Energy Accumulation for the Bastille Flare

Details Energy Accumulation for the Bastille Flare Energy Accumulation for the Bastille Flare

May 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003aspc..289..397p&link_type=abstract

The Proceedings of the IAU 8th Asian-Pacific Regional Meeting, Volume I, held 2-5 July 2002 at National Center of Sciences, Hito

Astronomy and Astrophysics

Astronomy

Scientific paper

Magnetic field evolution above the NOAA 9077 active region is considered before the flare on 2000 July 14. The system of 3D MHD resistive equations is solved for a compressible plasma. The anisotropy of thermal conductivity in the magnetic field is taken into account. It is shown that a vertical current sheet (CS) appears in the corona due to disturbances that are produced at the photospheric magnetic field changing before the flare. The j x B / c force in the CS can accelerate plasma flux upwards and produce a coronal mass ejection (CME).

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