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Silicate cooling model fits to Galileo NIMS data of volcanism on IO

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dc.contributor.author Davies, A. en_US
dc.contributor.author Lopes-Gautier, R. en_US
dc.contributor.author Smythe, W. en_US
dc.contributor.author Carlson, R. en_US
dc.date.accessioned 2004-09-23T21:10:16Z
dc.date.available 2004-09-23T21:10:16Z
dc.date.issued 2000-11 en_US
dc.identifier.citation Icarus, v. 148, no. 1, pp.211-225 en_US
dc.identifier.citation Pasadena, CA, USA en_US
dc.identifier.clearanceno 00-1626 en_US
dc.identifier.uri http://hdl.handle.net/2014/15852
dc.description.abstract The Near Infrared Mapping Spectrometer (NIMS) has obtained spectra of volcanoes on the surface of the jovian satellite Io. en_US
dc.format.extent 322652 bytes
dc.format.mimetype application/pdf
dc.language.iso en_US
dc.subject.other Thermal emission lava flow active volcanism sulfur flow en_US
dc.title Silicate cooling model fits to Galileo NIMS data of volcanism on IO en_US


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