惠斯勒回声列车是由充满活力的冬季闪电引发的.
I Kolmašová1,2, O Santolík3,4, J Manninen5
1Department of Space Physics, Institute of Atmospheric Physics of the Czech Academy of Sciences, Prague, Czechia. iko@ufa.cas.cz.
Nature communications
|August 21, 2024
概括
强烈的雷暴可以在地球磁层中引发持久的哨声回声列车. 这些在芬兰观察到的信号,从遥远的风暴中传到4000多公里.
科学领域:
- 空间物理 空间物理
- 大气科学 大气科学
- 电磁主义 电磁主义
背景情况:
- 闪电会产生电磁脉冲,这些电磁脉冲在磁层中以哨子波的形式传播.
- 这些哨子的多个反射可以创建日益分散的回声列车.
- 磁层等离子管对于这些信号的远距离传播至关重要.
研究的目的:
- 调查2017年1月3日观察到的哨声回声列车的条件和来源.
- 为了确定所涉及的磁层管道的持续时间和特征.
- 为了确定引发观测到的回声列车的闪电事件的起源.
主要方法:
- 通过高度站 (芬兰Kannuslehto) 记录的无线电波信号的分析.
- 呼叫器回声列车及其分散模式的识别和描述.
- 信号观测与来自不同地理位置的闪电活动的相关性.
主要成果:
- 一个磁层等离子管道活跃了近八个小时.
- 惠斯勒回声列车是由三个不同的雷暴的闪电触发的.
- 从挪威的一场风暴和地中海地区两场遥远的风暴中观察到显著的回声列车产生.
- 这涉及到高达4000公里的亚星球传播距离.
结论:
- 强烈的雷暴,即使在遥远的地方,也可以反复激活磁层管道.
- 这种能量化导致了哨声回声列车的形成.
- 这些发现突出了陆地闪电对地球磁层在长距离上的重大影响.
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