git: 12f2e9525bd8 - stable/14 - leap-seconds: Update to leap-seconds 3960057600 obtained from IERS

From: Cy Schubert <cy_at_FreeBSD.org>
Date: Mon, 22 Jul 2024 02:36:41 UTC
The branch stable/14 has been updated by cy:

URL: https://cgit.FreeBSD.org/src/commit/?id=12f2e9525bd8be328febbc5839f763e4a271c05d

commit 12f2e9525bd8be328febbc5839f763e4a271c05d
Author:     Cy Schubert <cy@FreeBSD.org>
AuthorDate: 2024-07-21 01:41:09 +0000
Commit:     Cy Schubert <cy@FreeBSD.org>
CommitDate: 2024-07-22 02:36:30 +0000

    leap-seconds: Update to leap-seconds 3960057600 obtained from IERS
    
    IERS is the canonical source of leap-seconds. IANA, NIST and USNO obtain
    their leap-second updates from IERS.
    
    This resolves an issue for IPv6-only hosts as IERS is not accessible
    via IPv6, requiring IPv6-only host to rely on some other source,
    above.
    
    From this point forward we should fetch the file from IERS, the
    organization responsible for deciding when to insert leap-seconds.
    
    PR:             279413
    Obtained from:  https://hpiers.obspm.fr/iers/bul/bulc/ntp/leap-seconds.list
    Discussed with: imp
    
    (cherry picked from commit 04b4dcf04fc345b29b78e5061768091648b8ee2a)
---
 usr.sbin/ntp/ntpd/leap-seconds | 373 +++++++++++++----------------------------
 1 file changed, 119 insertions(+), 254 deletions(-)

