Please use this identifier to cite or link to this item:
http://hdl.handle.net/2080/239
Full metadata record
DC Field | Value | Language |
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dc.contributor.author | Sarangi, S K | - |
dc.contributor.author | Margolis, J S | - |
dc.date.accessioned | 2006-02-23T06:57:21Z | - |
dc.date.available | 2006-02-23T06:57:21Z | - |
dc.date.issued | 1978 | - |
dc.identifier.citation | Icarus, Vol 36, Iss 3, P 330-333 | en |
dc.identifier.uri | http://hdl.handle.net/2080/239 | - |
dc.description | Copyright for this article belongs to Elsevier Science Ltd http://dx.doi.org/10.1016/0019-1035(78)90112-4 | en |
dc.description.abstract | A 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.extent | 399992 bytes | - |
dc.format.mimetype | application/pdf | - |
dc.language.iso | en | - |
dc.publisher | Elsevier | en |
dc.title | A determination of Jovian ammonia abundance based on a 2 μm spectrum | en |
dc.type | Article | en |
Appears in Collections: | Journal Articles |
Files in This Item:
File | Description | Size | Format | |
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skso10.pdf | 390.62 kB | Adobe PDF | View/Open |
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