Open AccessA Possible Structure of the Magnetic Field in Solar Filaments Obtained by Flux Emergence
Author(s) -
Tetsuya Magara
Publication year - 2007
Publication title -
publications of the astronomical society of japan
Language(s) - English
Resource type - Journals
SCImago Journal Rank - 1.99
H-Index - 110
eISSN - 2053-051X
pISSN - 0004-6264
DOI - 10.1093/pasj/59.6.l51
Subject(s) - protein filament , physics , flux tube , magnetic flux , magnetic field , coronal loop , flux (metallurgy) , solar prominence , coronal mass ejection , helmet streamer , astrophysics , solar wind , materials science , composite material , metallurgy , quantum mechanics
Accelerating Research
Robert Robinson Avenue,
Oxford Science Park, Oxford
OX4 4GP, United Kingdom
Address
John Eccles HouseRobert Robinson Avenue,
Oxford Science Park, Oxford
OX4 4GP, United Kingdom