Possible observation of a disconnected magnetic structure in a coronal transient

Details Possible observation of a disconnected magnetic structure in a coronal transient Possible observation of a disconnected magnetic structure in a coronal transient

Dec 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983jgr....8810210i&link_type=abstract

Journal of Geophysical Research (ISSN 0148-0227), vol. 88, Dec. 1, 1983, p. 10210-10214.

Other

44

Coronagraphs, Solar Corona, Solar Magnetic Field, Brightness, Coronal Loops, Plasma Dynamics, Polarimetry, Solar Maximum Mission

Scientific paper

The authors present SMM coronagraph/polarimeter observations of the coronal transient of March 15 - 16, 1980, which show a bright front convex toward the sun propagating out through the corona at 175 km s-1. A fan-shaped bright region connecting this front to the inner corona collapses into a narrow bright ray over the next few hours. The authors interpret these observations as resulting from the disconnection of magnetic loops from the underlying prominencelike loop structures seen rising earlier in the event. Other similar "inverted arches" exist in the C/P data but are usually seen with poorer temporal resolution.

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