Detection of a slowly moving coronal transient event

Details Detection of a slowly moving coronal transient event Detection of a slowly moving coronal transient event

Jul 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984apj...282l..35f&link_type=abstract

Astrophysical Journal, Part 2 - Letters to the Editor (ISSN 0004-637X), vol. 282, July 1, 1984, p. L35-L37.

Astronomy and Astrophysics

Astrophysics

10

Solar Corona, Solar Wind, Coronagraphs, Solar Wind Velocity, Temporal Distribution

Scientific paper

Data are presented from the K-III coronameter which show the development of a bright coronal structure over a period of 3 hours. Interpreting the upward motion as movement within the plane of the sky, the velocity inferred for the event is 14 km s-1. The amount of material removed from the corona at the site of this event over a period of 24 hours is of the order of 1015 grams. It is concluded that this event was an extremely slow coronal mass ejection transient.

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