NEWS & EVENTS

RIPPLING CURRENT SHEET GENERATED BY MAGNETODISK RECONNECTION ON JUPITER

The Jovian magnetodisk deviates from the geographical equator and is distributed close to the magnetic equator. The location and motion of the magnetodisk are vital parameters for studying the magnetospheric dynamics and the coupling with the ionosphere. The primary motion of the magnetodisk is rotating with Jupiter as the tilted magnetic dipole axis rotates about the planetary spin axis. Additionally, small-scale flapping-like motions are observed in the magnetodisk, although the mechanism behind these motions remains unclear. In this study, we find that when magnetic reconnection occurs, the magnetodisk current sheet behaves as a kink-like wave when crossing the spacecraft. The spacecraft then crosses the current sheet repeatedly and records multiple reconnection signals during one rotation period. These observations suggest that the multiple magnetic reconnection sites break the magnetodisk field lines, causing the current sheet to become a rippling-like structure, which also rotates with the magnetosphere.