POLAR MOTION AT SEASONAL FREQUENCIES

dc.contributor.authorHopfner J.
dc.date.accessioned2020-11-23T10:55:16Z
dc.date.available2020-11-23T10:55:16Z
dc.date.issued1996
dc.description.abstractStudying the planetary-dynamic behaviour of the Earth connected with geophysical processes as sources of excitation is of particular importance. In order to make a contribution concerning seasonal influences of near-surface geophysical processes on polar motion and Earth rotation, numerical investigations based on a time series of Earth Rotation Parameters and Atmospheric Angular Momentum parameters from 1976 to 1987 were performed. Atmospheric Angular Momentum changes are the dominant cause of polar motion and length-of-day variation at seasonal frequencies. Since there is another excitation source, the problem is to be considered such that the total excitation portion is composed of atmospheric and non-atmospheric portions. Particularly in polar motion, the paper deals with the separation of these portions for the seasonal constituents and presents interesting information about their character.
dc.identifierhttps://elibrary.ru/item.asp?id=593379
dc.identifier.citationJournal of Geodynamics, 1996, , 1, 51-61
dc.identifier.issn0264-3707
dc.identifier.urihttps://repository.geologyscience.ru/handle/123456789/19428
dc.titlePOLAR MOTION AT SEASONAL FREQUENCIES
dc.typeСтатья

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