Large-scale electric fields in post-flare loops

Details Large-scale electric fields in post-flare loops Large-scale electric fields in post-flare loops

Sep 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987soph..109..321h&link_type=abstract

Solar Physics (ISSN 0038-0938), vol. 109, no. 2, 1987, p. 321-333.

Physics

3

Coronal Loops, Electrical Resistivity, Solar Atmosphere, Solar Flares, Solar Magnetic Field, Stark Effect, Dynamic Models, Electric Fields, Equations Of Motion, Ion Cyclotron Radiation, Magnetohydrodynamics, Short Circuits

Scientific paper

As the electrical conductivity along the magnetic field in the solar atmosphere is large, parallel electric fields have been neglected in most investigations. The importance of such fields is demonstrated for post-flare loops, and a model for them is introduced which takes into account the effect of parallel electric fields. The electric field calculated from the model is consistent with the electric field observed by Foukal et al. (1983).

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