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Modeling of the physical selenocentric surface using modern satellite observations and harmonic analysis methods

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dc.contributor.author Andreev A.
dc.contributor.author Demina N.
dc.contributor.author Nefedyev Y.
dc.contributor.author Demin S.
dc.contributor.author Zagidullin A.
dc.date.accessioned 2019-01-22T20:47:03Z
dc.date.available 2019-01-22T20:47:03Z
dc.date.issued 2018
dc.identifier.issn 1742-6588
dc.identifier.uri https://dspace.kpfu.ru/xmlui/handle/net/148759
dc.description.abstract © Published under licence by IOP Publishing Ltd. On the basis of satellite observations taken during "Apollo", "Clementine", "Kaguya", "LRO", "GRAIL", and "SMART-1" space missions a model of lunar physical surface of 18th order of expansion into a series of harmonic coefficients was constructed. In order to expand the data on relief into spherical functions a step-by-step regression was applied. All the constructed models included only significant elements. The regression analysis of the models of lunar relief for various expansion orders was carried out; as a result, it was determined that increase in order of expansion did not play a prominent role from a certain stage. The influence of model's overdetermined structure on values of the parameters determined was also investigated.
dc.relation.ispartofseries Journal of Physics: Conference Series
dc.title Modeling of the physical selenocentric surface using modern satellite observations and harmonic analysis methods
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-SID85049518242


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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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