Please use this identifier to cite or link to this item: http://hdl.handle.net/2080/239
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dc.contributor.authorSarangi, S K-
dc.contributor.authorMargolis, J S-
dc.date.accessioned2006-02-23T06:57:21Z-
dc.date.available2006-02-23T06:57:21Z-
dc.date.issued1978-
dc.identifier.citationIcarus, Vol 36, Iss 3, P 330-333en
dc.identifier.urihttp://hdl.handle.net/2080/239-
dc.descriptionCopyright for this article belongs to Elsevier Science Ltd http://dx.doi.org/10.1016/0019-1035(78)90112-4en
dc.description.abstractA spectrum of Jupiter in the two micron region has been analyzed to determine the Jovian ammonia abundance. The result is a 4 cm - amagat, assuming an airmass factor η = 2.5 and a single effective reflecting layer for this wavelength. This is compared with the abundances observed at other wavelengths.en
dc.format.extent399992 bytes-
dc.format.mimetypeapplication/pdf-
dc.language.isoen-
dc.publisherElsevieren
dc.titleA determination of Jovian ammonia abundance based on a 2 μm spectrumen
dc.typeArticleen
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