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Theoretical Models for the Magnetic Field Distribution of Bipolar Regions in the Solar Corona.
Author(s) -
Ludwig Oster
Publication year - 1962
Publication title -
the astronomical journal
Language(s) - English
Resource type - Journals
SCImago Journal Rank - 2.61
H-Index - 271
eISSN - 1538-3881
pISSN - 0004-6256
DOI - 10.1086/108783
Subject(s) - physics , corona (planetary geology) , nanoflares , astrophysics , astronomy , magnetic field , distribution (mathematics) , coronal mass ejection , solar wind , astrobiology , mathematics , quantum mechanics , venus , mathematical analysis

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