Planetary wave oscillations in the occurrence time of Equatorial Spread-F

C. Vineeth, L. Jose, T. Pant
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Abstract

This paper presents the role of planetary waves in modulating the occurrence time of Equatorial Spread F (ESF). The investigation has been carried out using the data from the digital Ionosonde and Proton Precession Magnetometer located over Trivandrum, India (8.5° E; 77° N; 0.5° N dip lat.). The analysis shows that the start-time of the ESF during the winter months is modulated significantly by a planetary wave of quasi-16-day periodicity. It is suggested that these waves are propagated to ionospheric altitudes from lower atmosphere through modified electrodynamics since the equatorial electrojet and pre-reversal enhancement were also showed the same oscillations.
赤道扩散- f发生时间内的行星波振荡
本文讨论了行星波对赤道传播波发生时间的调制作用。这项调查是利用位于印度Trivandrum(8.5°E;77°N;0.5°N倾角较晚。分析表明,冬季ESF的开始时间受到周期为16天的行星波的显著调制。由于赤道电喷和反转前增强也表现出相同的振荡,因此这些波从低层大气通过修正的电动力学传播到电离层高度。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
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