Frequency response of magnetic flux sheaths

dc.contributor.author	Venkatakrishnan, P
dc.date.accessioned	2008-12-30T11:21:08Z
dc.date.available	2008-12-30T11:21:08Z
dc.date.issued	1979-08
dc.identifier.citation	Solar Physics, Vol. 63, pp. 135 - 141	en
dc.identifier.issn	00038-0938
dc.identifier.uri	http://hdl.handle.net/2248/4209
dc.description.abstract	When a sound wave is incident on a magnetic flux sheath, it causes fluctuations in the mean magnetic field of the sheath. We have calculated the space-average of the longitudinal component of these fluctuations and plotted this against the frequency of the incident sound wave. The main result is the presence of local maxima and minima in the response curve. If such maxima and minima could be detected in any actual observation then these would provide an estimate of the thickness of these magnetic structures.	en
dc.language.iso	en	en
dc.publisher	D. Reidel Publishing Co.	en
dc.relation.uri	http://adsabs.harvard.edu/abs/1979SoPh...63..135V	en
dc.relation.uri	http://www.springerlink.com/content/u82377u04480035w/	en
dc.rights	© D. Reidel Publishing Co.	en
dc.subject	Magnetic Flux	en
dc.subject	Magnetoacoustics	en
dc.subject	Magnetohydrodynamic Stability	en
dc.subject	Plasma Sheaths	en
dc.subject	Solar Atmosphere	en
dc.subject	Solar Magnetic Field	en
dc.subject	Frequency Response	en
dc.subject	Magnetoacoustic Waves	en
dc.subject	Magnetohydrodynamic Waves	en
dc.subject	Sound Waves	en
dc.subject	Wave Interaction	en
dc.title	Frequency response of magnetic flux sheaths	en
dc.type	Article	en