Magneto-seismology : the influence of the properties of solar waveguides on MHD wave propagation
The ubiquitous nature of magnetohydrodynamic (MHD) waves and oscillations resolved in magnetic structures in the solar atmosphere is beginning to be documented. To date, the majority of the waves predicted by theory, i.e. the theory of (MHD) waves in a cylindrical, magnetic waveguide, have been obse...
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University of Sheffield
2010
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| Online Access: | http://ethos.bl.uk/OrderDetails.do?uin=uk.bl.ethos.557119 |