使用GNSS观测在地球大气层中探测流星海的前景
Panagiotis Vergados1, Siddharth Krishnamoorthy1, Léo Martire1
1Jet Propulsion Laboratory, California Institute of Technology, Pasadena, CA USA.
概括
流星海产生大气重力波 (GWs),可通过全球导航卫星系统 (GNSS) 无线电遮蔽和卫星温度数据检测到. 这些波提供了关于石海大气合的见解.
科学领域:
- 大气科学 大气科学
- 地质物理学 地质物理学
- 太空物理空间物理学
背景情况:
- 流星海是大气干扰引发的海洋波.
- 它们的大气合和检测能力仍然不太清楚.
- 理论上,引力波可以将大气和海洋现象联系起来.
研究的目的:
- 为了研究石海与地球大气层的物理合.
- 为了评估meteotsunami产生的大气波的检测能力.
- 为了分析2013年6月13日美国东海岸发生的流星海事件.
主要方法:
- 使用全球导航卫星系统 (GNSS) 的无线电隐蔽 (RO) 测量.
- 使用宽带发射放射测量 (SABER) 温度数据对大气进行探测.
- 分析地面GNSS的电离层总电子含量 (TEC) 观测结果.
- 应用线性重力波 (GW) 理论用于动态合分析.
主要成果:
- RO数据揭示了在事件附近的平流层GW活动.
- 据SABER数据证实,在中层层中,GW的垂直波长增加了.
- 9小时后,GNSS-TEC数据检测到了远场电离层反应.
- 观察结果与GW理论对石海合的预测一致.
结论:
- 在研究石海与大气相互作用方面,GNSS RO测量非常有价值.
- 流星海会产生可检测的大气重力波.
- 结合的GNSS RO和TEC数据增强了对这些现象的理解.
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