\(\mathrm{H}_{2} \mathrm{~S}\) opacity may significantly affect the brightness temperatures of Uranus and Neptune due to possible depletion of ammonia in the tropospheres of those planets (de Pater et al. 1991, Icarus 91, 220-233). Though the rotational line centers of \(\mathrm{H}_{2} \mathrm{~S}\)
✦ LIBER ✦
Interpretation of Auroral “Lightcurves” with Application to Jovian H+3Emissions
✍ Scribed by John E.P. Connerney; Takehiko Satoh; Richard L. Baron
- Publisher
- Elsevier Science
- Year
- 1996
- Tongue
- English
- Weight
- 324 KB
- Volume
- 122
- Category
- Article
- ISSN
- 0019-1035
No coin nor oath required. For personal study only.
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