Improved constraints on Neptune's atmosphere from submillimetre-wavelength observations

Details Improved constraints on Neptune's atmosphere from submillimetre-wavelength observations Improved constraints on Neptune's atmosphere from submillimetre-wavelength observations

Jan 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005a%26a...429.1097m&link_type=abstract

Astronomy and Astrophysics, v.429, p.1097-1105 (2005)

Astronomy and Astrophysics

Astrophysics

13

Planets And Satellites: Individual: Neptune, Radio Lines: Solar System

Scientific paper

We describe observations of Neptune carried out using the James Clerk Maxwell Telescope (Mauna Kea, Hawaii) during September 1998. High-quality data for the sub-mm-wavelength rotational transitions of HCN (J=4-3) and CO (J=3-2 and 4-3) were obtained, and we use the data to make improved determinations of the abundances of these trace species and the temperature profile of Neptune's atmosphere.

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