Magnetic field configurations which can produce prominences with inverse polarity

Details Magnetic field configurations which can produce prominences with inverse polarity Magnetic field configurations which can produce prominences with inverse polarity

Dec 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990soph..130..403a&link_type=abstract

(Committee of European Radio Astronomers, SNSF, URSI, et al., Workshop on Particle Beams in the Solar Atmosphere, Braunwald, Swi

Physics

4

Magnetic Field Configurations, Polarity, Solar Prominences, Magnetic Flux, Solar Activity, Stellar Models

Scientific paper

Several observational aspects of prominences with inverse magnetic
polarity are summarized. It is shown that these features can be
explained in a natural way if inverse polarity prominences result from
the merging of two adjacent bipolar magnetic regions.

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