Remarks on the magnetic support of quiescent prominences

Details Remarks on the magnetic support of quiescent prominences Remarks on the magnetic support of quiescent prominences

Feb 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985soph...95..263a&link_type=abstract

Solar Physics (ISSN 0038-0938), vol. 95, Feb. 1985, p. 263-268. Research supported by the Science and Engineering Research Counc

Physics

18

Solar Magnetic Field, Solar Prominences, Current Sheets, Magnetic Field Configurations

Scientific paper

The development of magnetic field structures which can lead to prominence configurations of the Kuperus-Raadu type is discussed. Starting from streamer type configurations and preserving the total current in the system the authors find that simple two-dimensional static configurations lead to prominences which in general lie systematically much lower than the heights found from observations. It is therefore concluded that either more complex field configurations are needed to explain the recent observations by Leroy et al. (1983) or the initial configurations must be very special.

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