The dynamics of solar flares - The ascending stage of solar flares

Details The dynamics of solar flares - The ascending stage of solar flares The dynamics of solar flares - The ascending stage of solar flares

Jun 1979

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1979acasn..20..143c&link_type=abstract

Acta Astronomica Sinica, vol. 20, June 1979, p. 143-152. In Chinese, with abstract in English.

Astronomy and Astrophysics

Astronomy

6

Gas Explosions, Ion Motion, Plasma Dynamics, Solar Flares, Solar Magnetic Field, Stellar Models, Atmospheric Models, Current Sheets, Deceleration, Gas Expansion, Lines Of Force, Magnetohydrodynamic Stability, Particle Acceleration, Solar Atmosphere

Scientific paper

The mechanism of plasma ejection due to the reconnection of solar magnetic field lines in local unstable regions of the solar atmosphere is investigated in order to explain the ascending stage of solar flares. A model based on Maxwellian stresses of such reconnected field lines in neutral current sheets and the explosive expansion of ionized gases is used to effectively interpret the dynamics involved in the acceleration and deceleration of the ascending front of solar flare plasma ejection.

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