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Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/3803
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dc.contributor.authorVenkatakrishnan, P-
dc.date.accessioned2008-09-23T09:53:32Z-
dc.date.available2008-09-23T09:53:32Z-
dc.date.issued1986-04-
dc.identifier.citationSolar Physics, Vol. 104, No. 2, pp. 347 - 357en
dc.identifier.issn0038-0938-
dc.identifier.urihttp://hdl.handle.net/2248/3803-
dc.description.abstractThe effect of applying external pressure fluctuations on slender flux tubes is studied as a nonlinear initial value problem. It is shown that persistent nonlinear resonant response to pressure fluctuations is possible for slender magnetic flux tubes. Radiation does not seem to significantly damp the resonance for forcing periods much larger than the cooling time. Thus, the absence of observational evidence for resonant interaction between the narrow band five-minute oscillations and the tubes seems to indicate that the tubes are shorter than the extent of the eigenfunction of the oscillations.en
dc.language.isoenen
dc.publisherSpringeren
dc.relation.urihttp://dx.doi.org/10.1007/BF00159087en
dc.relation.urihttp://adsabs.harvard.edu/abs/1986SoPh..104..347V-
dc.subjectMagnetic Fluxen
dc.subjectPhotosphereen
dc.subjectPressure Effectsen
dc.subjectSolar Magnetic Fielden
dc.subjectBoundary Value Problemsen
dc.subjectCoolingen
dc.subjectOscillationsen
dc.subjectResonant Frequenciesen
dc.titleNonlinear response of slender magnetic flux tubes to external pressure fluctuationsen
dc.typeArticleen
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