Retrieval of Chemical Abundances in Titan's Upper Atmosphere From Cassini UVIS Observations With Pointing Motion

Author:

Fan Siteng1ORCID,Shemansky Donald E.2ORCID,Li Cheng1ORCID,Gao Peter3,Wan Linfeng4,Yung Yuk L.15

Affiliation:

1. Division of Geological and Planetary Sciences California Institute of Technology Pasadena CA USA

2. Space Environment Technologies Altadena CA USA

3. Department of Astronomy University of California Berkeley CA USA

4. Department of Earth and Planetary Sciences University of California Santa Cruz CA USA

5. Jet Propulsion Laboratory California Institute of Technology Pasadena CA USA

Funder

National Aeronautics and Space Administration

Publisher

American Geophysical Union (AGU)

Subject

General Earth and Planetary Sciences,Environmental Science (miscellaneous)

Reference28 articles.

1. The valence shell photoabsorption of the linear alkanes, CnH2n+2 (n=1–8): absolute oscillator strengths (7–220 eV)

2. New benzene absorption cross sections in the VUV, relevance for Titan’s upper atmosphere

3. Temperature-dependent photoabsorption cross sections in the VUV-UV region. I. Methane and ethane

4. Chiang R. Lisman S. Wong E. Enright P. Breckenridge W. &Jahanshahi M.(1993).Robust attitude control for Cassini spacecraft flying by Titan. Paper presented at Guidance Navigation and Control Conference Monterey CA. doi:https://doi.org/10.2514/6.1993‐3754

5. Vacuum ultraviolet spectroscopy of cyanogen and cyanoacetylenes

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