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MHD waves and oscillations in the solar plasma

Observational and theoretical progress in studies of wave phenomena in the solar plasma.

fine scale structure in the solar atmosphereThe Sun's magnetic field is responsible for many spectacular phenomena. Recently our understanding of the solar corona has been significantly improved by the direct detection, by TRACE and SOHO, of waves. The new subject of coronal seismology is rapidly developing. We aim to address recent observational and theoretical progress in studies of wave phenomena in the solar plasma.


Professor Robert von Fay-Siebenburgen (Erdelyi) | talks
Professor Michael Thompson | talks
Professor Michael Ruderman | talks
Professor Bernard Roberts | talks


Date and Time:

14 March 2005 at 9:30 am


Full Day



The Royal Society
6-9 Carlton House Terrace
+44 20 74 51 2500

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