Magnetic Reconnection in the Plasma Disk at 23 Jupiter Radii
Abstract
A key open question in astrophysics is how plasma is transported within strongly magnetized, rapidly rotating systems. Magnetic reconnection and flux tube interchange are possible mechanisms, with Jupiter serving as the best local analog for distant systems. However, magnetic reconnection at Jupiter remains poorly understood. A key indicator of active magnetic reconnection is the ion diffusion region, but its detection at Jupiter has remained unconfirmed. Here, we report a unique magnetic reconnection event in Jupiter's inner magnetosphere that presents the first detection of an ion diffusion region. We provide evidence that this event involves localized flux tube interchange motion driven by centrifugal forces, which occurs inside a thin current sheet formed by the collision and twisting of two distinct flux tubes. This study provides new insights into Io-genic plasma transport at Jupiter and the unique role of magnetic reconnection in rapidly rotating systems, two key unresolved questions.
Cite
@article{arxiv.2503.21032,
title = {Magnetic Reconnection in the Plasma Disk at 23 Jupiter Radii},
author = {Jian-zhao Wang and Fran Bagenal and Stefan Eriksson and Robert E. Ergun and Peter A. Delamere and Robert J. Wilson and Robert W. Ebert and Philip W. Valek and Frederic Allegrini and Licia C. Ray},
journal= {arXiv preprint arXiv:2503.21032},
year = {2025}
}