Some possibilities of microwave diagnostics of eruptive prominences

Details Some possibilities of microwave diagnostics of eruptive prominences Some possibilities of microwave diagnostics of eruptive prominences

Jun 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992angeo..10..354m&link_type=abstract

Annales Geophysicae (ISSN 0992-7689), vol. 10, no. 6, June 1992, p. 354-358.

Physics

2

H Alpha Line, Microwave Emission, Solar Prominences, Solar Radio Emission, Solar Corona, Stellar Mass Ejection

Scientific paper

The relation of a short-duration 'disappearance' of the S-component
source above the active region to H-alpha events is discussed. Assuming
that the cases investigated exhibit coverage of the radio sources by
coronal mass ejections, estimates are made of coronal mass ejection
velocities, dimensions, and optical thicknesses.

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