A twisted flux model for solar prominences. II - Formation of a dip in a magnetic structure before the formation of a solar prominence

Details A twisted flux model for solar prominences. II - Formation of a dip in a magnetic structure before the formation of a solar prominence A twisted flux model for solar prominences. II - Formation of a dip in a magnetic structure before the formation of a solar prominence

Apr 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989a%26a...214..360d&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 214, no. 1-2, April 1989, p. 360-368. Research supported by SERC.

Astronomy and Astrophysics

Astrophysics

37

Solar Magnetic Field, Solar Prominences, Chromosphere, Cold Plasmas, Magnetic Flux, Polarity

Scientific paper

The possibility of dip formation in a linear force-free field before the
formation of a filament is investigated. The creation of a dip prior to
prominence formation requires a greatly sheared magnetic field and a
particular magnetic base flux. In the present work, attention is given
to a bipolar region devoid of parasite polarity.

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