Multi-wavelength Observations of Neptune's Atmosphere

Details Multi-wavelength Observations of Neptune's Atmosphere Multi-wavelength Observations of Neptune's Atmosphere

Sep 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008epsc.conf..660m&link_type=abstract

European Planetary Science Congress 2008, Proceedings of the conference held 21-25 September, 2008 in Münster, Germany. Online a

Physics

Scientific paper

We conducted a multi-wavelength observing campaign on Neptune between June and October, 2003. We used the 10-m Keck telescope at near- and mid-infrared wavelengths and the VLA at radio wavelengths. At mid-infrared and radio wavelengths the south polar region is relatively warm, which we interpret as being caused by global dynamics in Neptune's atmosphere: subsiding motions over the pole and the equator and rising at southern midlatitudes are qualitatively consistent all the observations.

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