Astronomy and Astrophysics – Astronomy
Scientific paper
Aug 1999
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1999acasn..40..272s&link_type=abstract
Acta Astron. Sin., Vol. 40, No. 3, p. 272 - 278
Astronomy and Astrophysics
Astronomy
Solar Magnetic Fields: Magnetic Reconnection, Solar Coronal Loops: Magnetic Fields
Scientific paper
By using the finite element method, a partial differential equation (magnetohydrostatic equation) is solved. The plasma presssure and coronal magnetic field of the multipolar active region are determined. The authors have found that the height of the magnetic field lines above the neutral line of strong magnetic field decreases as the magnetic shearing increases. It is believed that the low-lying magnetic loops store eruption energy before solar high energy eruption in the complex multipolar active region. It has also been found that the coronal plasma pressure increases with the magnetic shearing. This implies that the increase of coronal mass density may be the source of coronal mass ejection.
Su Min
Su Qingrui
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