基于张衡一号卫星的电力线工频电场背景噪声时空分布特征研究

      Research on the spatiotemporal characteristics of electric field background noise of power line emission based on CSES satellite observation

      • 摘要: 卫星观测地面电力系统产生的电力线工频辐射(power line emission, PLE)近年来饱受关注。为了更准确的识别和研究电离层中的PLE,工频电场背景噪声时空分布特征研究同样至关重要。本研究通过张衡一号卫星(China Seismo-Electromagnetic Satellite, CSES)电场仪2019—2021收集的极低频(extremely low frequency, ELF)频段的电场数据,分析50/60 Hz的电离层夜间(2:00LT)和日间(14:00LT)电场背景噪声时空变化特征,发现全球工频电场背景噪声主要来源自下而上的闪电活动,闪电密度大的区域,电离层工频电场背景噪声强,并且夜间远大于日间,与地磁活动相关性较弱。此外,闪电密度大的区域,工频电场背景噪声存在明显的周期性变化特征;闪电密度小的区域,工频电场背景噪声的周期性变化不显著。电离层工频背景噪声时空分布除了受到源的强度和低电离层电子密度的影响,还会受到地磁场构型的影响,磁纬越高,闪电信号越容易进入电离层。因此电离层工频背景噪声会存在年、季节等时间及纬度、经度等空间复杂变化特征。

         

        Abstract: The power line emission (PLE) generated by the ground power system observed by satellite has attracted much attention in recent years. To enhance the precision in identifying and researching the PLE phenomenon in the topside ionosphere, the study of the spatiotemporal distribution characteristics of the power frequency electric field background noise is also crucial. This study used extremely low frequency (ELF) electric field data collected by the China Seismo-Electromagnetic Satellite (CSES) from 2019 to 2021 to analyze the spatiotemporal variation characteristics of 50/60Hz ionospheric electric field background noise at 2:00LT during the night and 14:00LT during the day. It is found that the global power frequency electric field background noise mainly comes from bottom-up lightning activity. In areas with high lightning density, the ionospheric power frequency electric field background noise is strong, and the night side is much larger than the day side, and the correlation with geomagnetic activity is weak. In addition, in areas with high lightning density, the power frequency electric field background has obvious periodic variation characteristics; in areas with low lightning density, the periodic variation of the power frequency electric field background is not significant. The temporal and spatial distribution of the ionospheric power frequency background noise is affected not only by the intensity of the source and the electron density of the lower ionosphere, but also by the configuration of the geomagnetic field. The higher the magnetic latitude, the easier it is for lightning signals to enter the ionosphere. Therefore, the ionospheric power frequency background noise will have complex variation characteristics in time such as the year and season, and in space such as latitude and longitude.

         

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