UNSPECIFIED (2004) Coronal waves: Coronal heating and coronal seismology. In: 5th Solar-B Science Meeting, NOV 12-14, 2003, Int House Japan, Tokyo, JAPAN.

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Abstract

SOHO and TRACE missions have demonstrated that wave phenomena are abundant in the corona and provided us with an observational basis for MHD coronal seismology. This review covers the recent observational finding of coronal wave phenomena and their theoretical models. The relevance of these observational and theoretical efforts to the coronal. heating is discussed. Possible observability of these phenomena with EIS and XRT instruments is discussed.

Item Type:	Conference Item (UNSPECIFIED)
Subjects:	Q Science > QB Astronomy
Series Name:	ASTRONOMICAL SOCIETY OF THE PACIFIC CONFERENCE SERIES
Journal or Publication Title:	Solar-B Mission and the Forefront of Solar Physics, Proceedings
Publisher:	ASTRONOMICAL SOC PACIFIC
ISBN:	1-58381-187-7
Editor:	Sakurai, T and Sekii, T
Date:	2004
Volume:	325
Number of Pages:	10
Page Range:	pp. 253-262
Publication Status:	Published
Title of Event:	5th Solar-B Science Meeting
Location of Event:	Int House Japan, Tokyo, JAPAN
Date(s) of Event:	NOV 12-14, 2003
URI:	http://wrap.warwick.ac.uk/id/eprint/34202

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