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Temporal and spatial variations in ionospheric electron density profiles over South Africa during strong magnetic storms

机译:强磁暴期间南非电离层电子密度分布的时空变化

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Observations from the South African TrigNet global navigation satellite system (GNSS) and vertical total electron content (VTEC) data from the Jason-1 satellite were used to analyze the variations in ionospheric electron density profiles over South Africa before and after the severe geomagnetic storms on 15 May 2005. Computerized ionospheric tomography (CIT) was used to inverse the 3-D structure of ionospheric electron density and its response to the magnetic storms. Inversion results showed that electron density significantly increased at 10:00 UT, 15 May compared with that at the same period on 14 May. Positive ionospheric storms were observed in the inversion region during the magnetic storms. Jason-1 data show that the VTEC observed on descending orbits on 15 May significantly increased, whereas that on ascending orbits only minimally changed. This finding is identical to the CIT result.
机译:来自南非TrigNet全球导航卫星系统(GNSS)的观测和来自Jason-1卫星的垂直总电子含量(VTEC)数据被用于分析在南非发生严重地磁暴前后南非电离层电子密度剖面的变化。 2005年5月15日。计算机电离层层析成像(CIT)用于逆转电离层电子密度的3维结构及其对磁暴的响应。反演结果表明,与5月14日同期相比,5月15日10:00 UT的电子密度显着增加。在电磁风暴期间,在反转区域观测到了正电离层风暴。 Jason-1数据显示,在5月15日下降轨道上观测到的VTEC显着增加,而在上升轨道上观测到的VTEC变化很小。该发现与CIT结果相同。

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