Wave propagation in solar magnetic tubes

Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/315

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DC Field	Value	Language
dc.contributor.author	Venkatakrishnan, P	-
dc.date.accessioned	2005-02-04T16:35:38Z	-
dc.date.available	2005-02-04T16:35:38Z	-
dc.date.issued	1981-09	-
dc.identifier.citation	BASI, Vol. 9, No. 3, pp. 214-226	en
dc.identifier.uri	http://hdl.handle.net/2248/315	-
dc.description.abstract	The work done on propagation of waves in magnetic tubes is reviewed. It is seen that majority of the results obtained so far are based on the thin tube approximation. It is shown that estimates of the mechanical energy flux based on such an approximation could be grossly in error. The need for studying the propagation of waves in finite tubes is emphasised. The possibility of non-linear effects altering the propagation characteristics of these waves is pointed out.	en
dc.format.extent	1219431 bytes	-
dc.format.mimetype	application/pdf	-
dc.language.iso	en	-
dc.publisher	Astronomical Society of India	en
dc.subject	sun	en
dc.subject	small scale magnetic fields	en
dc.subject	wave propagation	en
dc.subject	heating of chromosphere and corona	en
dc.title	Wave propagation in solar magnetic tubes	en
dc.type	Article	en
Appears in Collections:	BASI Publications

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