𝔖 Bobbio Scriptorium
✦   LIBER   ✦

Photochemical Models of Pluto's Atmosphere

✍ Scribed by L.M. Lara; W.-H. Ip; R. Rodrigo

Publisher
Elsevier Science
Year
1997
Tongue
English
Weight
551 KB
Volume
130
Category
Article
ISSN
0019-1035

No coin nor oath required. For personal study only.

πŸ“œ SIMILAR VOLUMES

Mirages and the Nature of Pluto's Atmosp
Mirages and the Nature of Pluto's Atmosphere
✍ J.A. Stansberry; J.I. Lunine; W.B. Hubbard; R.V. Yelle; D.M. Hunten πŸ“‚ Article πŸ“… 1994 πŸ› Elsevier Science 🌐 English βš– 615 KB
Coupled Atmosphere-Ocean Models of Titan
Coupled Atmosphere-Ocean Models of Titan's Past
✍ Christopher P. McKay; James B. Pollack; Jonathan I. Lunine; RΓ©gis Courtin πŸ“‚ Article πŸ“… 1993 πŸ› Elsevier Science 🌐 English βš– 587 KB

We have developed a coupled atmosphere and ocean model of Titan's surface. The atmospheric model is a 1-D spectrally-resolved radiative-convective model. The ocean thermodynamics are based upon solution theory. The ocean, initially composed of CH4, becomes progressively enriched in ethane over time.

Pluto's Radius and Atmosphere: Results f
Pluto's Radius and Atmosphere: Results from the Entire 9 June 1988 Occultation Data Set
✍ R.L. Millis; L.H. Wasserman; O.G. Franz; R.A. Nye; J.L. Elliot; E.W. Dunham; A.S πŸ“‚ Article πŸ“… 1993 πŸ› Elsevier Science 🌐 English βš– 790 KB

We have analyzed all photometric observations of the 9 June 1988 occultation of the star P8 by Pluto in order to derive the radius of Pluto and certain parameters of its atmosphere. Our analysis is based on a "haze" model; but where relevant, we also discuss the thermal gradient model. With either m