高功率高频加热 F2 层引起的顶部电离层等离子体密度扰动的空间结构

IF 0.7 4区 地球科学 Q4 GEOCHEMISTRY & GEOPHYSICS
V. L. Frolov, E. S. Andreeva, A. M. Padokhin
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引用次数: 0

摘要

摘要 该研究分析了低轨道卫星无线电层析成像测量的结果,这些测量是在 SURA 加热设施发射的大功率 O 偏振高频无线电波改变中纬度电离层 F2 层期间激发的地球顶部电离层人工电子密度变化的空间结构。文章探讨了在大功率高频无线电波反射高度附近形成的等离子体密度降低的空腔的特征、由于等离子体从加热区域沿地磁场位移而在顶部电离层形成的等离子体密度增加的导管以及在电离层高度诱发的各种波干扰。此外,还研究了在电离层扰动区中心部分上方的垂直柱中探测到的具有特殊性质的等离子体密度扰动的特性。所研究的不规则现象的大小从几十公里到几百公里不等,其存在区域远远超出了大功率 O 偏振无线电波与电离层等离子体在其反射高度附近发生共振相互作用的区域,在该区域会激发最强烈的人工电离层湍流。
本文章由计算机程序翻译,如有差异,请以英文原文为准。

Spatial Structure of Plasma Density Disturbances in the Topside Ionosphere Caused by High-Power HF Heating of the F2 Layer

Spatial Structure of Plasma Density Disturbances in the Topside Ionosphere Caused by High-Power HF Heating of the F2 Layer

Spatial Structure of Plasma Density Disturbances in the Topside Ionosphere Caused by High-Power HF Heating of the F2 Layer

The study analyzes the results of low-orbital satellite radio tomography measurements of the spatial structure of artificial electron-density variations Earth’s topside ionosphere excited during modification of the F2 layer of the mid-latitude ionosphere by high-power O-polarized HF radio waves emitted by the SURA heating facility. The article considers the characteristics of the cavity with a reduced plasma density that forms near the reflection height of a high-power HF radio wave, ducts with increased plasma density that form in the topside ionosphere due to displacement of plasma from the heated region along the geomagnetic field, and various wave disturbances induced at ionospheric heights. In addition, the properties of detected plasma density disturbances of a special nature in the vertical column above the central part of the disturbed region of the ionosphere are also investigated. The sizes of the studied irregularities are from several tens to several hundreds of kilometers, and the area of their existence goes far beyond the region of resonance interaction of a high-power O-polarized radio wave with ionospheric plasma near its reflection height, where the most intense artificial ionospheric turbulence is excited.

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来源期刊
Geomagnetism and Aeronomy
Geomagnetism and Aeronomy Earth and Planetary Sciences-Space and Planetary Science
CiteScore
1.30
自引率
33.30%
发文量
65
审稿时长
4-8 weeks
期刊介绍: Geomagnetism and Aeronomy is a bimonthly periodical that covers the fields of interplanetary space; geoeffective solar events; the magnetosphere; the ionosphere; the upper and middle atmosphere; the action of solar variability and activity on atmospheric parameters and climate; the main magnetic field and its secular variations, excursion, and inversion; and other related topics.
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