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Ammonia Abundance at the Galileo Probe Site Derived from Absorption of its Radio Signal

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dc.contributor.author Folkner, W. M. en_US
dc.contributor.author Woo, R. en_US
dc.contributor.author Nandi, S. en_US
dc.date.accessioned 2004-09-25
dc.date.available 2004-09-25
dc.date.issued 1998-09 en_US
dc.identifier.citation Journal of Geophysical Research en_US
dc.identifier.citation USA en_US
dc.identifier.clearanceno 98-1136 en_US
dc.identifier.uri http://hdl.handle.net/2014/20242
dc.description.abstract The radio signal from the Galileo prove to the orbiter experienced attenuation due to ammonia in Jupiter's atmosphere during the probe descent. en_US
dc.format.extent 761968 bytes
dc.format.mimetype application/pdf
dc.language.iso en_US
dc.subject.other Ammonia Jupiter Galileo radio signal en_US
dc.title Ammonia Abundance at the Galileo Probe Site Derived from Absorption of its Radio Signal en_US


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