On the coronal transient-eruptive prominence of 1980 August 5

Details On the coronal transient-eruptive prominence of 1980 August 5 On the coronal transient-eruptive prominence of 1980 August 5

Jun 1981

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1981apj...246l.161f&link_type=abstract

Astrophysical Journal, Part 2 - Letters to the Editor, vol. 246, June 15, 1981, p. L161-L164. NSF-supported research.

Astronomy and Astrophysics

Astrophysics

31

Electron Density (Concentration), Solar Corona, Solar Prominences, H Alpha Line, Ionization, Telescopes

Scientific paper

A coronal transient was observed in association with an eruptive prominence event using the Mauna Loa experiment system. The transient, a rarefaction, formed before the acceleration of the eruptive prominence. Upward velocities of various features, as seen in the plane of the sky, show a marked difference as a function of time between the transient and the eruptive prominence. A region of enhanced electron density formed slowly in front of the rarefaction.

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