Magnetic field dynamics and the formation, evolution, and decay of a filament on the sun

Details Magnetic field dynamics and the formation, evolution, and decay of a filament on the sun Magnetic field dynamics and the formation, evolution, and decay of a filament on the sun

Oct 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993azh....70.1099m&link_type=abstract

Astronomicheskij Zhurnal, vol. 70, p. 1099

Astronomy and Astrophysics

Astronomy

1

Solar Magnetic Field, Solar Activity, Polarity, Line Spectra, Magnetic Variations, Plasma Decay

Scientific paper

A study is made of the relationship existing between the magnetic field and the generation, evolution and decay of a dark filament on the sun. It is shown that, during the first stage of its evolution, a filament generated at the outer boundary of the active region penetrated the active region along the polarity inversion line following a decrease in magnetic field at this line. An abrupt increase in the magnetic field at different sections of the polarity inversion line resulted in a sudden disappearance of the entire filament.

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