无碰撞重联区中的混沌感应电阻
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1. 洛阳师范学院空间物理研究所 洛阳 471934;2. 中国科学院紫金山天文台 南京 210023;3. 河南省电磁变换与探测重点实验室 洛阳 471934

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P182;

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国家自然科学基金项目(42174195、11873018、11790302、11761131007)资助


Chaos-induced Resistivity in Collisionless Magnetic Reconnection Region
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Affiliation:

1. Institute of Space Physics, Luoyang Normal University, Luoyang 471934;2. Purple Mountain Observatory, Chinese Academy of Sciences, Nanjing 210023;3. Henan Key Laboratory of Electromagnetic Transformation and Detection, Luoyang 471934;

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    摘要:

    无碰撞磁场重联作为一种将磁能有效转化为等离子体动能和热能的机制, 已经被广泛应用于解释太阳耀斑、地球磁暴等各类等离子体的爆发活动. 然而, 在无碰撞重联区中反常电阻的微观物理机制仍然是尚未解决的基本问题. 在众多反常电阻的形成机制中, 基于磁零点附近粒子轨道混沌性产生的混沌感应电阻, 虽然不是最普遍流行的形成机制, 但它的微观物理图像却是最为清晰的. 回顾了无碰撞重联区中混沌感应电阻的早期研究和基本理论模型, 介绍了关于混沌感应电阻研究的新进展并阐述了混沌感应电阻未来的研究方向.

    Abstract:

    Collisionless magnetic reconnection, which converts the magnetic energy into the kinetic energy of plasma particles via the heating or acceleration, has been believed widely to be able to explain various eruptive phenomena such as solar flares and geomagnetic storms. However, the microphysical mechanism of anomalous resistivity in the collisionless magnetic reconnection is still an unsolved fundamental problem. Among the many physical mechanisms of anomalous resistivity formation, chaos-induced resistivity based on the chaos of the charged particle orbits near the magnetic neutral point is not the most popular formation mechanism, but its microscopic physical picture is the clearest. This paper first briefly reviews the early research and physical model of the chaos-induced resistivity in collisionless magnetic reconnection region, introduces the recent research progress of the chaos-induced resistivity, and expounds the future research direction of the chaos-induced resistivity.

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引用本文

王桢,陈玲,吴德金.无碰撞重联区中的混沌感应电阻[J].天文学报,2023,64(3):37. WANG Zhen, CHEN Ling, WU De-jin. Chaos-induced Resistivity in Collisionless Magnetic Reconnection Region[J]. Acta Astronomica Sinica,2023,64(3):37.

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  • 收稿日期:2022-09-23
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  • 在线发布日期: 2023-06-02
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