首页> 外文期刊>Journal of Geophysical Research, A. Space Physics: JGR >Formation of polar ionospheric tongue of ionization during minor geomagnetic disturbed conditions
【24h】

Formation of polar ionospheric tongue of ionization during minor geomagnetic disturbed conditions

机译:形成极性电离层的舌头在小地磁扰动电离条件

获取原文
获取原文并翻译 | 示例
           

摘要

Previous investigations of ionospheric storm-enhanced density (SED) and tongue of ionization (TOI) focused mostly on the behavior of TOI during intense geomagnetic storms. Little attention has been paid to the spatial and temporal variations of TOI during weak to moderate geomagnetic disturbed conditions. In this paper we investigate the source and development of TOI during a moderate geomagnetic storm on 14 October 2012. Multi-instrumental observations including GPS total electron content (TEC), Defense Meteorological Satellite Program(DMSP) in situmeasured total ion concentration and ion drift velocity, SuperDARNmeasured polar ion convection patterns, and electron density profiles from the Poker Flat Incoherent Scatter Radar (PFISR) have been utilized in the current analysis. GPS TECmaps showsalient TOI structures persisting for about 5 h over high latitudes of North America on 14 October 2012 in the later recovery phase of the storm when the magnitudes of IMF By and Bz were less than 5 nT. The PFISR electron density profiles indicate that the extra ionization for TEC enhancements mainly occurred in the topside ionosphere with no obvious changes in the bottomside ionosphere and vertical plasma drifts. Additionally, there were no signatures of penetration electric fields in the equatorial electrojet data and upward ion drifts at high latitudes. At the same time, strong subauroral polarization streams with ion drift speeds exceeding 2.5 km/s carried sunward fluxes and migrated toward lower latitudes for about 5° based on the DMSP cross-track driftmeasurements. Based on thosemeasurements, we postulate that the combined effects of initial build-up of ionization at midlatitudes through daytime production of ionization and equatorward (or less poleward than normal daytime) neutral wind reducing downward diffusion along the inclined filed lines, and an expanded polar ion convection pattern and its associated horizontal plasma transport are important in the formation of the TOI.
机译:先前的调查电离层storm-enhanced密度(SED)和舌头电离(钢铁洪流)主要关注的行为在强烈的磁暴的钢铁洪流。已经注意到空间和时间变化的钢铁洪流在弱温和的地磁扰动的条件。本文我们研究源和在一个温和的地磁发展钢铁洪流2012年10月14日风暴。包括GPS观测总电子含量(TEC),国防气象卫星程序(DMSP) situmeasured总离子浓度和离子漂移速度,SuperDARNmeasured极性离子对流模式,从扑克平面和电子密度配置文件非相干散射雷达(PFISR)利用在当前分析。坚持5 showsalient钢铁洪流结构h / 14日北美的高纬度地区2012年10月后的复苏阶段风暴在国际货币基金组织的大小和热晕不到5元,PFISR电子密度资料表明,额外的电离TEC的增强主要发生在上部电离层与没有明显的变化bottomside电离层和垂直等离子体漂移。此外,没有签名的渗透在赤道电场电喷流数据和上行离子漂浮在高纬度。与离子极化流漂移速度超过2.5公里/ s朝着太阳通量和转向低纬度地区大约5°基于DMSP航迹driftmeasurements。基于thosemeasurements,我们假定结合初始积累的影响通过白天电离在情理之中生产的电离和朝赤道方向(或更少向极比正常白天)中性风减少沿斜向下扩散提起线,和一个扩展极性离子对流模式及其相关水平的等离子体运输的形成是很重要的你。

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