Analysis of Ionospheric Zonal Irregularity Velocity Under Low Latitude During Solar Maxima 24

Matheus Henrique Monteiro de Oliveira, Jonas de Sousa dos Santos, Alison de Oliveira Moraes, M. Abdu, César Buchile Abud De Oliveira, L. Salles
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Abstract

Ionospheric scintillation have their origin in plasma irregularities that cause rapid fluctuations of phase and amplitude in transmitted signals. The applied methodology uses data provided by GPS Ephemeris and scintillation monitors as input to estimate plasma bubbles drift velocities. Results for a low-latitude station in Brazil are consistent with bibliography and indicate the reliability of the method and its usage as a tool to analyze large data to select samples for deeper scintillation studies.
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太阳极大期24低纬度下电离层纬向不规则速度分析
电离层闪烁起源于等离子体的不规则性,这种不规则性会引起传输信号中相位和幅度的快速波动。应用的方法使用GPS星历和闪烁监测器提供的数据作为输入来估计等离子体气泡的漂移速度。巴西一个低纬度观测站的结果与参考文献一致,表明了该方法的可靠性,并可作为分析大数据以选择样本进行更深层次闪烁研究的工具。
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