On the forthcoming return of the leonid meteoric swarm

dc.contributor.author	Kondrat'eva E.
dc.contributor.author	Murav'eva I.
dc.contributor.author	Reznikov E.
dc.date.accessioned	2018-09-17T21:47:47Z
dc.date.available	2018-09-17T21:47:47Z
dc.date.issued	1997
dc.identifier.issn	0038-0946
dc.identifier.uri	https://dspace.kpfu.ru/xmlui/handle/net/135447
dc.description.abstract	The Leonid meteoric swarm, which was observed for the last time in 1966, is returning to the Sun, having a period of about 33 years. The increase of the swarm activity has already been noticed. By applying a numerical-simulation technique, an attempt is made to forecast the appearance of the compact portion of the swarm. This portion is related to the comet Tempel-Tuttle, whose orbital elements were used as a basis for calculations. © 1997 MAHK Hayka/Interperiodica Publishing.
dc.relation.ispartofseries	Solar System Research
dc.title	On the forthcoming return of the leonid meteoric swarm
dc.type	Article
dc.relation.ispartofseries-issue	6
dc.relation.ispartofseries-volume	31
dc.collection	Публикации сотрудников КФУ
dc.relation.startpage	489
dc.source.id	SCOPUS00380946-1997-31-6-SID27644547164

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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.