Magnetic instabilities in solar filements: Models of twisting motions and ejecta

Details Magnetic instabilities in solar filements: Models of twisting motions and ejecta Magnetic instabilities in solar filements: Models of twisting motions and ejecta

Nov 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984esasp.220..273s&link_type=abstract

In ESA The Hydromagnetics of the Sun p 273-274 (SEE N85-25091 14-92)

Astronomy and Astrophysics

Astronomy

2

Ejecta, Solar Magnetic Field, Solar Prominences, Astronomical Models, H Alpha Line, Magnetic Field Configurations, Magnetohydrodynamic Stability, Spectroheliographs

Scientific paper

Time sequences of two destabilized solar filaments were derived using a spectrograph operated in H alpha. The opposite directed velocities observed in the first filament are interpreted in terms of a twisted magnetic flux rope model. The sudden disappearance of the second filament corresponds to high velocity plasmoids confined in magnetic field lines and then ejected.

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