Rotation‐Controlled Diurnal Evolution of Uranus' Asymmetric Bow Shock at Equinox

Abstract Uranus possesses the most extreme magnetic and rotational geometry in the solar system, resulting in a uniquely dynamic and asymmetric interaction between its magnetosphere and the solar wind. Here we investigate the diurnal evolution of the Uranian bow shock (BS) at equinox using global mu...

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Detalles Bibliográficos

Principais autores:	X. Cao, C. Paty, F. Chu, J. Lei
Formato:	Artigo
Idioma:	Inglês
Publicado:	Wiley 2026-06-01
Series:	AGU Advances
Assuntos:	Uranus magnetosphere bow shock ice giant solar wind interaction
Acceso en liña:	https://doi.org/10.1029/2026AV002307
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