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leap-seconds.list (257697) leap-seconds.list (270817)
1#
2# In the following text, the symbol '#' introduces
1#
2# In the following text, the symbol '#' introduces
3# a comment, which continues from that symbol until
3# a comment, which continues from that symbol until
4# the end of the line. A plain comment line has a
5# whitespace character following the comment indicator.
4# the end of the line. A plain comment line has a
5# whitespace character following the comment indicator.
6# There are also special comment lines defined below.
7# A special comment will always have a non-whitespace
6# There are also special comment lines defined below.
7# A special comment will always have a non-whitespace
8# character in column 2.
9#
10# A blank line should be ignored.
11#
12# The following table shows the corrections that must
13# be applied to compute International Atomic Time (TAI)
14# from the Coordinated Universal Time (UTC) values that
15# are transmitted by almost all time services.
16#
17# The first column shows an epoch as a number of seconds
8# character in column 2.
9#
10# A blank line should be ignored.
11#
12# The following table shows the corrections that must
13# be applied to compute International Atomic Time (TAI)
14# from the Coordinated Universal Time (UTC) values that
15# are transmitted by almost all time services.
16#
17# The first column shows an epoch as a number of seconds
18# since 1900.0 and the second column shows the number of
19# seconds that must be added to UTC to compute TAI for
20# any timestamp at or after that epoch. The value on
21# each line is valid from the indicated initial instant
22# until the epoch given on the next one or indefinitely
23# into the future if there is no next line.
18# since 1 January 1900, 00:00:00 (1900.0 is also used to
19# indicate the same epoch.) Both of these time stamp formats
20# ignore the complexities of the time scales that were
21# used before the current definition of UTC at the start
22# of 1972. (See note 3 below.)
23# The second column shows the number of seconds that
24# must be added to UTC to compute TAI for any timestamp
25# at or after that epoch. The value on each line is
26# valid from the indicated initial instant until the
27# epoch given on the next one or indefinitely into the
28# future if there is no next line.
24# (The comment on each line shows the representation of
29# (The comment on each line shows the representation of
25# the corresponding initial epoch in the usual
30# the corresponding initial epoch in the usual
26# day-month-year format. The epoch always begins at
27# 00:00:00 UTC on the indicated day. See Note 5 below.)
31# day-month-year format. The epoch always begins at
32# 00:00:00 UTC on the indicated day. See Note 5 below.)
28#
33#
29# Important notes:
30#
31# 1. Coordinated Universal Time (UTC) is often referred to
32# as Greenwich Mean Time (GMT). The GMT time scale is no
33# longer used, and the use of GMT to designate UTC is
34# discouraged.
35#
34# Important notes:
35#
36# 1. Coordinated Universal Time (UTC) is often referred to
37# as Greenwich Mean Time (GMT). The GMT time scale is no
38# longer used, and the use of GMT to designate UTC is
39# discouraged.
40#
36# 2. The UTC time scale is realized by many national
41# 2. The UTC time scale is realized by many national
37# laboratories and timing centers. Each laboratory
38# identifies its realization with its name: Thus
39# UTC(NIST), UTC(USNO), etc. The differences among
40# these different realizations are typically on the
41# order of a few nanoseconds (i.e., 0.000 000 00x s)
42# and can be ignored for many purposes. These differences
43# are tabulated in Circular T, which is published monthly
44# by the International Bureau of Weights and Measures
45# (BIPM). See www.bipm.fr for more information.
46#
42# laboratories and timing centers. Each laboratory
43# identifies its realization with its name: Thus
44# UTC(NIST), UTC(USNO), etc. The differences among
45# these different realizations are typically on the
46# order of a few nanoseconds (i.e., 0.000 000 00x s)
47# and can be ignored for many purposes. These differences
48# are tabulated in Circular T, which is published monthly
49# by the International Bureau of Weights and Measures
50# (BIPM). See www.bipm.fr for more information.
51#
47# 3. The current defintion of the relationship between UTC
48# and TAI dates from 1 January 1972. A number of different
49# time scales were in use before than epoch, and it can be
50# quite difficult to compute precise timestamps and time
52# 3. The current definition of the relationship between UTC
53# and TAI dates from 1 January 1972. A number of different
54# time scales were in use before that epoch, and it can be
55# quite difficult to compute precise timestamps and time
51# intervals in those "prehistoric" days. For more information,
52# consult:
53#
54# The Explanatory Supplement to the Astronomical
55# Ephemeris.
