Astronomy and Astrophysics – Astrophysics
Scientific paper
Dec 1998
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1998arbes...4..124j&link_type=abstract
Astrophysics Reports, Special Issue, No. 4, p. 124 - 130
Astronomy and Astrophysics
Astrophysics
Solar Wind: Solar Magnetic Fields, Solar Wind: Origin, Solar Wind: Magnetic Reconnection
Scientific paper
The small scale magnetic field reconnections are widely observed on the solar surface. The authors try to study numerically the reconnection of the coronal magnetic field with the magnetic field emergent from the Sun. In the processes of magnetic reconnection, the magnetic energy is converted into the heat energy and plasma kinetic energy in the corona. Through the calculation, one can find the inverse temperature distribution in the base of the corona. In the same time, the plasma in the base of the corona can gain the outflow velocity of about VAlfven. The magnetic energy emergent from the Sun is a reasonable source of coronal heating and the origin of the solar wind.
Jing Hai-rong
Yang Zhiliang
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