在地磁风暴期间,电离层电子温度超标的极端两相变化
Artem Smirnov1,2, Yuri Shprits3,4, Hermann Lühr3
1Department of Earth and Environmental Sciences, Ludwig Maximilian University of Munich (LMU), Munich, Germany. artem.smirnov@gfz.de.
Scientific reports
|February 11, 2025
概括
早晨的电子温度 (Te) 超标显示了地磁风暴期间的两阶段反应. 最初增强,它在风暴恢复阶段大幅耗尽并消失,揭示了新的电离层动态.
科学领域:
- 空间物理 空间物理
- 离子球物理 离子球物理
- 大气科学 大气科学
背景情况:
- 早晨的电子温度 (Te) 超标是在日出时观察到的关键电离层特征.
- 尽管进行了广泛的研究,但其在地磁风暴期间的行为尚未得到充分理解.
研究的目的:
- 为了研究上午Te overshoot对地磁活动的反应.
- 为了揭示近地太空环境动态中的新物理模式.
主要方法:
- 利用神经网络模型来分析电离层数据.
- 检查了地磁风暴期间Te overshoot的两阶段反应.
主要成果:
- 在暴风雨的主要阶段观察到Te overshoot的初始增强.
- 记录了随后的剧烈耗尽 (>1000 K) 和在恢复阶段超标的消失.
- 这些变化与迅速透和干扰动力发电场相关联,影响等离子体漂移和冷却速度.
结论:
- 这项研究揭示了上午Te超标对地磁风暴的两相反应.
- 这些发现突出了电场对电离层等离子体密度和温度的影响.
- 展示了数字双胞胎模型在发现复杂的太空天气现象方面的潜力.
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