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Analysis of the topography and gravitational field of venus using space missions data and fractal geometry

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dc.date.accessioned 2019-01-22T20:55:58Z
dc.date.available 2019-01-22T20:55:58Z
dc.date.issued 2018
dc.identifier.uri https://dspace.kpfu.ru/xmlui/handle/net/149483
dc.description.abstract © 2018, American Institute of Aeronautics and Astronautics Inc, AIAA. All rights reserved. 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 D = 1.061, in longitude is D = 1.037; the mean fractal dimension of Venus gravitational potential model in latitude is D = 0.96, in longitude is D = 1.053.
dc.title Analysis of the topography and gravitational field of venus using space missions data and fractal geometry
dc.type Conference Paper
dc.collection Публикации сотрудников КФУ
dc.source.id SCOPUS-2018-SID85056194294


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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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