56# or
57# Terry Quinn, "The BIPM and the Accurate Measurement
58# of Time," Proc. of the IEEE, Vol. 79, pp. 894-905,
59# July, 1991.
60#
56# intervals in those "prehistoric" days. For more information,
57# consult:
58#
59# The Explanatory Supplement to the Astronomical
60# Ephemeris.
61# or
62# Terry Quinn, "The BIPM and the Accurate Measurement
63# of Time," Proc. of the IEEE, Vol. 79, pp. 894-905,
64# July, 1991.
65#
61# 4. The insertion of leap seconds into UTC is currently the
62# responsibility of the International Earth Rotation Service,
63# which is located at the Paris Observatory:
66# 4. The decision to insert a leap second into UTC is currently
67# the responsibility of the International Earth Rotation and
68# Reference Systems Service. (The name was changed from the
69# International Earth Rotation Service, but the acronym IERS
70# is still used.)
64#
71#
65# Central Bureau of IERS
66# 61, Avenue de l'Observatoire
67# 75014 Paris, France.
72# Leap seconds are announced by the IERS in its Bulletin C.
68#
73#
69# Leap seconds are announced by the IERS in its Bulletin C
74# See www.iers.org for more details.
70#
75#
71# See hpiers.obspm.fr or www.iers.org for more details.
76# Every national laboratory and timing center uses the
77# data from the BIPM and the IERS to construct UTC(lab),
78# their local realization of UTC.
72#
79#
73# All national laboratories and timing centers use the
74# data from the BIPM and the IERS to construct their
75# local realizations of UTC.
76#
77# Although the definition also includes the possibility
80# Although the definition also includes the possibility
78# of dropping seconds ("negative" leap seconds), this has
79# never been done and is unlikely to be necessary in the
81# of dropping seconds ("negative" leap seconds), this has
82# never been done and is unlikely to be necessary in the
80# foreseeable future.
81#
82# 5. If your system keeps time as the number of seconds since
83# some epoch (e.g., NTP timestamps), then the algorithm for
84# assigning a UTC time stamp to an event that happens during a positive
83# foreseeable future.
84#
85# 5. If your system keeps time as the number of seconds since
86# some epoch (e.g., NTP timestamps), then the algorithm for
87# assigning a UTC time stamp to an event that happens during a positive
85# leap second is not well defined. The official name of that leap
86# second is 23:59:60, but there is no way of representing that time
87# in these systems.
88# Many systems of this type effectively stop the system clock for
89# one second during the leap second and use a time that is equivalent
90# to 23:59:59 UTC twice. For these systems, the corresponding TAI
88# leap second is not well defined. The official name of that leap
89# second is 23:59:60, but there is no way of representing that time
90# in these systems.
91# Many systems of this type effectively stop the system clock for
92# one second during the leap second and use a time that is equivalent
93# to 23:59:59 UTC twice. For these systems, the corresponding TAI
91# timestamp would be obtained by advancing to the next entry in the
92# following table when the time equivalent to 23:59:59 UTC
93# is used for the second time. Thus the leap second which
94# occurred on 30 June 1972 at 23:59:59 UTC would have TAI
95# timestamps computed as follows:
96#
97# ...
98# 30 June 1972 23:59:59 (2287785599, first time): TAI= UTC + 10 seconds
99# 30 June 1972 23:59:60 (2287785599,second time): TAI= UTC + 11 seconds
100# 1 July 1972 00:00:00 (2287785600) TAI= UTC + 11 seconds
101# ...
102#
103# If your system realizes the leap second by repeating 00:00:00 UTC twice
104# (this is possible but not usual), then the advance to the next entry
94# timestamp would be obtained by advancing to the next entry in the
95# following table when the time equivalent to 23:59:59 UTC
96# is used for the second time. Thus the leap second which
97# occurred on 30 June 1972 at 23:59:59 UTC would have TAI
98# timestamps computed as follows:
99#
100# ...
101# 30 June 1972 23:59:59 (2287785599, first time): TAI= UTC + 10 seconds
102# 30 June 1972 23:59:60 (2287785599,second time): TAI= UTC + 11 seconds
103# 1 July 1972 00:00:00 (2287785600) TAI= UTC + 11 seconds
104# ...
105#
106# If your system realizes the leap second by repeating 00:00:00 UTC twice
107# (this is possible but not usual), then the advance to the next entry
105# in the table must occur the second time that a time equivlent to
108# in the table must occur the second time that a time equivalent to
106# 00:00:00 UTC is used. Thus, using the same example as above:
107#
108# ...
