Tomographic method for meteor-flux determination from radar observations

dc.contributor.author	Belkovich O.
dc.contributor.author	Sidorov V.
dc.contributor.author	Filimonova T.
dc.contributor.author	Nugmanov I.
dc.date.accessioned	2018-09-17T21:47:44Z
dc.date.available	2018-09-17T21:47:44Z
dc.date.issued	1997
dc.identifier.issn	0038-0946
dc.identifier.uri	https://dspace.kpfu.ru/xmlui/handle/net/135446
dc.description.abstract	Potentialities of the tomographic method are studied as this method used to determine the density distribution of the sporadic-meteor flux over the celestial sphere from radar observations with measuring radiowave-arrival angles. It is shown that the main features of the distributions obtained by this method are the same as those obtained by other methods but that the angular resolution is much higher. © 1997 MAHK Hayka /Interperiodica Publishing.
dc.relation.ispartofseries	Solar System Research
dc.title	Tomographic method for meteor-flux determination from radar observations
dc.type	Article
dc.relation.ispartofseries-issue	6
dc.relation.ispartofseries-volume	31
dc.collection	Публикации сотрудников КФУ
dc.relation.startpage	477
dc.source.id	SCOPUS00380946-1997-31-6-SID21944437022

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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.