Jasové profily kóm komet jako důsledek procesů disociace a ionizace v atmosférách komet

dc.contributor.author	Zahrádka, Jaromír
dc.date.accessioned	2009-03-12T15:56:05Z
dc.date.available	2009-03-12T15:56:05Z
dc.date.issued	1999
dc.identifier	Univerzitní knihovna (studovna)	cze
dc.identifier.issn	1211-555X
dc.identifier.uri	http://hdl.handle.net/10195/32196
dc.description.abstract	This paper present three bases gaseous models of the comet atmospheres. The models are able elucidate the surface brightness courses of the comet comas. 1. The comet atmosphere which is created by brigftness molecules coming out directly from the nucleus of the comet. 2. The comet atmosphere created by dissociating brightness molecules which arise from the parent molecules which come out from the nucleus of the comet. 3. The comet atmosphere created by brightness molecules which do not dissociate.	eng
dc.format	s. 407-412	cze
dc.format	p. 407-412	eng
dc.format.extent		cze
dc.format.mimetype		cze
dc.language.iso	cze
dc.publisher	Univerzita Pardubice	cze
dc.relation.ispartof	Scientific papers of the University of Pardubice. Series D Faculty of Economics and Administration. 4 (1999)	eng
dc.rights		cze
dc.subject	astronomie	cze
dc.subject	komety	cze
dc.subject	atmosféra	cze
dc.subject	atmosférické procesy	cze
dc.subject	ionizace	cze
dc.title	Jasové profily kóm komet jako důsledek procesů disociace a ionizace v atmosférách komet	cze
dc.type	Article	eng
dc.identifier.signature	47940
dc.peerreviewed	yes	eng
dc.publicationstatus	published	eng