109# 30 June 1972 23:59:59 (2287785599): TAI= UTC + 10 seconds
110# 30 June 1972 23:59:60 (2287785600, first time): TAI= UTC + 10 seconds
111# 1 July 1972 00:00:00 (2287785600,second time): TAI= UTC + 11 seconds
112# ...
113#
114# in both cases the use of timestamps based on TAI produces a smooth
109# 00:00:00 UTC is used. Thus, using the same example as above:
110#
111# ...
112# 30 June 1972 23:59:59 (2287785599): TAI= UTC + 10 seconds
113# 30 June 1972 23:59:60 (2287785600, first time): TAI= UTC + 10 seconds
114# 1 July 1972 00:00:00 (2287785600,second time): TAI= UTC + 11 seconds
115# ...
116#
117# in both cases the use of timestamps based on TAI produces a smooth
115# time scale with no discontinuity in the time interval.
118# time scale with no discontinuity in the time interval. However,
119# although the long-term behavior of the time scale is correct in both
120# methods, the second method is technically not correct because it adds
121# the extra second to the wrong day.
116#
122#
117# This complexity would not be needed for negative leap seconds (if they
118# are ever used). The UTC time would skip 23:59:59 and advance from
119# 23:59:58 to 00:00:00 in that case. The TAI offset would decrease by
120# 1 second at the same instant. This is a much easier situation to deal
121# with, since the difficulty of unambiguously representing the epoch
123# This complexity would not be needed for negative leap seconds (if they
124# are ever used). The UTC time would skip 23:59:59 and advance from
125# 23:59:58 to 00:00:00 in that case. The TAI offset would decrease by
126# 1 second at the same instant. This is a much easier situation to deal
127# with, since the difficulty of unambiguously representing the epoch
122# during the leap second does not arise.
123#
124# Questions or comments to:
125# Judah Levine
126# Time and Frequency Division
127# NIST
128# Boulder, Colorado
128# during the leap second does not arise.
129#
130# Questions or comments to:
131# Judah Levine
132# Time and Frequency Division
133# NIST
134# Boulder, Colorado
129# jlevine@boulder.nist.gov
135# Judah.Levine@nist.gov
130#
131# Last Update of leap second values: 11 January 2012
132#
136#
137# Last Update of leap second values: 11 January 2012
138#
133# The following line shows this last update date in NTP timestamp
139# The following line shows this last update date in NTP timestamp
134# format. This is the date on which the most recent change to
135# the leap second data was added to the file. This line can
140# format. This is the date on which the most recent change to
141# the leap second data was added to the file. This line can
136# be identified by the unique pair of characters in the first two
142# be identified by the unique pair of characters in the first two
137# columns as shown below.
138#
139#$ 3535228800
140#
141# The NTP timestamps are in units of seconds since the NTP epoch,
143# columns as shown below.
144#
145#$ 3535228800
146#
147# The NTP timestamps are in units of seconds since the NTP epoch,
142# which is 1900.0. The Modified Julian Day number corresponding
143# to the NTP time stamp, X, can be computed as
148# which is 1 January 1900, 00:00:00. The Modified Julian Day number
149# corresponding to the NTP time stamp, X, can be computed as
144#
145# X/86400 + 15020
146#
150#
151# X/86400 + 15020
152#
147# where the first term converts seconds to days and the second
148# term adds the MJD corresponding to 1900.0. The integer portion
149# of the result is the integer MJD for that day, and any remainder
150# is the time of day, expressed as the fraction of the day since 0
151# hours UTC. The conversion from day fraction to seconds or to
152# hours, minutes, and seconds may involve rounding or truncation,
153# depending on the method used in the computation.
153# where the first term converts seconds to days and the second
154# term adds the MJD corresponding to the time origin defined above.
155# The integer portion of the result is the integer MJD for that
156# day, and any remainder is the time of day, expressed as the
157# fraction of the day since 0 hours UTC. The conversion from day
158# fraction to seconds or to hours, minutes, and seconds may involve
159# rounding or truncation, depending on the method used in the
160# computation.
154#
161#
155# The data in this file will be updated periodically as new leap
162# The data in this file will be updated periodically as new leap
156# seconds are announced. In addition to being entered on the line
163# seconds are announced. In addition to being entered on the line
157# above, the update time (in NTP format) will be added to the basic
164# above, the update time (in NTP format) will be added to the basic
158# file name leap-seconds to form the name leap-seconds.<NTP TIME>.
