Solar large-scale emitting chains: some CME-associated events

Details Solar large-scale emitting chains: some CME-associated events Solar large-scale emitting chains: some CME-associated events

Nov 2000

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2000jastp..62.1545c&link_type=abstract

Journal of Atmospheric and Solar-Terrestrial Physics, Volume 62, Issue 16, p. 1545-1551.

Physics

3

Scientific paper

Transient large-scale emitting chains and threads, associated with several coronal mass ejections (CMEs), are analyzed by the SOHO//EIT, TRACE, Yohkoh//SXT, Nobeyama Radioheliograph, and some other imaging data. It is illustrated that a pronounced evolution of the chains and threads in the EUV, soft X-ray, microwave, and other ranges can occur many hours both before and after a CME on a considerable part of the solar visible disk, especially near the place of a CME eruption. Such relations between chains and CMEs seem to be plausible due to both phenomena being the consequences of the evolution of large-scale magnetic fields and have often a global character.

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