POLAR MOTION AT SEASONAL FREQUENCIES

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dc.contributor.author Hopfner J.
dc.date.accessioned 2020-11-23T10:55:16Z
dc.date.available 2020-11-23T10:55:16Z
dc.date.issued 1996
dc.identifier https://elibrary.ru/item.asp?id=593379
dc.identifier.citation Journal of Geodynamics, 1996, , 1, 51-61
dc.identifier.issn 0264-3707
dc.identifier.uri https://repository.geologyscience.ru/handle/123456789/19428
dc.description.abstract Studying 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.title POLAR MOTION AT SEASONAL FREQUENCIES
dc.type Статья


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