 5218 weeks but that the
1514 	 * second century falls short by one week.
1515 	 */
1516 	res.lo += (res.lo >= 10435);
1517 	cents	= res.lo / 5218;
1518 	res.lo %= 5218;		/* res.lo is weeks in century now */
1519 
1520 	/* convert elapsed weeks in century to elapsed years and weeks */
1521 	res.lo	= res.lo * 157 + bctab[cents];
1522 	res.hi += cents * 100 + res.lo / 8192;
1523 	res.lo	= (res.lo % 8192) / 157;
1524 
1525 	return res;
1526 }
1527 
1528 /*
1529  * Given a second in the NTP time scale and a pivot, expand the NTP
1530  * time stamp around the pivot and convert into an ISO calendar time
1531  * stamp.
1532  */
1533 int
1534 isocal_ntp64_to_date(
1535 	struct isodate *id,
1536 	const vint64   *ntp
1537 	)
1538 {
1539 	ntpcal_split ds;
1540 	int32_t      ts[3];
1541 
1542 	/*
1543 	 * Split NTP time into days and seconds, shift days into CE
1544 	 * domain and process the parts.
1545 	 */
1546 	ds = ntpcal_daysplit(ntp);
1547 
1548 	/* split time part */
1549 	ds.hi += priv_timesplit(ts, ds.lo);
1550 	id->hour   = (uint8_t)ts[0];
1551 	id->minute = (uint8_t)ts[1];
1552 	id->second = (uint8_t)ts[2];
1553 
1554 	/* split date part */
1555 	ds.lo = ds.hi + DAY_NTP_STARTS - 1;	/* elapsed era days  */
1556 	ds.hi = ds.lo / 7;			/* elapsed era weeks */
1557 	ds.lo = ds.lo % 7;			/* elapsed week days */
1558 	if (ds.lo < 0) {			/* floor division!   */
1559 		ds.hi -= 1;
1560 		ds.lo += 7;
1561 	}
1562 	id->weekday = (uint8_t)ds.lo + 1;	/* weekday result    */
1563 
1564 	ds = isocal_split_eraweeks(ds.hi);	/* elapsed years&week*/
1565 	id->year = (uint16_t)ds.hi + 1;		/* shift to current  */
1566 	id->week = (uint8_t )ds.lo + 1;
1567 
1568 	return (ds.hi >= 0 && ds.hi < 0x0000FFFF);
1569 }
1570 
1571 int
1572 isocal_ntp_to_date(
1573 	struct isodate *id,
1574 	uint32_t	ntp,
1575 	const time_t   *piv
1576 	)
1577 {
1578 	vint64	ntp64;
1579 
1580 	/*
1581 	 * Unfold ntp time around current time into NTP domain, then
1582 	 * convert the full time stamp.
1583 	 */
1584 	ntp64 = ntpcal_ntp_to_ntp(ntp, piv);
1585 	return isocal_ntp64_to_date(id, &ntp64);
1586 }
1587 
1588 /*
1589  * Convert a ISO date spec into a second in the NTP time scale,
1590  * properly truncated to 32 bit.
1591  */
1592 vint64
1593 isocal_date_to_ntp64(
1594 	const struct isodate *id
1595 	)
1596 {
1597 	int32_t weeks, days, secs;
1598 
1599 	weeks = isocal_weeks_in_years((int32_t)id->year - 1)
1600 	      + (int32_t)id->week - 1;
1601 	days = weeks * 7 + (int32_t)id->weekday;
1602 	/* days is RDN of ISO date now */
1603 	secs = ntpcal_etime_to_seconds(id->hour, id->minute, id->second);
1604 
1605 	return ntpcal_dayjoin(days - DAY_NTP_STARTS, secs);
1606 }
1607 
1608 uint32_t
1609 isocal_date_to_ntp(
1610 	const struct isodate *id
1611 	)
1612 {
1613 	/*
1614 	 * Get lower half of 64-bit NTP timestamp from date/time.
1615 	 */
1616 	return isocal_date_to_ntp64(id).d_s.lo;
1617 }
1618 
1619 /* -*-EOF-*- */
1620