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Neptune's global circulation deduced from multi-wavelength observations

Abstract:

We observed Neptune between June and October 2003 at near- and mid-infrared wavelengths with the 10-m W.M. Keck II and I telescopes, respectively; and at radio wavelengths with the Very Large Array. Images were obtained at near-infrared wavelengths with NIRC2 coupled to the adaptive optics system in both broad- and narrow-band filters between 1.2 and 2.2 μ. In the mid-infrared we imaged Neptune at wavelengths between 8 and 22 μm, and obtained slit-resolved spectra at 8-13 μm and 18-22 μm. At ...

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Publication status:
Published

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Institution:
University of Oxford
Division:
MPLS
Department:
Physics
Sub department:
Atmos Ocean & Planet Physics
Role:
Author
Publisher:
Academic Press Inc.
Journal:
ICARUS More from this journal
Volume:
237
Pages:
211-238
Publication date:
2014-07-15
DOI:
EISSN:
1090-2643
ISSN:
0019-1035
Language:
English
Keywords:
Pubs id:
pubs:466431
UUID:
uuid:a9eab86f-aead-4e98-b9f0-06eb2a2b05df
Local pid:
pubs:466431
Source identifiers:
466431
Deposit date:
2014-06-17

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