Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/1751
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dc.contributor.authorRajaguru, S. P-
dc.contributor.authorHasan, S. S-
dc.date.accessioned2007-07-27T07:15:27Z-
dc.date.available2007-07-27T07:15:27Z-
dc.date.issued1999-
dc.identifier.citationT. R. Rimmele, K. S. Balasubramaniam, and R. R. Radick., eds., High Resolution Solar Physics: Theory, Observations, and Techniques, ASP Conference Series 183. pp. 53 – 60en
dc.identifier.urihttp://hdl.handle.net/2248/1751-
dc.description.abstractThe effects of radiative energy exchange on the convective instability of a weak field magnetic structure, which lead to a prediction and a physical explanation of the magnetic flux dependent field strength, are examined in detail using a real model stratification for the photospheric and convection zone structure of the Sun. Adopting the generalised Eddington approximation for the radiative transfer, which is valid both in the optically thick and the thin limits, we model the lateral radiative energy exchange by the tube with the external medium with a self-consistent inclusion of vertical radiative losses.en
dc.format.extent1777406 bytes-
dc.format.mimetypeapplication/pdf-
dc.language.isoenen
dc.publisherAstronomical Society of the Pacificen
dc.relation.ispartofseriesASP Conference Series No. 183-
dc.relation.urihttp://adsabs.harvard.edu/abs/1999ASPC..183...53Ren
dc.relation.urihttp://arxiv.org/abs/astro-ph/9901150-
dc.subjectRadiative Transfer Effectsen
dc.subjectConvective Collapseen
dc.subjectSolar Magnetic Flux Tubes-
dc.titleRadiative Transfer Effects and Convective Collapse: Size(flux)-Strength Distribution for the Small-Scale Solar Magnetic Flux Tubesen
dc.typeArticleen
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