Global variation of the para hydrogen fraction in Jupiter's atmosphere and implications for dynamics on the outer planets

Icarus

Volumn 57, Issue 2, 1984, Pages 184-204

  Conrath, Barney J ^a   Gierasch, Peter J ^b  

^a NASA GODDARD SPACE FLIGHT CENTER   (United States)

^b Center for Radiophysics and Space Research Cornell University ^*  (United States)

Author keywords

[No Author keywords available]

Indexed keywords

EID: 0000936526     PISSN: 00191035     EISSN: 10902643     Source Type: Journal    
DOI: 10.1016/0019-1035(84)90065-4     Document Type: Article

References (36)

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2. Theory of the line shape in pressure induced absorption
3. Evidence for disequilibrium of ortho and para hydrogen on Jupiter from Voyager IRIS measurements
4. Para hydrogen conversion on the first transition series
5. The helium abundance of Jupiter from Voyager
6. Dynamical consequences of orthohydrogen-parahydrogen disequilibrium on Jupiter and Saturn
7. Infrared observations of the Jovian system from Voyager 1
8. Infrared observations of the Jovian system from Voyager 2
9. Infrared spectrometer for Voyager
10. Albedo internal heat and energy balance of Jupiter Preliminary results of the Voyager infrared investigation
11. The catalysis of the para-hydrogen conversion by the solid free radical αα-diphenyl-β-picryl hydrazyl
12. The solar spectrum between 1200 and 3000 Å
13. Interaction of eddies and mean zonal flow on Jupiter as inferred from Voyager 1 and 2 images
14. Solar heating and internal heat flow on Jupiter
15. HCN formation on Jupiter: The coupled photochemistry of ammonia and acetylene
16. The atmosphere of Jupiter An analysis of the Voyager radio occultation measurements
17. Study of the ammonia ice cloud layer in the equatorial region of Jupiter from the infrared interferometric experiment on Voyager
18. Conversion of para and ortho hydrogen in the Jovian planets
19. Global thermal structure and dynamics of Saturn and Jupiter from Voyager infrared measurements
20. Ortho-para transition in molecular hydrogen
21. Cloud microphysics: Analysis of the clouds Earth, Venus, Mars, and Jupiter
22. Jupiter;s atmospheric composition and cloud structure deduced from absorption bands in reflected sunlight
23. 2
24. Optical ortho-para transitions in molecules
25. 2 in the atmospheres of the Jovian planets
26. The photochemistry of hydrocarbons in the Jovian atmosphere
27. Model atmospheres of the major planets
28. The structure of the Uranus atmosphere