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Solutions of the equation of heat flowThe geometry of sunspots has been used to suggest a problem in heat flow. The equation of heat transport is solved for the case of a cylinder with a given thermal conductivity imbedded in an otherwise uniform medium with different conductivity. The surface of this region radiates heat with flux proportional to temperature. At a lower surface, either in heat flux or temperature is held constant. The cylinder can have an anisotropic thermal conductivity. The variations in temperature along the radiating surface have been determined. A simple approximation is noted which has been found to give a general solution with acceptable accuracy. This method may be of some use in other situations requiring the solution of Laplace's equation with a free surface. The analysis is used to set limits on the ratio of diameter to depth for cases which preserve the sharp surface temperature transition across the cylinder.
Document ID
19810027876
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
Authors
Margolis, S. H.
(Harvard-Smithsonian Center for Astrophysics Cambridge, MA, United States)
Knobloch, E.
(Harvard-Smithsonian Center for Astrophysics Cambridge, Mass., United States)
Date Acquired
August 11, 2013
Publication Date
November 1, 1980
Publication Information
Publication: Royal Astronomical Society
Subject Category
Solar Physics
Accession Number
81A12280
Funding Number(s)
CONTRACT_GRANT: NSF AST-78-20392
CONTRACT_GRANT: NSG-7212
CONTRACT_GRANT: NSF AST-76-20255
CONTRACT_GRANT: NSF AST-76-20253
CONTRACT_GRANT: NSF AST-76-21707
Distribution Limits
Public
Copyright
Other

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