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A Three‐dimensional Line‐tied Magnetic Field Model for Solar Eruptions
Author(s) -
Philip A. Isenberg,
T. G. Forbes
Publication year - 2007
Publication title -
the astrophysical journal
Language(s) - English
Resource type - Journals
SCImago Journal Rank - 2.376
H-Index - 489
eISSN - 1538-4357
pISSN - 0004-637X
DOI - 10.1086/522025
Subject(s) - physics , rope , magnetic flux , corona (planetary geology) , flux (metallurgy) , magnetic field , instability , field line , toroid , torus , magnetic cloud , coronal mass ejection , rotation (mathematics) , mechanics , astrophysics , solar wind , plasma , geometry , mathematics , quantum mechanics , materials science , structural engineering , astrobiology , venus , engineering , metallurgy

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