The observation of a high-latitude coronal transient

Details The observation of a high-latitude coronal transient The observation of a high-latitude coronal transient

Jun 1980

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980apj...238l.161s&link_type=abstract

Astrophysical Journal, Part 2 - Letters to the Editor, vol. 238, June 15, 1980, p. L161-L164.

Astronomy and Astrophysics

Astronomy

11

Solar Activity, Solar Corona, Solar Physics, Stellar Mass Ejection, Spaceborne Astronomy, Surges

Scientific paper

On 1979 September 27 NRL's earth-orbiting coronagraph (Solwind) observed a coronal mass ejection whose outward direction in the plane of the sky was within 12 deg of the sun's north polar axis. Such high-latitude transients were not observed by the OSO 7 and Skylab coronagraphs during the declining phase of the last sunspot cycle, but may be relatively common near sunspot maximum.

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