A study of the material motion into an eruptive prominence

Details A study of the material motion into an eruptive prominence A study of the material motion into an eruptive prominence

Nov 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984esasp.220..243p&link_type=abstract

In ESA The Hydromagnetics of the Sun p 243-244 (SEE N85-25091 14-92)

Physics

Magnetic Field Configurations, Solar Magnetic Field, Solar Prominences, Coronal Loops, Densitometers, H Alpha Line, Solar Limb

Scientific paper

The time evolution of the material motion into an eruptive prominence was studied. The observational material was obtained with an H alpha filter. Isodensity map contours were used to formulate the geometrical structure of the loops and to describe the material motion through them. Twisting of the material flow along the loop was studied. Interpretation of such a phenomenon by considering the visible trajectory as describing the magnetic skeleton in the coronal space is proposed.

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