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Magnetohydrodynamic waves in solar coronal loops

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Figure

Figure	1.1:	 	The	solar	corona	during	the	total	 solar	 eclipse	 of	 March	 29,	 2006	 (Koen	 van	 Gorp).
Figure	 1.4:	 A	 possible	 mechanism	 for	 the	 excitation	 of	 transverse	 loop	 oscillations	 by	 a	 flare	 (from	 Nakariakov	 &
Figure	3.4:	Plot	of	the	frequency	(left)	and	the	phase	velocity	(right)	for	the	various	wave	modes	supported	by	a	 magnetic	cylinder.
Figure	 3.5:	 Perturbed	 pressure	 and	 displacement	 vector	 for
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