Quasi-stationary substructure within a sporadic E layer observed by the Low Frequency Array (LOFAR)

A. Wood, G. Dorrian, B. Boyde, R. Fallows, David Themens, M. Mevius, Tim Sprenger, Robert Main, S. Eleri Pryse, S. Elvidge
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Abstract

Observations made with the Low Frequency Array (LOFAR) have been used to infer the presence of variations in a sporadic E layer on a spatial scale of several kilometres and a temporal scale of ~10 minutes. LOFAR stations across the Netherlands observed Cygnus A between 17 UT and 18 UT on 14th July 2018 at frequencies between 24.9 MHz and 64.0 MHz. Variations in the relative signal intensity, together with consideration of geometric optics, were used to infer the presence of a plasma structure. Spatial variations between the stations and the dispersive nature of the observations suggested that this plasma structure was located within the ionosphere. Independent confirmation of the presence of a sporadic E layer, and variation within it, was obtained from observations made by the Juliusruh ionosonde (54.6° N, 13.4° E), which observed reflection of radio waves at an altitude of ~120 km and from frequencies of up to ~6 MHz. The large number (38) of LOFAR stations across the Netherlands together with the sub-second temporal resolution and broadband frequency coverage of the observations enabled the fine details of the spatial variation and the evolution of the structure to be determined. The structure was quasi-stationary, moving at ~12 m s-1, and it exhibited significant variation on spatial scales of a few kilometres. The observations were consistent with the steepening of a plasma density gradient at the edge of the feature over time due to an instability process. A 1-D numerical model showed that the observations were consistent with an electron density enhancement in the sporadic E layer with a density change of 2x1011 m-3 and a spatial scale of several kilometres. Collectively, these results show the ability of LOFAR to observe substructure within sporadic E layers and how this substructure varies with time. They also show the potential value of such datasets to constrain models of instability processes, or to discriminate between competing models.
低频阵列(LOFAR)观测到的零星 E 层内的准稳态子结构
利用低频阵列(LOFAR)进行的观测被用来推断零星 E 层在几公里的空间尺度和 ~10 分钟的时间尺度上是否存在变化。荷兰各地的 LOFAR 站在 2018 年 7 月 14 日 17 UT 至 18 UT 期间以 24.9 MHz 至 64.0 MHz 的频率对天鹅座 A 进行了观测。相对信号强度的变化,加上几何光学的考虑,被用来推断等离子体结构的存在。观测站之间的空间变化和观测的分散性表明,该等离子体结构位于电离层内。朱利叶斯鲁电离层(北纬 54.6°,东经 13.4°)的观测结果独立证实了零星 E 层的存在及其内部的变化。荷兰各地有大量(38 个)LOFAR 观测站,加上观测的亚秒级时间分辨率和宽带频率覆盖范围,使得该结构的空间变化和演变的细节得以确定。该结构是准稳态的,移动速度约为 12 米/秒,在几公里的空间范围内表现出显著的变化。观测结果与该特征边缘的等离子体密度梯度因不稳定过程而随时间陡增一致。一维数值模型显示,观测结果与零星 E 层的电子密度增强一致,密度变化为 2x1011 m-3,空间尺度为几公里。总之,这些结果表明了LOFAR观测零星E层内子结构的能力,以及这种子结构如何随时间变化。它们还显示了此类数据集在约束不稳定过程模型或区分相互竞争的模型方面的潜在价值。
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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