The composition and structure of Enceladus' plume from the complete set of Cassini UVIS occultation observations-Reference-Cited by-同舟云学术

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The composition and structure of Enceladus' plume from the complete set of Cassini UVIS occultation observations

Published:2020-07 Issue: Volume:344 Page:113461
ISSN:0019-1035
Container-title:Icarus
language:en
Short-container-title:Icarus

Author:

Hansen C.J.,Esposito L.W.,Colwell J.E.,Hendrix A.R.,Portyankina G.,Stewart A.I.F.,West R.A.

Funder

National Aeronautics and Space Administration

Publisher

Elsevier BV

Subject

Space and Planetary Science,Astronomy and Astrophysics

Reference57 articles.

1. Enceladus’ internal ocean and ice shell constrained from Cassini gravity, shape, and libration;Cadek;GRL,2016

2. The electronic spectrum of water in the discrete and continuum regions. Absolute optical oscillator strengths for photoabsorption (6 200 eV);Chan;Chem. Phys.,1993

3. Absorption cross sections of NH3, NH2D, NHD2, and ND3 in the spectral range 140–220 nm and implications for planetary isotopic fractionation;Cheng;Astrophys. J.,2006

4. Cassini UVIS stellar occultation observations of Saturn’s rings;Colwell;Astron. J.,2010

5. Identification of a dynamic atmosphere at Enceladus with the Cassini magnetometer;Dougherty;Science,2006

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