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高能中性原子成像揭示了土星环电流近11年的周期。

Energetic neutral atom imaging reveals nearly 11-year cycle of the ring current of Saturn.

作者信息

Li Yimeng, Yue Chao, Sun Yixin, Jia Xianzhe, Zong Qiugang, Zhou Xuzhi

机构信息

Institute of Space Physics and Applied Technology, Peking University, Beijing, China.

Department of Climate and Space Sciences and Engineering, University of Michigan - Ann Arbor, Ann Arbor, MI, USA.

出版信息

Nat Commun. 2024 Dec 5;15(1):10597. doi: 10.1038/s41467-024-55037-9.

Abstract

The drift motion of energetic charged particles can generate an azimuthal electric current around the planet known as the ring current, which regulates the field configuration of the magnetosphere. However, limited coverage of in-situ measurements makes it challenging to investigate the long-term variations of the global ring current. Taking advantage of the energetic neutral atom (ENA) imaging onboard the Cassini mission, we present a nearly 11-year cycle of the suprathermal ring current populations in Saturn's magnetosphere. We find that the peak location of the suprathermal ring current in local time oscillates between post-midnight and pre-midnight sectors, and its intensity minimizes during the solar maximum. These results indicate that the modulation of the suprathermal ring current is closely related to the solar cycle. Our analysis also offers a preview of the ring current at other giant planets, such as Jupiter, which will be imaged by ENA cameras onboard the JUICE mission.

摘要

高能带电粒子的漂移运动能够在行星周围产生一种方位电流,即所谓的环电流,它会调节磁层的场结构。然而,原位测量的覆盖范围有限,使得研究全球环电流的长期变化颇具挑战性。利用卡西尼任务搭载的高能中性原子(ENA)成像技术,我们展示了土星磁层中超热环电流粒子群近11年的周期变化。我们发现,当地时间中超热环电流的峰值位置在午夜后和午夜前扇区之间振荡,并且其强度在太阳活动极大期最小。这些结果表明,超热环电流的调制与太阳活动周期密切相关。我们的分析还为其他巨行星(如木星)的环电流提供了一个预览,木星将由JUICE任务搭载的ENA相机进行成像。

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