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Linux/kernel/time/timeconv.c

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  1 // SPDX-License-Identifier: LGPL-2.0+
  2 /*
  3  * Copyright (C) 1993, 1994, 1995, 1996, 1997 Free Software Foundation, Inc.
  4  * This file is part of the GNU C Library.
  5  * Contributed by Paul Eggert (eggert@twinsun.com).
  6  *
  7  * The GNU C Library is free software; you can redistribute it and/or
  8  * modify it under the terms of the GNU Library General Public License as
  9  * published by the Free Software Foundation; either version 2 of the
 10  * License, or (at your option) any later version.
 11  *
 12  * The GNU C Library is distributed in the hope that it will be useful,
 13  * but WITHOUT ANY WARRANTY; without even the implied warranty of
 14  * MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE.  See the GNU
 15  * Library General Public License for more details.
 16  *
 17  * You should have received a copy of the GNU Library General Public
 18  * License along with the GNU C Library; see the file COPYING.LIB.  If not,
 19  * write to the Free Software Foundation, Inc., 59 Temple Place - Suite 330,
 20  * Boston, MA 02111-1307, USA.
 21  */
 22 
 23 /*
 24  * Converts the calendar time to broken-down time representation
 25  *
 26  * 2009-7-14:
 27  *   Moved from glibc-2.6 to kernel by Zhaolei<zhaolei@cn.fujitsu.com>
 28  * 2021-06-02:
 29  *   Reimplemented by Cassio Neri <cassio.neri@gmail.com>
 30  */
 31 
 32 #include <linux/time.h>
 33 #include <linux/module.h>
 34 #include <linux/kernel.h>
 35 
 36 #define SECS_PER_HOUR   (60 * 60)
 37 #define SECS_PER_DAY    (SECS_PER_HOUR * 24)
 38 
 39 /**
 40  * time64_to_tm - converts the calendar time to local broken-down time
 41  *
 42  * @totalsecs:  the number of seconds elapsed since 00:00:00 on January 1, 1970,
 43  *              Coordinated Universal Time (UTC).
 44  * @offset:     offset seconds adding to totalsecs.
 45  * @result:     pointer to struct tm variable to receive broken-down time
 46  */
 47 void time64_to_tm(time64_t totalsecs, int offset, struct tm *result)
 48 {
 49         u32 u32tmp, day_of_century, year_of_century, day_of_year, month, day;
 50         u64 u64tmp, udays, century, year;
 51         bool is_Jan_or_Feb, is_leap_year;
 52         long days, rem;
 53         int remainder;
 54 
 55         days = div_s64_rem(totalsecs, SECS_PER_DAY, &remainder);
 56         rem = remainder;
 57         rem += offset;
 58         while (rem < 0) {
 59                 rem += SECS_PER_DAY;
 60                 --days;
 61         }
 62         while (rem >= SECS_PER_DAY) {
 63                 rem -= SECS_PER_DAY;
 64                 ++days;
 65         }
 66 
 67         result->tm_hour = rem / SECS_PER_HOUR;
 68         rem %= SECS_PER_HOUR;
 69         result->tm_min = rem / 60;
 70         result->tm_sec = rem % 60;
 71 
 72         /* January 1, 1970 was a Thursday. */
 73         result->tm_wday = (4 + days) % 7;
 74         if (result->tm_wday < 0)
 75                 result->tm_wday += 7;
 76 
 77         /*
 78          * The following algorithm is, basically, Proposition 6.3 of Neri
 79          * and Schneider [1]. In a few words: it works on the computational
 80          * (fictitious) calendar where the year starts in March, month = 2
 81          * (*), and finishes in February, month = 13. This calendar is
 82          * mathematically convenient because the day of the year does not
 83          * depend on whether the year is leap or not. For instance:
 84          *
 85          * March 1st            0-th day of the year;
 86          * ...
 87          * April 1st            31-st day of the year;
 88          * ...
 89          * January 1st          306-th day of the year; (Important!)
 90          * ...
 91          * February 28th        364-th day of the year;
 92          * February 29th        365-th day of the year (if it exists).
 93          *
 94          * After having worked out the date in the computational calendar
 95          * (using just arithmetics) it's easy to convert it to the
 96          * corresponding date in the Gregorian calendar.
 97          *
 98          * [1] "Euclidean Affine Functions and Applications to Calendar
 99          * Algorithms". https://arxiv.org/abs/2102.06959
100          *
101          * (*) The numbering of months follows tm more closely and thus,
102          * is slightly different from [1].
103          */
104 
105         udays   = ((u64) days) + 2305843009213814918ULL;
106 
107         u64tmp          = 4 * udays + 3;
108         century         = div64_u64_rem(u64tmp, 146097, &u64tmp);
109         day_of_century  = (u32) (u64tmp / 4);
110 
111         u32tmp          = 4 * day_of_century + 3;
112         u64tmp          = 2939745ULL * u32tmp;
113         year_of_century = upper_32_bits(u64tmp);
114         day_of_year     = lower_32_bits(u64tmp) / 2939745 / 4;
115 
116         year            = 100 * century + year_of_century;
117         is_leap_year    = year_of_century ? !(year_of_century % 4) : !(century % 4);
118 
119         u32tmp          = 2141 * day_of_year + 132377;
120         month           = u32tmp >> 16;
121         day             = ((u16) u32tmp) / 2141;
122 
123         /*
124          * Recall that January 1st is the 306-th day of the year in the
125          * computational (not Gregorian) calendar.
126          */
127         is_Jan_or_Feb   = day_of_year >= 306;
128 
129         /* Convert to the Gregorian calendar and adjust to Unix time. */
130         year            = year + is_Jan_or_Feb - 6313183731940000ULL;
131         month           = is_Jan_or_Feb ? month - 12 : month;
132         day             = day + 1;
133         day_of_year     += is_Jan_or_Feb ? -306 : 31 + 28 + is_leap_year;
134 
135         /* Convert to tm's format. */
136         result->tm_year = (long) (year - 1900);
137         result->tm_mon  = (int) month;
138         result->tm_mday = (int) day;
139         result->tm_yday = (int) day_of_year;
140 }
141 EXPORT_SYMBOL(time64_to_tm);
142 

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