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Progress in coronal seismology

Published online by Cambridge University Press:  01 September 2007

B. Roberts
B. Roberts*
Affiliation:
Mathematical Institute, University of St Andrews, St Andrews, Fife KY16 9SS, Scotland, UK email: bernie@mcs.st-and.ac.uk
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Abstract

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Coronal seismology is now a well developed area of solar physics, even though many questions remain for resolution. Here we take stock of the progress made since the first direct imaging of oscillating loops was achieved through TRACE spacecraft observations in 1999.

Keywords

Sun: oscillationsMHD wavescoronal seismology
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 3 , Symposium S247: Waves & Oscillations in the Solar Atmosphere: Heating and Magneto-Seismology , September 2007 , pp. 3 - 19
Copyright
Copyright © International Astronomical Union 2008

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