diff --git a/usr.sbin/ntp/ntpd/leap-seconds b/usr.sbin/ntp/ntpd/leap-seconds
index c5a95aa51799..da0efc8c8566 100644
--- a/usr.sbin/ntp/ntpd/leap-seconds
+++ b/usr.sbin/ntp/ntpd/leap-seconds
@@ -1,255 +1,120 @@
+#	ATOMIC TIME
+#	Coordinated Universal Time (UTC) is the reference time scale derived
+#	from The "Temps Atomique International" (TAI) calculated by the Bureau
+#	International des Poids et Mesures (BIPM) using a worldwide network of atomic
+#	clocks. UTC differs from TAI by an integer number of seconds; it is the basis
+#	of all activities in the world.
 #
-#	In the following text, the symbol '#' introduces
-#	a comment, which continues from that symbol until
-#	the end of the line. A plain comment line has a
-#	whitespace character following the comment indicator.
-#	There are also special comment lines defined below.
-#	A special comment will always have a non-whitespace
-#	character in column 2.
-#
-#	A blank line should be ignored.
-#
-#	The following table shows the corrections that must
-#	be applied to compute International Atomic Time (TAI)
-#	from the Coordinated Universal Time (UTC) values that
-#	are transmitted by almost all time services.
-#
-#	The first column shows an epoch as a number of seconds
-#	since 1 January 1900, 00:00:00 (1900.0 is also used to
-#	indicate the same epoch.) Both of these time stamp formats
-#	ignore the complexities of the time scales that were
-#	used before the current definition of UTC at the start
-#	of 1972. (See note 3 below.)
-#	The second column shows the number of seconds that
-#	must be added to UTC to compute TAI for any timestamp
-#	at or after that epoch. The value on each line is
-#	valid from the indicated initial instant until the
-#	epoch given on the next one or indefinitely into the
-#	future if there is no next line.
-#	(The comment on each line shows the representation of
-#	the corresponding initial epoch in the usual
-#	day-month-year format. The epoch always begins at
-#	00:00:00 UTC on the indicated day. See Note 5 below.)
-#
-#	Important notes:
-#
-#	1. Coordinated Universal Time (UTC) is often referred to
-#	as Greenwich Mean Time (GMT). The GMT time scale is no
-#	longer used, and the use of GMT to designate UTC is
-#	discouraged.
-#
-#	2. The UTC time scale is realized by many national
-#	laboratories and timing centers. Each laboratory
-#	identifies its realization with its name: Thus
-#	UTC(NIST), UTC(USNO), etc. The differences among
-#	these different realizations are typically on the
-#	order of a few nanoseconds (i.e., 0.000 000 00x s)
-#	and can be ignored for many purposes. These differences
-#	are tabulated in Circular T, which is published monthly
-#	by the International Bureau of Weights and Measures
-#	(BIPM). See www.bipm.org for more information.
-#
-#	3. The current definition of the relationship between UTC
-#	and TAI dates from 1 January 1972. A number of different
-#	time scales were in use before that epoch, and it can be
-#	quite difficult to compute precise timestamps and time
-#	intervals in those "prehistoric" days. For more information,
-#	consult:
-#
-#		The Explanatory Supplement to the Astronomical
-#		Ephemeris.
-#	or
-#		Terry Quinn, "The BIPM and the Accurate Measurement
-#		of Time," Proc. of the IEEE, Vol. 79, pp. 894-905,
-#		July, 1991. <http://dx.doi.org/10.1109/5.84965>
-#		reprinted in:
-#		   Christine Hackman and Donald B Sullivan (eds.)
-#		   Time and Frequency Measurement
-#		   American Association of Physics Teachers (1996)
-#		   <http://tf.nist.gov/general/pdf/1168.pdf>, pp. 75-86
-#
-#	4. The decision to insert a leap second into UTC is currently
-#	the responsibility of the International Earth Rotation and
-#	Reference Systems Service. (The name was changed from the
-#	International Earth Rotation Service, but the acronym IERS
-#	is still used.)
-#
-#	Leap seconds are announced by the IERS in its Bulletin C.
-#
-#	See www.iers.org for more details.
-#
-#	Every national laboratory and timing center uses the
-#	data from the BIPM and the IERS to construct UTC(lab),
-#	their local realization of UTC.
-#
-#	Although the definition also includes the possibility
-#	of dropping seconds ("negative" leap seconds), this has
-#	never been done and is unlikely to be necessary in the
-#	foreseeable future.
-#
-#	5. If your system keeps time as the number of seconds since
-#	some epoch (e.g., NTP timestamps), then the algorithm for
-#	assigning a UTC time stamp to an event that happens during a positive
-#	leap second is not well defined. The official name of that leap
-#	second is 23:59:60, but there is no way of representing that time
-#	in these systems.
-#	Many systems of this type effectively stop the system clock for
-#	one second during the leap second and use a time that is equivalent
-#	to 23:59:59 UTC twice. For these systems, the corresponding TAI
-#	timestamp would be obtained by advancing to the next entry in the
-#	following table when the time equivalent to 23:59:59 UTC
-#	is used for the second time. Thus the leap second which
-#	occurred on 30 June 1972 at 23:59:59 UTC would have TAI
-#	timestamps computed as follows:
-#
-#	...
-#	30 June 1972 23:59:59 (2287785599, first time):	TAI= UTC + 10 seconds
-#	30 June 1972 23:59:60 (2287785599,second time):	TAI= UTC + 11 seconds
-#	1  July 1972 00:00:00 (2287785600)		TAI= UTC + 11 seconds
-#	...
-#
-#	If your system realizes the leap second by repeating 00:00:00 UTC twice
