Detection of hydrogen sulfide above the clouds in Uranus’s atmosphere
Author:
Publisher
Springer Science and Business Media LLC
Subject
Astronomy and Astrophysics
Link
http://www.nature.com/articles/s41550-018-0432-1.pdf
Reference47 articles.
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2. Irwin, P. G. J. et al. The application of new methane line absorption data to Gemini-N/NIFS and KPNO/FTS observations of Uranus’ near-infrared spectrum. Icarus 220, 369–382 (2012).
3. Sromovsky, L. A., Fry, P. M. & Kim, J. H. Methane on Uranus: the case for a compact CH4 cloud layer at low latitudes and a severe CH4 depletion at high latitudes based on a re-analysis of Voyager occultation measurements and STIS spectroscopy. Icarus 215, 292–312 (2011).
4. Weidenschilling, S. J. & Lewis, J. S. Atmospheric and cloud structures of the Jovian planets. Icarus 20, 465–476 (1973).
5. de Pater, I., Romani, P. N. & Atreya, S. K. Possible microwave absorption by H2S gas in Uranus’ and Neptune’s atmospheres. Icarus 91, 220–233 (1991).
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