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Is the asymmetric cone model for halo coronal mass ejections correct?

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Is the asymmetric cone model for halo coronal mass ejections correct?

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dc.contributor.author Michałek, Grzegorz [SAP11013973] pl
dc.date.accessioned 2019-05-13T21:36:06Z
dc.date.available 2019-05-13T21:36:06Z
dc.date.issued 2010 pl
dc.identifier.issn 0038-0938 pl
dc.identifier.uri https://ruj.uj.edu.pl/xmlui/handle/item/74509
dc.language eng pl
dc.rights Dodaję tylko opis bibliograficzny *
dc.rights.uri *
dc.title Is the asymmetric cone model for halo coronal mass ejections correct? pl
dc.type JournalArticle pl
dc.description.physical 107-114 pl
dc.subject.en sun: solar activity pl
dc.subject.en sun: coronal mass ejections pl
dc.description.volume 261 pl
dc.description.number 1 pl
dc.identifier.doi 10.1007/s11207-009-9472-0 pl
dc.identifier.eissn 1573-093X pl
dc.title.journal Solar Physics pl
dc.language.container eng pl
dc.affiliation Wydział Fizyki, Astronomii i Informatyki Stosowanej : Instytut – Obserwatorium Astronomiczne pl
dc.subtype Article pl
dc.rights.original bez licencji pl
dc.identifier.project ROD UJ / O pl
.pointsMNiSW [2010 A]: 27


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