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Short-Period Oscillations of Earth Rotation

Published online by Cambridge University Press:  12 April 2016

B. Kołaczek ,
W. Kosek  and
H. Schuh
B. Kołaczek
Affiliation:
Space Research Centre, PAS Warsaw, Poland
W. Kosek
Affiliation:
Space Research Centre, PAS Warsaw, Poland
H. Schuh
Affiliation:
Deutsches Geodätisches Forschungsinstitut, DGFI München, Germany

Abstract

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Sub-seasonal variations and especially sub-seasonal oscillations with periods of about 120, 60, 50, 40 days in polar motion and of about 120, 60–90, and 50 days in LOD are presented. Variations of amplitudes of these sub-seasonal oscillations of polar motion are shown. Maxima of these amplitudes are of the order of 2–4 mas. These oscillations are elliptical ones. The correlation coefficients between geodetic and atmospheric excitation functions in this range of the spectrum are variable and have annual variations. Maxima of correlation coefficients are of the order of 0.6–0.8.

Modern geodetic VLBI experiments provide very accurate results in polar motion and UT1–UTC with a temporal resolution of 3–7 minutes. Several irregular, quasi-periodic variations were found. In many UT1–UTC data sets, oscillations with periods around 8 hours and between 5 and 7 hours can be seen.

Type
Part 6. Daily and Subdaily Polar Motion
Information
International Astronomical Union Colloquium , Volume 178: Polar Motion: Historical and Scientific Problems , 2000 , pp. 533 - 544
Copyright
Copyright © Astronomical Society of the Pacific 2000

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