The complex shape of the outer edge of Saturn’s B ring, as observed in Cassini occultation data-Reference-Cited by-同舟云学术

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The complex shape of the outer edge of Saturn’s B ring, as observed in Cassini occultation data

Published:2023-11 Issue: Volume:405 Page:115678
ISSN:0019-1035
Container-title:Icarus
language:en
Short-container-title:Icarus

Author:

French Richard G.^ORCID,Nicholson Philip D.,McGhee-French Colleen A.,Longaretti Pierre-Yves,Hedman Matthew M.,Colwell Joshua,Marouf Essam A.,Rappaport Nicole,Flury Sophia,Fong Jolene,Maguire Ryan,Steranka Glen

Publisher

Elsevier BV

Subject

Space and Planetary Science,Astronomy and Astrophysics

Reference33 articles.

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2. Sharp edges of planetary rings;Borderies;Nature,1982

3. A granular flow model for dense planetary rings;Borderies;Icarus,1985

4. Test particle motion around an oblate planet;Borderies-Rappaport;Icarus,1994

5. Viscosity in a sense planetary ring with self-gravitating particles;Daisaka;Icarus,2001

Cited by 2 articles. 订阅此论文施引文献订阅此论文施引文献，注册后可以免费订阅5篇论文的施引文献，订阅后可以查看论文全部施引文献

1. Stationary dynamics of planetary ring edge modes at Saturn’s B ring edge;Icarus;2024-04

2. The Uranus system from occultation observations (1977–2006): Rings, pole direction, gravity field, and masses of Cressida, Cordelia, and Ophelia;Icarus;2024-03

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