Solar Wind Dynamic Pressure Upstream From Saturn: Estimation From Magnetosheath Properties and Comparison With SKR-Reference-Cited by-同舟云学术

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Solar Wind Dynamic Pressure Upstream From Saturn: Estimation From Magnetosheath Properties and Comparison With SKR

Published:2019-10 Issue:10 Volume:124 Page:7799-7819
ISSN:2169-9380
Container-title:Journal of Geophysical Research: Space Physics
language:en
Short-container-title:J. Geophys. Res. Space Physics

Author:

Thomsen M. F.¹²^ORCID,Jackman C. M.³^ORCID,Lamy L.⁴^ORCID

Affiliation:

1. Planetary Science Institute Tucson AZ USA

2. Los Alamos National Laboratory Los Alamos NM USA

3. Department of Physics and AstronomyUniversity of Southampton Southampton UK

4. LESIA, Observatoire de Paris, Université PSL, CNRS, Sorbonne Universités, Université Paris Diderot Meudon France

Funder

Jet Propulsion Laboratory

Science and Technology Facilities Council

National Aeronautics and Space Administration

Publisher

American Geophysical Union (AGU)

Subject

Space and Planetary Science,Geophysics

Link

https://onlinelibrary.wiley.com/doi/pdf/10.1029/2019JA026819

Reference69 articles.

1. Modeling the size and shape of Saturn's magnetopause with variable dynamic pressure

2. Saturn's magnetodisc current sheet

3. Open flux estimates in Saturn's magnetosphere during the January 2004 Cassini-HST campaign, and implications for reconnection rates

4. Significance of Dungey-cycle flows in Jupiter's and Saturn's magnetospheres, and their identification on closed equatorial field lines

5. Relationship between solar wind corotating interaction regions and the phasing and intensity of Saturn kilometric radiation bursts

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2. Effect of a Magnetospheric Compression on Jovian Radio Emissions: In Situ Case Study Using Juno Data;Journal of Geophysical Research: Space Physics;2023-09

3. Saturn Anomalous Myriametric Radiation, a New Type of Saturn Radio Emission Revealed by Cassini;Geophysical Research Letters;2022-08-19

4. MSWIM2D: Two-dimensional Outer Heliosphere Solar Wind Modeling;The Astrophysical Journal Supplement Series;2022-06-01

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