๐”– Bobbio Scriptorium
โœฆ   LIBER   โœฆ

Hydrocarbons and eddy mixing in Neptune's atmosphere

โœ Scribed by S.K. Atreya

Publisher
Elsevier Science
Year
1992
Tongue
English
Weight
508 KB
Volume
12
Category
Article
ISSN
0273-1177

No coin nor oath required. For personal study only.

๐Ÿ“œ SIMILAR VOLUMES

The Origin of Carbon Monoxide in Neptune
The Origin of Carbon Monoxide in Neptune's Atmosphere
โœ K. Lodders; B. Fegley Jr. ๐Ÿ“‚ Article ๐Ÿ“… 1994 ๐Ÿ› Elsevier Science ๐ŸŒ English โš– 370 KB

The \(\mathrm{CO}\) abundance in the observable atmosphere of Neptune can be plausibly explained by rapid vertical mixing from the deeper atmosphere if Neptune has a greater complement of water than Uranus. Thermochemical equilibrium and kinetic calculations reveal that Neptune must and Uranus may h

Chlorinated Hydrocarbons in the Atmosphe
Chlorinated Hydrocarbons in the Atmosphere
โœ Dr. Anders Laveskog; Anne Lindskog ๐Ÿ“‚ Article ๐Ÿ“… 1976 ๐Ÿ› John Wiley and Sons ๐ŸŒ German โš– 109 KB
Neptune's Atmospheric Circulation and Cl
Neptune's Atmospheric Circulation and Cloud Morphology: Changes Revealed by 1998 HST Imaging
โœ L.A. Sromovsky; P.M. Fry; T.E. Dowling; K.H. Baines; S.S. Limaye ๐Ÿ“‚ Article ๐Ÿ“… 2001 ๐Ÿ› Elsevier Science ๐ŸŒ English โš– 808 KB

On 11-12 August 1998, we imaged Neptune using the Hubble Space Telescope WFPC2 CCD camera and NICMOS InSb camera to obtain high-spatial-resolution, absolutely calibrated imagery from the visible through the near infrared. We used nine HST orbits to intensively sample one rotation of Neptune, and fou