Spatially-resolved spectroscopy at 1.6 μm of Titan's atmosphere and surface-Reference-Cited by-同舟云学术

Spatially-resolved spectroscopy at 1.6 μm of Titan's atmosphere and surface

Author:

Ádámkovics M.¹,de Pater I.²,Roe H. G.³,Gibbard S. G.⁴,Griffith C. A.⁵

Affiliation:

1. Department of Chemistry; University of California; Berkeley California USA

2. Department of Astronomy; University of California; Berkeley California USA

3. Division of Geological and Planetary Sciences; California Institute of Technology; Pasadena California USA

4. Institute of Geophysics and Planetary Physics; Lawrence Livermore National Laboratory; Livermore California USA

5. Lunar and Planetary Laboratory; University of Arizona; Tucson Arizona USA

Publisher

American Geophysical Union (AGU)

Subject

General Earth and Planetary Sciences,Geophysics

Reference28 articles.

2. Properties of Titan's methane-ethane clouds from microphysical modeling (abstract);Barth;Bull. Am. Astron. Soc.,2004

3. Bouchez , A. H. 2003 Seasonal trends in Titan's atmosphere: Haze, wind, and clouds Calif. Inst. of Technol. Pasadena, Calif

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