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Main Author: Pantellini, Filippo
Format: Preprint
Published: 2025
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Online Access:https://arxiv.org/abs/2503.15396
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author Pantellini, Filippo
author_facet Pantellini, Filippo
contents Incompressible vortex flow are observed in a large variety of astrophysical plasmas such as the convection zone and the atmosphere of stars, in astrophysical jets in stellar winds and in planetary magnetospheres. More specifically, magnetohydrodynamic (MHD) simulations have shown that two large scale interlaced Alfvénic vortices structure the magnetic tail of Uranus at solstice time. Assuming identical vortices, we compute the general linear structure of the flow near their centers within the frame of ideal MHD. We then use the analytic results to interpret and qualify the vortices observed in a 3D MHD simulation of a fast rotating Uranus-type planet.
format Preprint
id arxiv_https___arxiv_org_abs_2503_15396
institution arXiv
publishDate 2025
record_format arxiv
spellingShingle On the linear structure of the interlaced Alfvén vortices in the tail of Uranus at solstice
Pantellini, Filippo
Earth and Planetary Astrophysics
Plasma Physics
Incompressible vortex flow are observed in a large variety of astrophysical plasmas such as the convection zone and the atmosphere of stars, in astrophysical jets in stellar winds and in planetary magnetospheres. More specifically, magnetohydrodynamic (MHD) simulations have shown that two large scale interlaced Alfvénic vortices structure the magnetic tail of Uranus at solstice time. Assuming identical vortices, we compute the general linear structure of the flow near their centers within the frame of ideal MHD. We then use the analytic results to interpret and qualify the vortices observed in a 3D MHD simulation of a fast rotating Uranus-type planet.
title On the linear structure of the interlaced Alfvén vortices in the tail of Uranus at solstice
topic Earth and Planetary Astrophysics
Plasma Physics
url https://arxiv.org/abs/2503.15396