Gecko [ rhythmmedical.in ]

Name	Size	Permission
africa	44.7 KB	-rw-rw-rw-
antarctica	15.46 KB	-rw-rw-rw-
asia	110.9 KB	-rw-rw-rw-
australasia	67.87 KB	-rw-rw-rw-
backward	3.99 KB	-rw-rw-rw-
etcetera	2.89 KB	-rw-rw-rw-
europe	118.54 KB	-rw-rw-rw-
factory	393 B	-rw-rw-rw-
iso3166.tab	4.22 KB	-rw-rw-rw-
leapseconds	3.11 KB	-rw-rw-rw-
northamerica	132.94 KB	-rw-rw-rw-
pacificnew	1.16 KB	-rw-rw-rw-
solar87	18.85 KB	-rw-rw-rw-
solar88	18.87 KB	-rw-rw-rw-
solar89	19.14 KB	-rw-rw-rw-
southamerica	72.65 KB	-rw-rw-rw-
systemv	1.51 KB	-rw-rw-rw-
yearistype.sh	680 B	-rw-rw-rw-
zone.tab	19.45 KB	-rw-rw-rw-

Code Editor : leapseconds

# <pre>
# This file is in the public domain, so clarified as of
# 2009-05-17 by Arthur David Olson.

# Allowance for leapseconds added to each timezone file.

# The International Earth Rotation Service periodically uses leap seconds
# to keep UTC to within 0.9 s of UT1
# (which measures the true angular orientation of the earth in space); see
# Terry J Quinn, The BIPM and the accurate measure of time,
# Proc IEEE 79, 7 (July 1991), 894-905.
# There were no leap seconds before 1972, because the official mechanism
# accounting for the discrepancy between atomic time and the earth's rotation
# did not exist until the early 1970s.

# The correction (+ or -) is made at the given time, so lines
# will typically look like:
#	Leap	YEAR	MON	DAY	23:59:60	+	R/S
# or
#	Leap	YEAR	MON	DAY	23:59:59	-	R/S

# If the leapsecond is Rolling (R) the given time is local time
# If the leapsecond is Stationary (S) the given time is UTC

# Leap	YEAR	MONTH	DAY	HH:MM:SS	CORR	R/S
Leap	1972	Jun	30	23:59:60	+	S
Leap	1972	Dec	31	23:59:60	+	S
Leap	1973	Dec	31	23:59:60	+	S
Leap	1974	Dec	31	23:59:60	+	S
Leap	1975	Dec	31	23:59:60	+	S
Leap	1976	Dec	31	23:59:60	+	S
Leap	1977	Dec	31	23:59:60	+	S
Leap	1978	Dec	31	23:59:60	+	S
Leap	1979	Dec	31	23:59:60	+	S
Leap	1981	Jun	30	23:59:60	+	S
Leap	1982	Jun	30	23:59:60	+	S
Leap	1983	Jun	30	23:59:60	+	S
Leap	1985	Jun	30	23:59:60	+	S
Leap	1987	Dec	31	23:59:60	+	S
Leap	1989	Dec	31	23:59:60	+	S
Leap	1990	Dec	31	23:59:60	+	S
Leap	1992	Jun	30	23:59:60	+	S
Leap	1993	Jun	30	23:59:60	+	S
Leap	1994	Jun	30	23:59:60	+	S
Leap	1995	Dec	31	23:59:60	+	S
Leap	1997	Jun	30	23:59:60	+	S
Leap	1998	Dec	31	23:59:60	+	S
Leap	2005	Dec	31	23:59:60	+	S
Leap	2008	Dec	31	23:59:60	+	S
Leap	2012	Jun	30	23:59:60	+	S

# INTERNATIONAL EARTH ROTATION AND REFERENCE SYSTEMS SERVICE (IERS)
#
# SERVICE INTERNATIONAL DE LA ROTATION TERRESTRE ET DES SYSTEMES DE REFERENCE
#
#
# SERVICE DE LA ROTATION TERRESTRE
# OBSERVATOIRE DE PARIS
# 61, Av. de l'Observatoire 75014 PARIS (France)
# Tel.      : 33 (0) 1 40 51 22 26
# FAX       : 33 (0) 1 40 51 22 91
# e-mail    : (E-Mail Removed)
# http://hpiers.obspm.fr/eop-pc
#
# Paris, 5 January 2012
#
#
# Bulletin C 43
#
# To authorities responsible
# for the measurement and
# distribution of time
#
#
# UTC TIME STEP
# on the 1st of July 2012
#
#
# A positive leap second will be introduced at the end of June 2012.
# The sequence of dates of the UTC second markers will be:
#
#                          2012 June 30,     23h 59m 59s
#                          2012 June 30,     23h 59m 60s
#                          2012 July  1,      0h  0m  0s
#
# The difference between UTC and the International Atomic Time TAI is:
#
# from 2009 January 1, 0h UTC, to 2012 July 1  0h UTC  : UTC-TAI = - 34s
# from 2012 July 1,    0h UTC, until further notice    : UTC-TAI = - 35s
#
# Leap seconds can be introduced in UTC at the end of the months of December
# or June, depending on the evolution of UT1-TAI. Bulletin C is mailed every
# six months, either to announce a time step in UTC or to confirm that there
# will be no time step at the next possible date.
#
#
# Daniel GAMBIS
# Head
# Earth Orientation Center of IERS
# Observatoire de Paris, France

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Code Editor : leapseconds