Coronal waves: Coronal heating and coronal seismology
UNSPECIFIED (2004) Coronal waves: Coronal heating and coronal seismology. In: 5th Solar-B Science Meeting, NOV 12-14, 2003, Int House Japan, Tokyo, JAPAN.Full text not available from this repository.
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|
|Editor:||Sakurai, T and Sekii, T|
|Number of Pages:||10|
|Page Range:||pp. 253-262|
|Title of Event:||5th Solar-B Science Meeting|
|Location of Event:||Int House Japan, Tokyo, JAPAN|
|Date(s) of Event:||NOV 12-14, 2003|
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