Atmospheric Excitation and Variations in the Length of Day
Publications of the Department of Astronomy, Tome 17 (1989), p. 37 .

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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 $\chi_{3}$).
Keywords: atmospheric excitation, length of day
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     author = {N. Pejovi\'c},
     title = {Atmospheric {Excitation} and {Variations} in the {Length} of {Day}},
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     volume = {17},
     year = {1989},
     language = {en},
     url = {http://geodesic.mathdoc.fr/item/PDA_1989_17_a3/}
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N. Pejović. Atmospheric Excitation and Variations in the Length of Day. Publications of the Department of Astronomy, Tome 17 (1989), p. 37 . http://geodesic.mathdoc.fr/item/PDA_1989_17_a3/