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分解太阳和地磁活动以及季节性依赖关系,以研究 GPS 锁定丢失与电离层湍流之间的关系。

Decomposing solar and geomagnetic activity and seasonal dependencies to examine the relationship between GPS loss of lock and ionospheric turbulence.

机构信息

Dipartimento di Fisica, Universitá di Roma Sapienza, 00185, Rome, Italy.

Istituto Nazionale di Geofisica e Vulcanologia, 00143, Rome, Italy.

出版信息

Sci Rep. 2023 Jun 7;13(1):9287. doi: 10.1038/s41598-023-34727-2.

DOI:10.1038/s41598-023-34727-2
PMID:37286574
原文链接:https://pmc.ncbi.nlm.nih.gov/articles/PMC10247704/
Abstract

Ionospheric irregularities are plasma density variations that occur at various altitudes and latitudes and whose size ranges from a few meters to a few hundred kilometers. They can have a negative impact on the Global Navigation Satellite Systems (GNSS), on their positioning accuracy and even cause a signal loss of lock (LoL), a phenomenon for which GNSS receivers can no longer track the satellites' signal. Nowadays, the study of plasma density irregularities is important because many of the crucial infrastructures of our society rely on the efficient operation of these positioning systems. It was recently discovered that, of all possible ionospheric plasma density fluctuations, those in a turbulent state and characterized by extremely high values of the Rate Of change of the electron Density Index appear to be associated with the occurrence of LoL events. The spatial distributions of this class of fluctuations at mid and high latitudes are reconstructed for the first time using data collected on Swarm satellites between July 15th, 2014 and December 31st, 2021, emphasizing their dependence on solar activity, geomagnetic conditions, and season. The results unequivocally show that the identified class of plasma fluctuations exhibits spatio-temporal behaviours similar to those of LoL events.

摘要

电离层不规则体是发生在不同高度和纬度的等离子体密度变化,其大小从几米到几百公里不等。它们可能对全球导航卫星系统(GNSS)产生负面影响,影响其定位精度,甚至导致信号锁定丢失(LoL),这种现象使得 GNSS 接收器无法再跟踪卫星信号。如今,研究等离子体密度不规则体非常重要,因为我们社会的许多关键基础设施都依赖于这些定位系统的有效运行。最近发现,在所有可能的电离层等离子体密度波动中,那些处于湍流状态且电子密度指数变化率极高的波动似乎与 LoL 事件的发生有关。首次使用 2014 年 7 月 15 日至 2021 年 12 月 31 日期间在 Swarm 卫星上收集的数据重建了中高纬度地区该类波动的空间分布,强调了它们对太阳活动、地磁条件和季节的依赖性。结果明确表明,所识别的等离子体波动类具有与 LoL 事件相似的时空行为。

https://cdn.ncbi.nlm.nih.gov/pmc/blobs/cde6/10247704/43755d52eb7f/41598_2023_34727_Fig7_HTML.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/cde6/10247704/66eba7dd5bd8/41598_2023_34727_Fig1_HTML.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/cde6/10247704/ac47c604e9bc/41598_2023_34727_Fig2_HTML.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/cde6/10247704/e74a328ec709/41598_2023_34727_Fig3_HTML.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/cde6/10247704/1223ffcb295e/41598_2023_34727_Fig4_HTML.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/cde6/10247704/d27923a4a677/41598_2023_34727_Fig5_HTML.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/cde6/10247704/6311b239c52c/41598_2023_34727_Fig6_HTML.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/cde6/10247704/43755d52eb7f/41598_2023_34727_Fig7_HTML.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/cde6/10247704/66eba7dd5bd8/41598_2023_34727_Fig1_HTML.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/cde6/10247704/ac47c604e9bc/41598_2023_34727_Fig2_HTML.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/cde6/10247704/e74a328ec709/41598_2023_34727_Fig3_HTML.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/cde6/10247704/1223ffcb295e/41598_2023_34727_Fig4_HTML.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/cde6/10247704/d27923a4a677/41598_2023_34727_Fig5_HTML.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/cde6/10247704/6311b239c52c/41598_2023_34727_Fig6_HTML.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/cde6/10247704/43755d52eb7f/41598_2023_34727_Fig7_HTML.jpg

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本文引用的文献

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Ionospheric Plasma IRregularities - IPIR - Data Product Based on Data From the Swarm Satellites.电离层等离子体不规则性——基于“蜂群”卫星数据的数据产品
J Geophys Res Space Phys. 2022 Apr;127(4):e2021JA030183. doi: 10.1029/2021JA030183. Epub 2022 Apr 8.
2
Looking for a proxy of the ionospheric turbulence with Swarm data.利用“蜂群”卫星数据寻找电离层湍流的代理指标。
Sci Rep. 2021 Mar 17;11(1):6183. doi: 10.1038/s41598-021-84985-1.