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Ionospheric responses to the 21 August 2017 solar eclipse by using data assimilation approach

机译:使用数据同化方法对2017年8月21日日食的电离层响应

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Using the physics-based thermosphere-ionosphere model (NCAR-TIEGCM) with an ensemble Kalman filter, this study reports the first data assimilative analysis of the ionosphere responses to the solar eclipse on 21 August 2017. The system, using a 2-min assimilation cycle of data from ground-based GNSS observations, show dynamic variations of the equatorial ionization anomaly (EIA) due to the electrodynamic effects of the solar eclipse. Two major ionospheric responses are captured: (1) an early appearance of EIA at the westward boundary of moon shadow and (2) an enhanced EIA at lower latitudes and suppressed EIA at the higher latitudes. These eclipse-induced conjugate EIA variations are produced by an eastward electric field perturbation around the magnetic equator and a westward electric field perturbation at the higher latitudes.
机译:使用基于物理学的热球-电离层模型(NCAR-TIEGCM)和集成卡尔曼滤波器,本研究报告了2017年8月21日对电离层对日食响应的首次数据同化分析。该系统使用2分钟的同化来自地面GNSS观测的数据周期显示,由于日食的电动力效应,赤道电离异常(EIA)的动态变化。捕获了两个主要的电离层响应:(1)EIA在月影西边界处的早期出现,(2)在较低纬度时增强了EIA,在较高纬度时抑制了EIA。这些由日食引起的共轭EIA变化是由磁赤道周围的向东电场扰动和较高纬度的向西电场扰动产生的。

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