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Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/4289
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dc.contributor.authorVenkatakrishnan, P-
dc.date.accessioned2009-01-28T12:30:09Z-
dc.date.available2009-01-28T12:30:09Z-
dc.date.issued1983-06-
dc.identifier.citationJournal of Astrophysics and Astronomy, vol. 4, No. 2, pp. 135 - 149en
dc.identifier.issn0250-6335-
dc.identifier.urihttp://hdl.handle.net/2248/4289-
dc.description.abstractThe nonlinear development of convective instability within slender flux tubes is studied using the method of characteristics. It is seen that the initial magnetic field influences the development of the instability. The asymptotic state of the unstable tube depends on the boundary conditions. Flux tubes subjected to ’open’ boundary conditions show a better evidence for field amplification than those subjected to ’closed’ boundary conditions. In either case, convective instability results in the generation of significant gas flow within slender flux tubes.en
dc.language.isoenen
dc.publisherIndian Academy of Sciencesen
dc.relation.urihttp://dx.doi.org/10.1007/BF02714204en
dc.relation.urihttp://adsabs.harvard.edu/abs/1983JApA....4..135Ven
dc.subjectAdiabatic Flowen
dc.subjectFlow Stabilityen
dc.subjectSolar Flux Densityen
dc.subjectSolar Magnetic Fielden
dc.subjectAsymptotic Methodsen
dc.subjectFlow Theoryen
dc.subjectMagnetic Field Configurationsen
dc.subjectUnsteady Flowen
dc.subjectSunen
dc.subjectMagnetic Field Sunen
dc.subjectConvection Fluid Dynamicsen
dc.titleNonlinear development of convective instability within slender flux tubes. I - Adiabatic flowen
dc.typeArticleen
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