首页> 外文期刊>Journal of Geophysical Research. Biogeosciences >Global Ionospheric and Thermospheric Effects of the June 2015 Geomagnetic Disturbances: Multi-Instrumental Observations and Modeling
【24h】

Global Ionospheric and Thermospheric Effects of the June 2015 Geomagnetic Disturbances: Multi-Instrumental Observations and Modeling

机译:2015年6月Geomagnetic扰动的全局电离层和热散,多乐谱观测和建模

获取原文
获取原文并翻译 | 示例
           

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 similar to 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:通过使用来自多台仪器的数据,我们在从期间电离层研究/热层行为21至23日到达地球不同强度的2015年6月,当三个行星际激波(IS)。第一个是被注册在16:45 UT 6月21日,造成类似于在SYM-H指数50 NT的增加。第二个是到达5:45 UT 6月22日和诱导的极光/亚暴活性的增强,导致热层中性质量密度和在高纬度地区电离层垂直电子总含量的快速增加。几个小时后,顶侧的电子内容和电子密度增加在上的阴面低纬度地区。第三和更大的IS到达18:30 UT 6月22日,并启动一个重大的地磁暴持续了几个小时。风暴引发的热层和电离层两个向阳面和阴面显著的影响。在热层中,向阳面中性质量密度300-500%,超过了安静时的水平,在夏季半球效果更强。在电离层中,观察到在两个向阳面和阴面正面和负面影响风暴。我们比较了由耦合Sami3模拟电离层观测也是电离层/对流水稻模型(SAMI3 / RCM)模型的模型。我们找到的数据和风暴的第一阶段的模型,当提示渗透电场(PPEF)是主要的驱动程序之间相当一致。在风暴主相,当电离层效应,最有可能的,通过PPEF和热层风的组合驱动结束时,模拟结果一致少与观测。

著录项

相似文献

  • 外文文献
  • 中文文献
  • 专利
获取原文

客服邮箱:kefu@zhangqiaokeyan.com

京公网安备:11010802029741号 ICP备案号:京ICP备15016152号-6 六维联合信息科技 (北京) 有限公司©版权所有
  • 客服微信

  • 服务号