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Io's Heat Flow From Infrared Radiometry: 1983-1993

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dc.contributor.author Veeder, G. en_US
dc.contributor.author Matson, D. en_US
dc.contributor.author Johnson, T. en_US
dc.contributor.author Blaney, D. en_US
dc.contributor.author Goguen, J. en_US
dc.date.accessioned 2004-10-05T06:23:33Z
dc.date.available 2004-10-05T06:23:33Z
dc.date.issued 1994
dc.identifier.clearanceno 94-1381
dc.identifier.uri http://hdl.handle.net/2014/33536
dc.description.abstract This paper presents results from a decade of infrared radiometry of IO. Results indicated that a new thermophysical model is required to match all the data. The thermal anomalies are modeled with a total of 10 source components at five locations. en_US
dc.format.extent 3279515 bytes
dc.format.mimetype application/pdf
dc.language.iso en_US
dc.subject.other Io en_US
dc.title Io's Heat Flow From Infrared Radiometry: 1983-1993 en_US


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