首页> 外文期刊>Journal of Geophysical Research, A. Space Physics: JGR >Global Ionospheric and Thermospheric Effects of the June 2015 Geomagnetic Disturbances: Multi-Instrumental Observations and Modeling
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Global Ionospheric and Thermospheric Effects of the June 2015 Geomagnetic Disturbances: Multi-Instrumental Observations and Modeling

机译:2015年6月的全球电离层和热散对效果Geomagnetic扰动:多乐器观测和建模

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摘要

By using data from multiple instruments, we investigate ionospheric/thermospheric behavior during the period from 21 to 23 June 2015, when three interplanetary shocks (IS) of different intensities arrived at Earth. The first IS was registered at 16:45 UT on 21 June and caused ~50 nT increase in the SYM-H index. The second IS arrived at 5:45 UT on 22 June and induced an enhancement of the auroral/substorm activity that led to rapid increase of thermospheric neutral mass density and ionospheric vertical total electron content at high latitudes. Several hours later, topside electron content and electron density increased at low latitudes on the nightside. The third and much larger IS arrived at 18:30 UT on 22 June and initiated a major geomagnetic storm that lasted for many hours. The storm provoked significant effects in the thermosphere and ionosphere on both dayside and nightside. In the thermosphere, the dayside neutral mass density exceeded the quiet time levels by 300-500%, with stronger effects in the summer hemisphere. In the ionosphere, both positive and negative storm effects were observed on both dayside and nightside. We compared the ionospheric observations with simulations by the coupled Sami3 is Also a Model of the Ionosphere/Rice Convection Model (SAMI3/RCM) model. We find rather good agreement between the data and the model for the first phase of the storm, when the prompt penetration electric field (PPEF) was the principal driver. At the end of the storm main phase, when the ionospheric effects were, most likely, driven by a combination of PPEF and thermospheric winds, the modeling results agree less with the observations.
机译:通过使用来自多种仪器的数据,我们在2015年6月21日至23日的时间内调查电离层/热散,当时不同强度到达地球的行星冲击(IS)。首先是6月21日16:45 UT登记,并造成〜50 nt的yd-h指数增加。第二次举行的第二次达到5:45 UT,诱导了高纬度地导致热散形质量密度和电离层垂直总电子含量快速增加的极光/取代活动。几个小时后,顶部电子含量和电子密度在夜间低纬度下增加。第三个和更大的时间是在6月22日18:30到达,并发起了一个持续数小时的主要地磁风暴。风暴在天空和夜间刺激热圈和电离层中的显着影响。在热层中,天晶体质量密度超过安静的时间水平300-500%,夏季半球效果更强。在电离层中,在天段和夜间旁边观察到阳性和阴性风暴效应。我们将通过偶联的Sami3与模拟进行比较,也是电离层/水稻对流模型(SAMI3 / RCM)模型的模型。当迅速穿透电场(PPEF)是主要驾驶员时,我们在数据和风暴的第一阶段之间找到了良好的一致性。在风暴主阶段结束时,当电离层的效果最有可能被PPEF和热散发风的组合驱动时,造型结果对观察结果较少。

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  • 作者单位

    Department of Planetology and Space Sciences Institut de Physique du Globe de Paris Paris Sorbonne Cité University of Paris Diderot Paris France;

    Department of Planetology and Space Sciences Institut de Physique du Globe de Paris Paris Sorbonne Cité University of Paris Diderot Paris France;

    Plasma Physics Division Naval Research Laboratory Washington DC USA;

    Department of Space Engineering Delft University of Technology Delft Netherlands;

    Department of Space Engineering Delft University of Technology Delft Netherlands;

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  • 原文格式 PDF
  • 正文语种 eng
  • 中图分类 空间物理;
  • 关键词

    period; registered; second;

    机译:期间;注册;第二;

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