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首页> 外文期刊>Geophysical Research Letters >Three-dimensional test particle simulation of the 17-18 March 2013 CME shock-driven storm
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Three-dimensional test particle simulation of the 17-18 March 2013 CME shock-driven storm

机译:2013年3月17日至18日CME冲击驱动风暴的三维测试粒子模拟

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摘要

Three-dimensional test particle simulation of energetic electrons (hundreds of keV to MeV), including both an initially trapped population and continuously injected population, driven by the Lyon-Fedder-Mobarry global MHD model coupled with Magnetosphere-Ionosphere Coupler/Solver boundary conditions, is performed for the 17 March 2013 storm. The electron trajectories are calculated and weighted using the ESA model for electron flux versus energy and L. The simulation captures the flux dropout at both GOES 13 and GOES 15 locations after a strong CME (coronal mass ejection)-shock arrival which produced a Dst=-132nT storm, and recovery to the prestorm value later, consistent with GOES satellite measurements. This study provides the first 3-D test particle simulation combining the trapped and injected populations. The result demonstrates that including both populations in the simulation is essential to study the dynamics of the outer radiation belt over the typical day-long timescale of ring current development, main phase, and early recovery phase.
机译:由Lyon-Fedder-Mobarry全局MHD模型与磁层-电离层耦合器/ Solver边界条件共同驱动的高能电子(数百keV到MeV)的三维测试粒子模拟,包括初始捕获的种群和连续注入的种群,是针对2013年3月17日的风暴执行的。使用ESA模型计算电子轨迹并加权,以计算电子通量与能量和L的关系。该模拟捕获了在强CME(日冕质量抛射)冲击到达后产生Dst =的GOES 13和GOES 15位置处的通量下降。 -132nT暴风雨,之后恢复到暴风雨前的值,与GOES卫星测量结果一致。这项研究提供了第一个3-D测试粒子模拟,结合了捕获和注入的种群。结果表明,在模拟中包括两个种群,对于研究环流发展,主要阶段和早期恢复阶段的典型全天时间尺度内外部辐射带的动力学至关重要。

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