Evidence for downflow following a coronal transient

Details Evidence for downflow following a coronal transient Evidence for downflow following a coronal transient

Jun 1975

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1975soph...42..391h&link_type=abstract

Solar Physics, vol. 42, June 1975, p. 391-394.

Physics

1

K Lines, Solar Corona, Solar Prominences, Spectrograms, H Alpha Line, Solar Limb, Solar Spectrometers, Spectral Line Width, Stellar Mass Ejection

Scientific paper

On 11 September 1973 a peculiar prominence was observed. The prominence
displayed strong (approximately 50 km per sec) systematic motions toward
and away from the observer. The unusual spectrographic appearance of the
prominence might have been due to downflowing material lifted into the
corona during an earlier coronal transient.

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