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Updated: Jun 6, 2025

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Simulating Impacts of Ice Storms on Forest Ecosystems
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雷暴产生的重力波对电离层-热层的影响使用TIEGCM-NG/MAGIC模拟和与GNSS TEC,ICON和COSMIC-2观测的比较
Xian Lu1, Haonan Wu1,2, Chris Heale3
1Department of Physics and Astronomy Clemson University Clemson SC USA.
概括
严重的雷暴会产生引力波,扰乱电离层和热层,形成由卫星观察到的同心图案. 这些波影响中性风,温度和电子密度,影响太空天气.
科学领域:
- 空间物理 空间物理
- 大气科学 大气科学
- 地质物理学 地质物理学
背景情况:
- 严重的雷暴可以产生大气重力波.
- 这些波可以传播到大气上层,影响电离层和热层.
- 了解这些干扰对于太空天气预报至关重要.
研究的目的:
- 为了研究由严重的雷暴系统引起的电离层和热层干扰.
- 分析龙卷风产生的重力波的特征和传播.
- 通过卫星观测验证模型模拟.
主要方法:
- 使用热层-离子层-电动力学通用循环模型-下一代 (TIEGCM-NG) 受到MAGIC重力波的推动.
- 模拟严重雷暴系统的冲击,并进行多次龙卷风触地.
- 将模型输出与ICON和COSMIC-2卫星的现场观测结果进行比较.
主要成果:
- 引力波在全球导航卫星系统 (GNSS) 旅行离子层干扰 (TID) 中创造了同心圆形的环形.
- 在中性风,温度和密度下观察到波浪周期和振幅的显著垂直演变.
- 检测到电子密度的大量扰动,改变了在赤道离子异常 (EIA) 峰附近的夜间电离层结构.
结论:
- TIEGCM-NG模型成功模拟了同心型TID及其传播到结合半球.
- 重力波对ICON和COSMIC-2探测到的电离层高度产生影响,与模型结果有很好的一致性.
- 离子密度的波动归因于垂直离子传输,由中性风或电动力学合驱动.
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