Radio and visible light observations of matter ejected from the sun

Details Radio and visible light observations of matter ejected from the sun Radio and visible light observations of matter ejected from the sun

Mar 1981

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1981apj...244l.123w&link_type=abstract

Astrophysical Journal, Part 2 - Letters to the Editor, vol. 244, Mar. 15, 1981, p. L123-L126.

Astronomy and Astrophysics

Astronomy

37

Radio Sources (Astronomy), Solar Corona, Solar Flares, Solar Magnetic Field, Solar Maximum Mission, Stellar Mass Ejection, Coronal Loops, Ejecta, Mass Transfer, Radio Observation, Transient Response, Visible Spectrum

Scientific paper

An initial set of visible light and radio observations of a coronal transient made with the Coronagraph/Polarimeter experiment on SMM and the radioheliograph at Culgoora, Australia is presented. It is noted that an enormous loop-shaped transient observed on April 7, 1980, exhibited bright material having whiplike, nonradial motions, as well as moving and stationary radio sources. The data make it possible to establish that a moving type IV radio source was located on or very close to the fast-moving loop. The thermal, kinetic, and magnetic energies in the transient are estimated and, for the first time, compared with the radiative energy of the associated flare.

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