-#	(this is possible but not usual), then the advance to the next entry
-#	in the table must occur the second time that a time equivalent to
-#	00:00:00 UTC is used. Thus, using the same example as above:
-#
-#	...
-#       30 June 1972 23:59:59 (2287785599):		TAI= UTC + 10 seconds
-#       30 June 1972 23:59:60 (2287785600, first time):	TAI= UTC + 10 seconds
-#       1  July 1972 00:00:00 (2287785600,second time):	TAI= UTC + 11 seconds
-#	...
-#
-#	in both cases the use of timestamps based on TAI produces a smooth
-#	time scale with no discontinuity in the time interval. However,
-#	although the long-term behavior of the time scale is correct in both
-#	methods, the second method is technically not correct because it adds
-#	the extra second to the wrong day.
-#
-#	This complexity would not be needed for negative leap seconds (if they
-#	are ever used). The UTC time would skip 23:59:59 and advance from
-#	23:59:58 to 00:00:00 in that case. The TAI offset would decrease by
-#	1 second at the same instant. This is a much easier situation to deal
-#	with, since the difficulty of unambiguously representing the epoch
-#	during the leap second does not arise.
-#
-#	Some systems implement leap seconds by amortizing the leap second
-#	over the last few minutes of the day. The frequency of the local
-#	clock is decreased (or increased) to realize the positive (or
-#	negative) leap second. This method removes the time step described
-#	above. Although the long-term behavior of the time scale is correct
-#	in this case, this method introduces an error during the adjustment
-#	period both in time and in frequency with respect to the official
-#	definition of UTC.
-#
-#	Questions or comments to:
-#		Judah Levine
-#		Time and Frequency Division
-#		NIST
-#		Boulder, Colorado
-#		Judah.Levine@nist.gov
-#
-#	Last Update of leap second values:   8 July 2016
-#
-#	The following line shows this last update date in NTP timestamp
-#	format. This is the date on which the most recent change to
-#	the leap second data was added to the file. This line can
-#	be identified by the unique pair of characters in the first two
-#	columns as shown below.
-#
-#$	 3676924800
-#
-#	The NTP timestamps are in units of seconds since the NTP epoch,
-#	which is 1 January 1900, 00:00:00. The Modified Julian Day number
-#	corresponding to the NTP time stamp, X, can be computed as
-#
-#	X/86400 + 15020
-#
-#	where the first term converts seconds to days and the second
-#	term adds the MJD corresponding to the time origin defined above.
-#	The integer portion of the result is the integer MJD for that
-#	day, and any remainder is the time of day, expressed as the
-#	fraction of the day since 0 hours UTC. The conversion from day
-#	fraction to seconds or to hours, minutes, and seconds may involve
-#	rounding or truncation, depending on the method used in the
-#	computation.
-#
-#	The data in this file will be updated periodically as new leap
-#	seconds are announced. In addition to being entered on the line
-#	above, the update time (in NTP format) will be added to the basic
-#	file name leap-seconds to form the name leap-seconds.<NTP TIME>.
-#	In addition, the generic name leap-seconds.list will always point to
-#	the most recent version of the file.
-#
-#	This update procedure will be performed only when a new leap second
-#	is announced.
-#
-#	The following entry specifies the expiration date of the data
-#	in this file in units of seconds since the origin at the instant
-#	1 January 1900, 00:00:00. This expiration date will be changed
-#	at least twice per year whether or not a new leap second is
-#	announced. These semi-annual changes will be made no later
-#	than 1 June and 1 December of each year to indicate what
-#	action (if any) is to be taken on 30 June and 31 December,
-#	respectively. (These are the customary effective dates for new
-#	leap seconds.) This expiration date will be identified by a
-#	unique pair of characters in columns 1 and 2 as shown below.
-#	In the unlikely event that a leap second is announced with an
-#	effective date other than 30 June or 31 December, then this
-#	file will be edited to include that leap second as soon as it is
-#	announced or at least one month before the effective date
-#	(whichever is later).
-#	If an announcement by the IERS specifies that no leap second is
-#	scheduled, then only the expiration date of the file will
-#	be advanced to show that the information in the file is still
-#	current -- the update time stamp, the data and the name of the file
-#	will not change.
-#
-#	Updated through IERS Bulletin C67
-#	File expires on:  28 December 2024
-#
-#@	3944332800
-#
-2272060800	10	# 1 Jan 1972
-2287785600	11	# 1 Jul 1972
-2303683200	12	# 1 Jan 1973
-2335219200	13	# 1 Jan 1974
-2366755200	14	# 1 Jan 1975
-2398291200	15	# 1 Jan 1976
-2429913600	16	# 1 Jan 1977
-2461449600	17	# 1 Jan 1978
-2492985600	18	# 1 Jan 1979
-2524521600	19	# 1 Jan 1980
-2571782400	20	# 1 Jul 1981
-2603318400	21	# 1 Jul 1982
-2634854400	22	# 1 Jul 1983
-2698012800	23	# 1 Jul 1985
-2776982400	24	# 1 Jan 1988
-2840140800	25	# 1 Jan 1990
-2871676800	26	# 1 Jan 1991
-2918937600	27	# 1 Jul 1992
-2950473600	28	# 1 Jul 1993
-2982009600	29	# 1 Jul 1994
-3029443200	30	# 1 Jan 1996
-3076704000	31	# 1 Jul 1997
-3124137600	32	# 1 Jan 1999
-3345062400	33	# 1 Jan 2006
-3439756800	34	# 1 Jan 2009
-3550089600	35	# 1 Jul 2012
-3644697600	36	# 1 Jul 2015
