EGU25-6572, updated on 14 Mar 2025
https://doi.org/10.5194/egusphere-egu25-6572
EGU General Assembly 2025
© Author(s) 2025. This work is distributed under
the Creative Commons Attribution 4.0 License.
Poster | Thursday, 01 May, 14:00–15:45 (CEST), Display time Thursday, 01 May, 14:00–18:00
 
Hall X4, X4.172
Magnetodisk Magnetic reconnection in the centrifugally dominated giant planets
Ruilong Guo1 and Zhonghua Yao2
Ruilong Guo and Zhonghua Yao
  • 1Shandong University, Institute of Space Sciences, China (grl@sdu.edu.cn)
  • 2Department of Earth Sciences, The University of Hong Kong, Hong Kong SAR, China

Understanding the dynamics of planetary magnetospheres and auroral phenomena hinges significantly on magnetic reconnection. The rapid rotation of Jupiter and Saturn and the internal mass sources in the inner magnetospheres give rise to the magnetodisk current sheet that encircles the planet. The magnetodisk current sheet provides a place that is conducive to reconnection. Notably, the magnetodisk reconnection process is not confined to the nightside magnetosphere. The reconnection sites occur at various local times throughout the magnetosphere and rotate with the magnetosphere. The discretely distributed small-scale magnetodisk reconnection sites can lead to a comprehensive release of energy and mass from the magnetosphere.

How to cite: Guo, R. and Yao, Z.: Magnetodisk Magnetic reconnection in the centrifugally dominated giant planets, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-6572, https://doi.org/10.5194/egusphere-egu25-6572, 2025.