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The fractal analysis of the topography and gravitational field of Venus

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dc.contributor.author Demin S.
dc.contributor.author Andreev A.
dc.contributor.author Demina N.
dc.contributor.author Nefedyev Y.
dc.date.accessioned 2019-01-22T20:47:02Z
dc.date.available 2019-01-22T20:47:02Z
dc.date.issued 2018
dc.identifier.issn 1742-6588
dc.identifier.uri https://dspace.kpfu.ru/xmlui/handle/net/148757
dc.description.abstract © Published under licence by IOP Publishing Ltd. The purpose of this paper is to present the results of structural analysis of gravitational and topographic parameters of Venus using the data from space missions, including "Magellan". The model gravitational potentials are presented as analytical functions of coordinates. The model is constructed on the basis of variations of Venus' artificial satellites orbits. As a result, fractal correlations of Venus' geoid anomalies and gravitational potential in both longitude and latitude as well as the mean value of fractal dimensions are calculated. The mean fractal dimension of Venus topographic model in latitude is D̄= 1.061, in longitude is D̄= 1.037; the mean fractal dimension of Venus gravitational potential model in latitude is D̄= 0.96, in longitude is D̄ = 1.053.
dc.relation.ispartofseries Journal of Physics: Conference Series
dc.title The fractal analysis of the topography and gravitational field of Venus
dc.type Conference Paper
dc.relation.ispartofseries-issue 1
dc.relation.ispartofseries-volume 1038
dc.collection Публикации сотрудников КФУ
dc.source.id SCOPUS17426588-2018-1038-1-SID85049512677


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  • Публикации сотрудников КФУ Scopus [24551]
    Коллекция содержит публикации сотрудников Казанского федерального (до 2010 года Казанского государственного) университета, проиндексированные в БД Scopus, начиная с 1970г.

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