Structure and development of quiet loops in the solar corona

descriptionPublicationkeyboard_double_arrow_right Article , Part of book or chapter of book , Other literature type 01 Jan 1994 English Publisher:Springer Science and Business Media LLCJournal:Space Science Reviews, volume 70, pages 189-192 (issn: 0038-6308, eissn: 1572-9672,

Copyright policy )

Authors: Eijiro Hiei;

doi: 10.1007/bf00777866 , 10.1017/s0252921100025252 , 10.1007/978-94-011-0930-7_33

Structure and development of quiet loops in the solar corona

- Summary
- Metrics

Abstract

AbstractSolar coronal features seen in X-ray emission change on two different timescales: a) flare loops and transient brightenings in active regions 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.

Related Organizations

Meisei University
Japan

Impact byBIP!

	selected citations These citations are derived from selected sources. This is an alternative to the "Influence" indicator, which also reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).	7
	popularity This indicator reflects the "current" impact/attention (the "hype") of an article in the research community at large, based on the underlying citation network.	Average
	influence This indicator reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).	Top 10%
	impulse This indicator reflects the initial momentum of an article directly after its publication, based on the underlying citation network.	Average