探讨将LOFAR和GNSS测量相结合以感知电离层不规则性的可能性

IF 3.4 2区 物理与天体物理 Q2 ASTRONOMY & ASTROPHYSICS
P. Flisek, B. Forte, R. Fallows, K. Kotulak, A. Krankowski, M. Bisi, M. Mevius, A. Froń, C. Tiburzi, M. Soida, Bartosz Śmierciak, M. Grzesiak, B. Matyjasiak, M. Pożoga, B. Dabrowski, G. Mann, C. Vocks, P. Zucca, L. Blaszkiewicz
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Here, a novel methodology for the detection and characterization of ionospheric irregularities is established on the basis of LOFAR scintillation measurements at VHF that takes into account of the lack of ergodicity in the intensity fluctuations induced by scintillation. The methodology estimates the S 4 scintillation index originating from irregularities with spatial scales in the inertial sub-range of electron density fluctuations in the ionosphere. The methodology is illustrated by means of observations that were collected through the Polish LOFAR stations located in Bałdy, Borówiec and Łazy: its validation was carried out by comparing LOFAR VHF scintillation observations with independent GNSS observations that were collected through a high-rate receiver located near the LOFAR station in Bałdy as well as through geodetic receivers from the Polish ASG-EUPOS network. Two case stud-\nies are presented: 31 March 2017 and 28 September 2017. 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引用次数: 0

摘要

电离层等离子体密度的不均匀性影响跨电离层无线电信号,导致信号的振幅和相位出现无线电波闪烁。电离层不规则性引起的闪烁量通常随着无线电波频率的增加而减少。由于电离层影响到各种技术系统(如民航、金融业务)以及低频射电天文学观测,因此必须以比目前更高的精度探测和监测电离层效应。本文在甚高频LOFAR闪烁测量的基础上,考虑到闪烁引起的强度波动缺乏遍历性,建立了一种检测和表征电离层不规则性的新方法。该方法估计了来自电离层电子密度波动惯性子范围内空间尺度不规则性的S4闪烁指数。该方法通过位于巴瓦迪的波兰LOFAR站收集的观测结果进行了说明,Borówiec和Łazy:其验证是通过将LOFAR甚高频闪烁观测值与独立的GNSS观测值进行比较来进行的,这些观测值是通过位于巴迪LOFAR站附近的高速接收机以及波兰ASG-EUPOS网络的大地测量接收机收集的。介绍了两个案例研究:2017年3月31日和2017年9月28日。LOFAR S4观测值与GNSS的TEC闪烁和变化率的独立电离层测量值之间的比较表明,由于无线电波闪烁的频率依赖性,LOFAR和GNSS对电离层结构的敏感性不同。此外,可以注意到LOFAR VHF闪烁的观测可以用于探测中纬度电离层中形成的等离子体结构,包括在空间尺度上发生的电子密度梯度,这些梯度不一定通过传统的全球导航卫星系统测量来检测:所有空间尺度的检测对于电离层过程的正确监测和建模至关重要。因此,除了传统的全球导航卫星系统电离层测量外,LOFAR对电离层结构的不同灵敏度使人们能够扩展对电离层过程的了解。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
Towards the possibility to combine LOFAR and GNSS measurements to sense ionospheric irregularities
Inhomogeneities within the ionospheric plasma density affect trans-ionospheric radio signals, causing radio wave scintillation in the amplitude and phase of the signals. The amount of scintillation induced by ionospheric irregularities typically decreases with the radio wave frequency. As the ionosphere affects a variety of technological systems (e.g., civil aviation, financial operations) as well as low-frequency radio astronomy observations, it is important to detect and monitor iono- spheric effects with higher accuracy than currently available. Here, a novel methodology for the detection and characterization of ionospheric irregularities is established on the basis of LOFAR scintillation measurements at VHF that takes into account of the lack of ergodicity in the intensity fluctuations induced by scintillation. The methodology estimates the S 4 scintillation index originating from irregularities with spatial scales in the inertial sub-range of electron density fluctuations in the ionosphere. The methodology is illustrated by means of observations that were collected through the Polish LOFAR stations located in Bałdy, Borówiec and Łazy: its validation was carried out by comparing LOFAR VHF scintillation observations with independent GNSS observations that were collected through a high-rate receiver located near the LOFAR station in Bałdy as well as through geodetic receivers from the Polish ASG-EUPOS network. Two case stud- ies are presented: 31 March 2017 and 28 September 2017. The comparison between LOFAR S4 observations and independent ionospheric measurements of both scintillation and rate of change of TEC from GNSS reveals that the sensitivity of LOFAR and GNSS to ionospheric structures is different as a consequence of the frequency dependency of radio wave scintillation. Furthermore, it can be noticed that observations of LOFAR VHF scintillation can be utilised to detect plasma structures forming in the mid-latitude ionosphere, including electron density gradients occurring over spatial scales that are not necessarily detected through traditional GNSS measurements: the detection of all spatial scales is important for a correct monitoring and modelling of ionospheric processes. Hence, the different sensitivity of LOFAR to ionospheric structures, in addition to traditional GNSS ionospheric measurements, allows to expand the knowledge of ionospheric processes.
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来源期刊
Journal of Space Weather and Space Climate
Journal of Space Weather and Space Climate ASTRONOMY & ASTROPHYSICS-GEOCHEMISTRY & GEOPHYSICS
CiteScore
6.90
自引率
6.10%
发文量
40
审稿时长
8 weeks
期刊介绍: The Journal of Space Weather and Space Climate (SWSC) is an international multi-disciplinary and interdisciplinary peer-reviewed open access journal which publishes papers on all aspects of space weather and space climate from a broad range of scientific and technical fields including solar physics, space plasma physics, aeronomy, planetology, radio science, geophysics, biology, medicine, astronautics, aeronautics, electrical engineering, meteorology, climatology, mathematics, economy, informatics.
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