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It is also important to keep the Earth orientation parameters up to date. This is done by downloading the eopc04_IAU2000.62-now from http://hpiers.obspm.fr/iers/eop/eopc04_05/ to $TEMPO2/earth directory.
51079 311508 311555 311604 311698 311769 311837 51109 311908 311969 312052 312148 312221 312295 51139 312361 312427 312516 312579 312636 312686 51169 312720 312775 0 0 0 0 2 END format for final entry (if incomplete): 48949 268419 268505 268590 268675 268760 0 5 END Last entry: B.131Columns 2 to 7 list the UT1R-TAI corrections in units of 0.1 ms. The following key may be useful in explaining the format of this file.
51139 312361 312427 312516 312579 312636 312686 UT date correction correction ... ... ... correction at MJD 51139 at MJD 51144 at MJD 51164
%getut1 B.nnnThis produces a file ut1.tmp in the iers directory.
NOTE: Some messing around is necessary after a leap second has been introduced. First, getut1 is run on the B bulletin which contains the leap second adjustment and ut1.tmp saved. The value of nleap (= TAI-UTC) in the file $clkcorrdir/iers/iers.awk must then be adjusted to the new value of TAI-UTC (it is usually increased by 1; the current value is listed in Circular T). Then getut1 is run on the same B bulletin and ut1.tmp concatenated with the saved ut1.tmp. The concatenated file must then be edited to have a unique and correct value of the offset for each time. Offsets before the leap sec will be correct in the first file and offsets after the leap sec will be correct in the second file.
Please report errors or problems with these clock correction procedures to Dick Manchester.