Structural characteristics of eruptive prominences

Details Structural characteristics of eruptive prominences Structural characteristics of eruptive prominences

Oct 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992soph..141..289d&link_type=abstract

Solar Physics (ISSN 0038-0938), vol. 141, no. 2, p. 289-301.

Physics

Plasma Physics

16

Photosphere, Solar Corona, Solar Flares, Solar Magnetic Field, Solar Prominences, Stellar Mass Ejection, Cold Plasmas, H Alpha Line, Magnetic Field Configurations, Magnetic Field Reconnection, Plasma Density, Plasma Physics, Shock Fronts

Scientific paper

The observed properties of solar prominence eruptions or disparition
brusques are reviewed. The relationships of these properties to coronal
mass ejections and flares are examined using theoretical models. The
importance of magnetic measurements in future coordinated observations
is stressed.

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