Physics
Scientific paper
Feb 2004
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004asthe..97..107n&link_type=abstract
The Astronomical Herald (ISSN 0374-2466), Vol. 97, No. 2, p. 107 - 117 (2004)
Physics
4
Magnetic Reconnection, Solar Flares
Scientific paper
Magnetic reconnection is a kind of engine process which releases an enormous magnetic energy through the "reconnection" of magnetic field lines. This process is universal in plasma systems, and widely appears in astrophysical phenomena. Magnetic reconnection is famous for an elementary process of solar flares and the geomagnetospheric substorms which are related to the space-weather. In spite of its popularity and importance, any suitable model which is specified as an astrophysical model has not been established yet. We considered an astro-physics-oriented reconnection model, and established "self-similarly evolving model of magnetic reconnection". We expect that this new model will be inspected by the next solar mission "Solar-B".
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