A determination of Jovian ammonia abundance based on a 2 μm spectrum

Please use this identifier to cite or link to this item: http://hdl.handle.net/2080/239

Full metadata record

DC Field	Value	Language
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
skso10.pdf		390.62 kB	Adobe PDF	View/Open