165# file name leap-seconds to form the name leap-seconds.<NTP TIME>.
159# In addition, the generic name leap-seconds.list will always point to
166# In addition, the generic name leap-seconds.list will always point to
160# the most recent version of the file.
161#
162# This update procedure will be performed only when a new leap second
167# the most recent version of the file.
168#
169# This update procedure will be performed only when a new leap second
163# is announced.
170# is announced.
164#
165# The following entry specifies the expiration date of the data
171#
172# The following entry specifies the expiration date of the data
166# in this file in units of seconds since 1900.0. This expiration date
167# will be changed at least twice per year whether or not a new leap
168# second is announced. These semi-annual changes will be made no
169# later than 1 June and 1 December of each year to indicate what
170# action (if any) is to be taken on 30 June and 31 December,
173# in this file in units of seconds since the origin at the instant
174# 1 January 1900, 00:00:00. This expiration date will be changed
175# at least twice per year whether or not a new leap second is
176# announced. These semi-annual changes will be made no later
177# than 1 June and 1 December of each year to indicate what
178# action (if any) is to be taken on 30 June and 31 December,
171# respectively. (These are the customary effective dates for new
172# leap seconds.) This expiration date will be identified by a
173# unique pair of characters in columns 1 and 2 as shown below.
179# respectively. (These are the customary effective dates for new
180# leap seconds.) This expiration date will be identified by a
181# unique pair of characters in columns 1 and 2 as shown below.
174# In the unlikely event that a leap second is announced with an
182# In the unlikely event that a leap second is announced with an
175# effective date other than 30 June or 31 December, then this
176# file will be edited to include that leap second as soon as it is
177# announced or at least one month before the effective date
183# effective date other than 30 June or 31 December, then this
184# file will be edited to include that leap second as soon as it is
185# announced or at least one month before the effective date
178# (whichever is later).
179# If an announcement by the IERS specifies that no leap second is
180# scheduled, then only the expiration date of the file will
186# (whichever is later).
187# If an announcement by the IERS specifies that no leap second is
188# scheduled, then only the expiration date of the file will
181# be advanced to show that the information in the file is still
189# be advanced to show that the information in the file is still
182# current -- the update time stamp, the data and the name of the file
190# current -- the update time stamp, the data and the name of the file
183# will not change.
184#
191# will not change.
192#
185# Updated through IERS Bulletin C46
186# File expires on: 28 June 2014
193# Updated through IERS Bulletin C48
194# File expires on: 28 June 2015
187#
195#
188#@ 3612902400
196#@ 3644438400
189#
1902272060800 10 # 1 Jan 1972
1912287785600 11 # 1 Jul 1972
1922303683200 12 # 1 Jan 1973
1932335219200 13 # 1 Jan 1974
1942366755200 14 # 1 Jan 1975
1952398291200 15 # 1 Jan 1976
1962429913600 16 # 1 Jan 1977

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217# the following special comment contains the
218# hash value of the data in this file computed
219# use the secure hash algorithm as specified
220# by FIPS 180-1. See the files in ~/pub/sha for
221# the details of how this hash value is
222# computed. Note that the hash computation
223# ignores comments and whitespace characters
224# in data lines. It includes the NTP values
197#
1982272060800 10 # 1 Jan 1972
1992287785600 11 # 1 Jul 1972
2002303683200 12 # 1 Jan 1973
2012335219200 13 # 1 Jan 1974
2022366755200 14 # 1 Jan 1975
2032398291200 15 # 1 Jan 1976
2042429913600 16 # 1 Jan 1977

--- 20 unchanged lines hidden (view full) ---

225# the following special comment contains the
226# hash value of the data in this file computed
227# use the secure hash algorithm as specified
228# by FIPS 180-1. See the files in ~/pub/sha for
229# the details of how this hash value is
230# computed. Note that the hash computation
231# ignores comments and whitespace characters
232# in data lines. It includes the NTP values
225# of both the last modification time and the
233# of both the last modification time and the
226# expiration time of the file, but not the
227# white space on those lines.
228# the hash line is also ignored in the
229# computation.
230#
234# expiration time of the file, but not the
235# white space on those lines.
236# the hash line is also ignored in the
237# computation.
238#
231#h 1151a8f e85a5069 9000fcdb 3d5e5365 1d505b37
239#h a4862ccd c6f43c6 964f3604 85944a26 b5cfad4e