Determination of the Effective Collision Frequency of Electrons in the E and D Regions of the High-Latitude Ionosphere from Analysis of Radio Occultation Measurements

IF 0.6 4区 物理与天体物理 Q4 ASTRONOMY & ASTROPHYSICS
V. N. Gubenko, V. E. Andreev, I. A. Kirillovich, T. V. Gubenko, A. A. Pavelyev, D. V. Gubenko
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引用次数: 0

Abstract

Collisions between electrons and neutral molecules are of special interest for the physics of the Earth’s ionosphere, in particular, for determining the ionospheric conductivity and current systems in the lower ionosphere of the planet, as well as elucidating the role they play in attenuating radio waves propagating inside the D and E regions of the ionosphere. The effective collision frequency of electrons can be estimated from laboratory studies of electron mobility in atmospheric gases in combination with rocket measurements of temperature and particle density in the Earth’s upper atmosphere, or it can be determined independently from analysis of radio occultation data. We have developed a method for reconstructing the vertical profiles of the absorption coefficient of decimeter (wavelength ~19 cm) radio waves by solving the inverse problem of signal absorption in the D and E regions of the Earth’s ionosphere. Based on the analysis of radio occultation data from the FORMOSAT-3/COSMIC satellites, the altitude profiles of the absorption coefficient of decimeter (DM) radio waves in the planet’s ionosphere during the geomagnetic storm on June 22–23, 2015, were determined. It is known that the absorption coefficient at a given fixed frequency is directly proportional to both the electron density and the collision frequency of electrons with ions and neutrals. Using the data on the vertical profiles of the absorption coefficient of DM radio waves and the electron density reconstructed from the analysis of FORMOSAT-3/COSMIC radio occultations, we estimated the effective collision frequency of electrons in the D and E regions of the Earth’s high-latitude ionosphere. The practical significance of studying the frequency of electron collisions and the effects of radio wave absorption in the D and E regions of the planet’s ionosphere is associated with maintaining the uninterrupted operation of space radio communication and navigation systems.

Abstract Image

从掩星测量分析确定高纬度电离层E区和D区电子有效碰撞频率
摘要电子和中性分子之间的碰撞对于地球电离层的物理学具有特殊的意义,特别是对于确定电离层电导率和地球电离层下部的电流系统,以及阐明它们在电离层D和E区域内传播的无线电波衰减中所起的作用。电子的有效碰撞频率可以通过对大气气体中电子迁移率的实验室研究,结合对地球高层大气中温度和粒子密度的火箭测量来估计,或者可以通过对无线电掩星数据的分析独立确定。通过求解地球电离层D区和E区信号吸收逆问题,提出了一种重建分米(波长~19 cm)无线电波吸收系数垂直剖面的方法。基于对FORMOSAT-3/COSMIC卫星掩星数据的分析,确定了2015年6月22日至23日地磁暴期间地球电离层分米(DM)无线电波吸收系数的高度剖面图。已知在给定固定频率下的吸收系数与电子密度和电子与离子和中性离子的碰撞频率成正比。利用DM无线电波吸收系数垂直剖面数据和FORMOSAT-3/COSMIC掩星分析重建的电子密度数据,估算了地球高纬度电离层D区和E区电子的有效碰撞频率。研究行星电离层D区和E区电子碰撞频率和无线电波吸收效应的现实意义与保持空间无线电通信和导航系统的不间断运行有关。
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来源期刊
Cosmic Research
Cosmic Research 地学天文-工程:宇航
CiteScore
1.10
自引率
33.30%
发文量
41
审稿时长
6-12 weeks
期刊介绍: Cosmic Research publishes scientific papers covering all subjects of space science and technology, including the following: ballistics, flight dynamics of the Earth’s artificial satellites and automatic interplanetary stations; problems of transatmospheric descent; design and structure of spacecraft and scientific research instrumentation; life support systems and radiation safety of manned spacecrafts; exploration of the Earth from Space; exploration of near space; exploration of the Sun, planets, secondary planets, and interplanetary medium; exploration of stars, nebulae, interstellar medium, galaxies, and quasars from spacecraft; and various astrophysical problems related to space exploration. A chronicle of scientific events and other notices concerning the main topics of the journal are also presented.
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