Rapid magnetic reconnection and transient phenomena with particle acceleration in the solar corona

Details Rapid magnetic reconnection and transient phenomena with particle acceleration in the solar corona Rapid magnetic reconnection and transient phenomena with particle acceleration in the solar corona

Apr 1981

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1981izssr..45..576s&link_type=abstract

(Evropeiskii Simpozium po Kosmicheskim Lucham, 7th, Leningrad, USSR, Sept. 15-19, 1980.) Akademiia Nauk SSSR, Izvestiia, Seriia

Physics

3

Current Sheets, Magnetic Field Inversions, Particle Acceleration, Plasma Conductivity, Plasma Turbulence, Solar Corona, Chromosphere, Coronal Loops, Heat Transfer, Magnetohydrodynamic Flow, Solar Magnetic Field, Transient Response

Scientific paper

The paper presents a model for rapid magnetic-field reconfiguration in the solar atmosphere as a result of the reconnection of field lines in a high-temperature current sheet with anomalous conductivity. The model explains the penetration of rising magnetic flux into the upper corona and the rapid 'opening' of the closed magnetic field, and makes it possible to describe three different but related phenomena: coronal transients, transient coronal holes, and particle acceleration in the corona.

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