Astronomy and Astrophysics – Astrophysics
Scientific paper
Jun 1984
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984acasn..25..376s&link_type=abstract
(Acta Astronomica Sinica, vol. 25, 1985, p. 376-381) Chinese Astronomy and Astrophysics (ISSN 0275-1062), vol. 9, June 1985, p.
Astronomy and Astrophysics
Astrophysics
1
Compressibility Effects, Force-Free Magnetic Fields, Magnetic Effects, Shearing, Solar Flares, Solar Magnetic Field, Gas Pressure, Magnetic Flux, Solar Gravitation
Scientific paper
The corresponding field configurations of the solar isothermal atmosphere obtained from a series of non-constant shearing magnetic fields after considering both the gravity and gas pressure are examined and compared. When the shearing magnetic field increases, magnetic islands will appear, followed by shearing, quasi-three-dimensional field structures approaching the open state, and with almost anti-parallal field lines. It is possible that this is related to the initial phase of a two ribbon flare.
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