Atmospheric Excitation and Variations in the Length of Day
Publications of the Department of Astronomy, Tome 17 (1989) no. 1
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The LOD (length of day) and $X3 spectra were computed using the maximum entropy method (MEM). The comparisons show excellent correlation between the axial component of the atmospheric EAMF ($\chi_{3}$) and the changes in the Earth's rotation rate corrected for the effects of the lunar and solar tides. The most important changes are the seasonal variations with annual and semi-annual periods, and a cluster of small peaks with periods between 40 and 70 days i both spectra (LOD and $\chi_{3}$).
@article{PDA_1989_17_1_a3,
author = {N. Pejovi\'c},
title = {Atmospheric {Excitation} and {Variations} in the {Length} of {Day}},
journal = {Publications of the Department of Astronomy},
pages = {37 - 50},
publisher = {mathdoc},
volume = {17},
number = {1},
year = {1989},
url = {http://geodesic.mathdoc.fr/item/PDA_1989_17_1_a3/}
}
N. Pejović. Atmospheric Excitation and Variations in the Length of Day. Publications of the Department of Astronomy, Tome 17 (1989) no. 1. http://geodesic.mathdoc.fr/item/PDA_1989_17_1_a3/