Structure and development of quiet loops in the solar corona

Details Structure and development of quiet loops in the solar corona Structure and development of quiet loops in the solar corona

Oct 1994

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994ssrv...70..189h&link_type=abstract

Space Science Reviews, Volume 70, Issue 1-2, pp. 189-192

Physics

Coronal Loop, Solar Corona, X-Ray Image

Scientific paper

X-ray emission from solar coronal loops changes on two different timescales: a) flare loops and transient active region brightenings show a rapid variability, b) quiet region loops are quasi-steady and change only slowly with time. This different time behavior has been analyzed on the basis of Yohkoh SXT observations and we report here on the results from our analysis, mainly focussing on quiet loop variability.

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