Prominence motions and their implications for magnetic fields

Details Prominence motions and their implications for magnetic fields Prominence motions and their implications for magnetic fields

Jan 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984soph...90...37b&link_type=abstract

Solar Physics (ISSN 0038-0938), vol. 90, Jan. 1984, p. 37-40.

Physics

11

Solar Magnetic Field, Solar Prominences, Electrohydrodynamics, Equipartition Theorem, Magnetic Field Configurations, Magnetic Flux, Plasma Currents

Scientific paper

Using results obtained in Ballester and Kleczek (1983) and the equipartition principle, an attempt is made to calculate the lower limits of magnetic fields in three solar prominences. The values are then compared with the magnetic fields found by experimental methods. Furthermore, Ampere's law was used to calculate the lower limits of electric currents inside the conical surface where the knot's motion is located. The results obtained are compared with a few deteminations of electric currents in prominences. An attempt is made to use a three-currents system to explain the configuration of magnetic fields in solar prominences.

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