Three-Dimensional Magnetohydrodynamic Simulations of the Solar Wind Interaction With a Hyperfast-Rotating Uranus
Author:
Affiliation:
1. LESIA, Observatoire de Paris, Université PSL, CNRS, Sorbonne Université, Université Paris Diderot, Sorbonne Paris Cité; Meudon France
2. LUTH, Observatoire de Paris, PSL Research University, CNRS UMR 8102, Université Paris Diderot; Meudon France
Funder
Plas@par
CNES (Centre national d'Etudes spatiales)
Observatoire de Paris
Publisher
American Geophysical Union (AGU)
Subject
Space and Planetary Science,Geophysics
Link
http://onlinelibrary.wiley.com/wol1/doi/10.1029/2018JA025331/fullpdf
Reference18 articles.
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3. Heliospheric magnetic field strength out to 66 AU: Voyager 1, 1978-1996;Burlaga;Journal of Geophysical Research,1998
4. Diurnal and seasonal variability of Uranus's magnetosphere;Cao;Journal of Geophysical Research: Space Physics,2017
5. How is the Jovian main auroral emission affected by the solar wind?;Chané;Journal of Geophysical Research: Space Physics,2017
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