Atmospheric and cloud structures of the Jovian planets

Icarus

Volumn 20, Issue 4, 1973, Pages 465-476

  Weidenschilling, S J ^a   Lewis, J S ^a,b  

^a MASSACHUSETTS INSTITUTE OF TECHNOLOGY   (United States)

^b Planetary Astronomy Laboratory Department of Earth and Planetary Sciences ^*  (United States)

Author keywords

[No Author keywords available]

Indexed keywords

EID: 0001001392     PISSN: 00191035     EISSN: 10902643     Source Type: Journal    
DOI: 10.1016/0019-1035(73)90019-5     Document Type: Article

References (24)

1. Formation of the outer planets
2. 2O cloud models for the outer planets
3. The planet Jupiter
4. The freezing point curve of the system water-ammonia
5. Multi-phase ammonia water system
6. Structure of Jupiter chemical composition contraction and rotation
7. Interior of Jupiter and Saturn
8. Formation of spectral lines in planetary atmospheres IV. Theoretical evidence for structure of Jovian clouds from spectroscopic observation methane and hydrogen quadrupole lines
9. Wet adiabatic model atmospheres for Jupiter
10. 2S systems
11. Observability of spectroscopically active compounds in the atmosphere of Jupiter
12. Chemistry of the outer solar system
13. Jupiter's clouds; structure and composition
14. 2O system. I.
15. The structure of models of Neptune
16. Uranus atmosphere structure and composition
17. Optical characteristics and structure of the Jovian atmosphere V. Probable structure of the ammonia aerosol layer
18. Cloud base levels for Jupiter and Venus and the heretomolecular nucleation theory
19. On the upper atmosphere of Neptune
20. Photochemistry of planetary atmospheres
21. The total and partial vapor pressures of aqueous ammonia solutions