Short-period fluctuation analysis of the new BIH LOD series

Details Short-period fluctuation analysis of the new BIH LOD series Short-period fluctuation analysis of the new BIH LOD series

Dec 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988acasn..29..113d&link_type=abstract

(Acta Astronomica Sinica, vol. 29, 1988, p. 113-117) Chinese Astronomy and Astrophysics (ISSN 0275-1062), vol. 12, Dec. 1988, p.

Astronomy and Astrophysics

Astrophysics

Solar Terrestrial Interactions, Tides, Daytime, Iterative Solution, Least Squares Method, Periodic Variations, Sidereal Time, Universal Time

Scientific paper

The short-period tidal fluctuations in the length of day series reduced by Li (1986) are analyzed using the Marple (1980) algorithm. The results show sharp peaks at 13.652, 27.586, and 31.746 days. The amplitudes of these peaks are calculated and compared with the results of Robertson et al. (1985). The elastic deformation parameter at the fortnightly and monthly frequencies is found to be 0.56 + or - 0.21 and 0.89 + or - 0.21, respectively.

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