Spatial structure in Neptune’s 7.90-μm stratospheric CH4 emission, as measured by VLT-VISIR

Author:

Sinclair J.A.,Orton G.S.ORCID,Fletcher L.N.,Roman M.ORCID,de Pater I.,Encrenaz T.,Hammel H.B.ORCID,Giles R.S.ORCID,Velusamy T.,Moses J.I.,Irwin P.G.J.ORCID,Momary T.W.ORCID,Rowe-Gurney N.ORCID,Tabataba-Vakili F.

Funder

National Science Foundation

European Research Council

National Aeronautics and Space Administration

Publisher

Elsevier BV

Subject

Space and Planetary Science,Astronomy and Astrophysics

Reference68 articles.

1. Clouds, hazes, and the stratospheric methane abundance in Neptune;Baines;Icarus,1994

2. Hydrocarbons in neptune’s stratosphere from voyager infrared observations;Bezard;J. Geophys. Res.,1991

3. Detection of the methyl radical on neptune;Bézard;Astrophys. J.,1999

4. Spectral irradiance calibration in the infrared. X. A self-consistent radiometric all-sky network of absolutely calibrated stellar spectra;Cohen;Astron. J.,1999

5. Thermal structure and dynamics of Neptune’s atmosphere from voyager measurements;Conrath;J. Geophys. Res.,1991

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