-3692217600	37	# 1 Jan 2017
-#
-#	the following special comment contains the
-#	hash value of the data in this file computed
-#	use the secure hash algorithm as specified
-#	by FIPS 180-1. See the files in ~/pub/sha for
-#	the details of how this hash value is
-#	computed. Note that the hash computation
-#	ignores comments and whitespace characters
-#	in data lines. It includes the NTP values
-#	of both the last modification time and the
-#	expiration time of the file, but not the
-#	white space on those lines.
-#	the hash line is also ignored in the
-#	computation.
-#
-#h 	199a9d45 3f630d2f e47cb9cc c2f0fa47 96932227
+#
+#	ASTRONOMICAL TIME (UT1) is the time scale based on the rate of rotation of the earth.
+#	It is now mainly derived from Very Long Baseline Interferometry (VLBI). The various
+#	irregular fluctuations progressively detected in the rotation rate of the Earth led
+#	in 1972 to the replacement of UT1 by UTC as the reference time scale.
+#
+#
+#	LEAP SECOND
+#	Atomic clocks are more stable than the rate of the earth's rotation since the latter
+#	undergoes a full range of geophysical perturbations at various time scales: lunisolar
+#	and core-mantle torques, atmospheric and oceanic effects, etc.
+#	Leap seconds are needed to keep the two time scales in agreement, i.e. UT1-UTC smaller
+#	than 0.9 seconds. Therefore, when necessary a "leap second" is applied to UTC.
+#	Since the adoption of this system in 1972 it has been necessary to add a number of seconds to UTC,
+#	firstly due to the initial choice of the value of the second (1/86400 mean solar day of
+#	the year 1820) and secondly to the general slowing down of the Earth's rotation. It is
+#	theoretically possible to have a negative leap second (a second removed from UTC), but so far,
+#	all leap seconds have been positive (a second has been added to UTC). Based on what we know about
+#	the earth's rotation, it is unlikely that we will ever have a negative leap second.
+#
+#
+#	HISTORY
+#	The first leap second was added on June 30, 1972. Until the year 2000, it was necessary in average to add a
+#       leap second at a rate of 1 to 2 years. Since the year 2000 leap seconds are introduced with an
+#	average interval of 3 to 4 years due to the acceleration of the Earth's rotation speed.
+#
+#
+#	RESPONSIBILITY OF THE DECISION TO INTRODUCE A LEAP SECOND IN UTC
+#	The decision to introduce a leap second in UTC is the responsibility of the Earth Orientation Center of
+#	the International Earth Rotation and reference System Service (IERS). This center is located at Paris
+#	Observatory. According to international agreements, leap seconds should be scheduled only for certain dates:
+#	first preference is given to the end of December and June, and second preference at the end of March
+#	and September. Since the introduction of leap seconds in 1972, only dates in June and December were used.
+#
+#		Questions or comments to:
+#			Christian Bizouard:  christian.bizouard@obspm.fr
+#			Earth orientation Center of the IERS
+#			Paris Observatory, France
+#
+#
+#
+#    	COPYRIGHT STATUS OF THIS FILE
+#    	This file is in the public domain.
+#
+#
+#	VALIDITY OF THE FILE
+#	It is important to express the validity of the file. These next two dates are
+#	given in units of seconds since 1900.0.
+#
+#	1) Last update of the file.
+#
+#	Updated through IERS Bulletin C (https://hpiers.obspm.fr/iers/bul/bulc/bulletinc.dat)
+#
+#	The following line shows the last update of this file in NTP timestamp:
+#
+#$	3929093563
+#
+#	2) Expiration date of the file given on a semi-annual basis: last June or last December
+#
+#	File expires on 28 June 2025
+#
+#	Expire date in NTP timestamp:
+#
+#@	3960057600
+#
+#
+#	LIST OF LEAP SECONDS
+#	NTP timestamp (X parameter) is the number of seconds since 1900.0
+#
+#	MJD: The Modified Julian Day number. MJD = X/86400 + 15020
+#
+#	DTAI: The difference DTAI= TAI-UTC in units of seconds
+#	It is the quantity to add to UTC to get the time in TAI
+#
+#	Day Month Year : epoch in clear
+#
+#NTP Time      DTAI    Day Month Year
+#
+2272060800      10      # 1 Jan 1972
+2287785600      11      # 1 Jul 1972
+2303683200      12      # 1 Jan 1973
+2335219200      13      # 1 Jan 1974
+2366755200      14      # 1 Jan 1975
+2398291200      15      # 1 Jan 1976
+2429913600      16      # 1 Jan 1977
+2461449600      17      # 1 Jan 1978
+2492985600      18      # 1 Jan 1979
+2524521600      19      # 1 Jan 1980
+2571782400      20      # 1 Jul 1981
+2603318400      21      # 1 Jul 1982
+2634854400      22      # 1 Jul 1983
+2698012800      23      # 1 Jul 1985
+2776982400      24      # 1 Jan 1988
+2840140800      25      # 1 Jan 1990
+2871676800      26      # 1 Jan 1991
+2918937600      27      # 1 Jul 1992
+2950473600      28      # 1 Jul 1993
+2982009600      29      # 1 Jul 1994
+3029443200      30      # 1 Jan 1996
+3076704000      31      # 1 Jul 1997
+3124137600      32      # 1 Jan 1999
+3345062400      33      # 1 Jan 2006
+3439756800      34      # 1 Jan 2009
+3550089600      35      # 1 Jul 2012
+3644697600      36      # 1 Jul 2015
+3692217600      37      # 1 Jan 2017
+#
+#	A hash code has been generated to be able to verify the integrity
+#	of this file. For more information about using this hash code,
+#	please see the readme file in the 'source' directory :
+#	https://hpiers.obspm.fr/iers/bul/bulc/ntp/sources/README
+#
+#h	be738595 57b0cf1b b0218343 fb77062f 5a775e7