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Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/4209
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dc.contributor.authorVenkatakrishnan, P-
dc.date.accessioned2008-12-30T11:21:08Z-
dc.date.available2008-12-30T11:21:08Z-
dc.date.issued1979-08-
dc.identifier.citationSolar Physics, Vol. 63, pp. 135 - 141en
dc.identifier.issn00038-0938-
dc.identifier.urihttp://hdl.handle.net/2248/4209-
dc.description.abstractWhen 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.isoenen
dc.publisherD. Reidel Publishing Co.en
dc.relation.urihttp://adsabs.harvard.edu/abs/1979SoPh...63..135Ven
dc.relation.urihttp://www.springerlink.com/content/u82377u04480035w/en
dc.rights© D. Reidel Publishing Co.en
dc.subjectMagnetic Fluxen
dc.subjectMagnetoacousticsen
dc.subjectMagnetohydrodynamic Stabilityen
dc.subjectPlasma Sheathsen
dc.subjectSolar Atmosphereen
dc.subjectSolar Magnetic Fielden
dc.subjectFrequency Responseen
dc.subjectMagnetoacoustic Wavesen
dc.subjectMagnetohydrodynamic Wavesen
dc.subjectSound Wavesen
dc.subjectWave Interactionen
dc.titleFrequency response of magnetic flux sheathsen
dc.typeArticleen
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