Magnetohydrodynamic waves in dynamic plasmas with solar applications : effect of thermal conduction
The highly magnetised coronal loops have been confirmed to support a variety of MHD waves and oscillations which are observed widely in the solar atmosphere and most of them are seen to be rapidly damped. One of these oscillations are interpreted as longitudinal slow (propagating or standing) MHD wa...
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University of Sheffield
2013
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| Online Access: | http://ethos.bl.uk/OrderDetails.do?uin=uk.bl.ethos.572385 |