• ISSN 2097-1893
    • CN 10-1855/P

    修正电子声波在准静态平行电场演化中的作用

    The role of modified electron acoustic waves in the evolution of quasi-static parallel electric fields

    • 摘要: 极光弧是一种常见的极光形态,其形成过程包含:源区扰动能量经Alfvén波传输到加速区、在加速区内产生加速结构、加速电子产生极光等三个环节. 观测表明极光弧对应具有U型结构的准静态平行电场,且U型结构底部有明显电场聚集特征. 针对如何从最初的能量输入演化出具有U型结构的准静态电场,基于现有极光粒子加速理论的模拟研究未能给出与观测特征相符的电场聚集结果. 这极可能是现有理论遗漏了某种关键的能量转化环节. 我们的研究表明,该环节的核心正是过渡区特有的修正电子声波. 据此,本文构建了首次纳入修正电子声波耦合的动态理论模型,其输出与U型结构的观测特征高度一致,并直接揭示了修正电子声波在准静态电场形成与演化中的决定性作用. 该成果为完善极光粒子加速理论提供了新的物理基础.

       

      Abstract: The auroral arc is a common form of aurora. Its formation involves three processes: the transfer of disturbed energy from the source region to the acceleration region via Alfvén waves, the generation of acceleration structures within the acceleration region, and the acceleration of electrons to produce aurora. Observations indicate that the auroral arc corresponds to a quasi-static parallel electric field with a U-shaped structure, with a clear concentration of the electric field at the bottom of the U-shaped structure. Regarding how the initial energy input evolves into a quasi-static electric field with a U-shaped structure, simulation studies based on existing auroral particle acceleration theories have not yet fully reproduced results that are fully consistent with the observed characteristics. This suggests that the existing theory may still lack a description of a key energy conversion process. Our research indicates that the core of this process lies precisely in the modified electron acoustic wave unique to the transition region. Based on this, we have constructed a dynamic theoretical model that incorporates, for the first time, the coupling of modified electron acoustic waves and kinetic Alfvén waves. The model's output is in good agreement with the observed characteristics of the U-shaped structure, directly revealing the decisive role of modified electron acoustic waves in the formation and evolution of the quasi-static electric field. This achievement provides a new physical foundation for improving the theory of auroral particle acceleration.

       

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