Properties of large-scale TIDs observed in Central China

This paper investigates the large scale travelling ionospheric disturbances (LSTIDs) using the observation data of an HF Doppler array located in Central China. The data observed in a high solar activity year (year 1989) are analyzed to obtain the main propagation parameters of LSTIDs such as period, horizontal phase velocity and propagating direction. Results are outlined as follows: Most of the LSTIDs propagate southward; others tend to propagate northward, mostly in summer; dispersion of most LSTIDs is matched with that of Lamb pseudomode, while others have the dispersion of long period gravity wave mode. The horizontal phase velocities of these two modes are about 220 and 450 m/s respectively. The analysis shows that LSTIDs are strongly pertinent to solar activity and space magnetic storms; thus the results presented here are significant for the research of ionospheric weather in mid-low latitude region.     

江汉平原上空QTEC变化特征的统计分析

提出了一种观测台网用多接收机性能一致性的标定方法，并利用江汉平原GPS接收台网的观测数据，分析了该地区上空QTEC的日变化、季节变化、年变化和逐年变化的统计特征．标定结果表明，不同接收机之间的仪器偏差是从双频GPS卫星信标推算QTEC的主要误差来源之一，必须校正．统计分析证实，江汉平原上空QTEC的日变化特征同时受电离层和等离子层控制，其年变化以半年周期为主，峰值和谷值分别出现在两分点和两至点附近，QTEC值的逐年变化从太阳活动峰年到低年逐年下降，与以太阳黑子数为代表的太阳活动密切相关．     

Focusing-defocusing phenomena of radio echo signal after passage of the morning solar terminator

Summary Campaign results of high-repetition ionospheric soundings, performed at the ionospheric station of Rome using a Digisonde 128P, are presented. We introduce an index derived from run rapid ionograms that can be used to detect oscillations of isodensity surfaces ofF ionospheric region started by morning solar terminator.     

人工扰动电离层仿真系统的设计与实现

设计并开发了一种人工扰动电离层仿真系统．建立了数值模型，规划出系统总体构造，在实现过程中引入VC、VF混合编程的概念，以达到两种语言优势互补的目的．文中详细论述了VC、VF混合编程对于数据的处理，生成Fortran的动态链接库，以及在VC中调用生成库的技术．通过仿真模拟，得出了电离层加热过程中电子密度、电子温度等随时间演化的规律，及发射电波频率、功率对加热效果的影响．试用证明，该系统有效地模拟了电离层人工扰动的状态，为在我国实施加热工程提供了可靠的科学依据．     

A model for the normal ionosphere over Rome

Summary Some results of statistical analyses on data from the Rome ionospheric station during the period 1948–1983 are shown as a model of the normal ionosphere over Rome.

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Riassunto Si presenta un modello della ionosfera normale su Roma ottenuto con l'analisi statistica dei dati provenienti dalla locale stazione ionosferica lungo il periodo 1948–1983.

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Резюме Предлагается модель нормальной ионосферы на Пимом на основе статистического анализа данных, полученных в Риме на ионосферной станциqi в течение 1948–1983 г.г.

     

The upper atmosphere as a parallel combination of three variable bandpass filters

Summary We show that the upper atmosphere acts as a parallel combination of three main variable bandpass filters whose bandwidths extend from ∼10¹³ to ∼10¹⁵ Hz, ∼3 MHz to ∼10 GHz and ∼40 Hz to ∼10 kHz. The transmission coefficient of the first bandwidth increases as the intensity of the incident electromagnetic radiation within its passband increases. One consequence of the latter is that the eccentricity effects of the Earth's orbital geometry are (stochastically) amplified. This apparently explains why the 100 000 year eccentricity cycle cannot be predicted by the Milankovitch version of the astronomical theory or any other version that involves a linear response. Revised version of a paper presented at an International Symposium on ?Environmental Protection? held at Dar es Salaam, Tanzania from 6 to 15 May 1988.     

Electromagnetic radiation from a conducting tether moving in the ionosphere

Summary We set up a model to compute electromagnetic radiation associated with the motion of a conductor through a magnetized plasma. Calculations are carried out, in the framework of cold-plasma theory, for radiation near the ion cyclotron frequency. Results are applied to the TSS (Tethered Satellite System) project presently under development.

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Riassunto S’imposta il formalismo generale per il calcolo della radiazione elettromagnetica associata con il moto di un conduttore in moto attraverso un plasma magnetizzato. I calcoli sono poi fatti specificamente per la radiazione nelle vicinanze della frequenza di ciclotrone degli ioni. I risultati sono applicati ai parametri del progetto spaziale TSS (Tethered Satellite System) che è attualmente in fase di sviluppo.

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Резюме Мы предлагаем модель для вычисления электромагнитного излучения, связанного с движением проводника через намагниченныю плазму. Вычисления проводятся в рамках теории холодной плазмы для изучения вблизи ионной циклотронной частоты. Полученные результаты применяются к ТСС (связанная система спутников), проект которой разрабатывается в настояцее время.

     

On the effect of electron-mass variation in numerical simulations of the Farley-Buneman instability

The Farley-Buneman instability is the plasma instability in the E region of the Earth’s ionosphere. Many studies on instability simulations use algorithms based on the particle method, which has many shortcomings. In particular, the solutions obtained with this method involve numerical noises owing to a finite number of the particles, since the electron mass is increased in order to reduce the computational complexity of the algorithm. In this study, the effect of an increase in the electron mass on the qualitative and quantitative characteristics of the instability development process are considered. For this purpose, a software package developed on the basis of a mathematical model consisting of the Poisson equation for the electric potential, the fluid equation for electrons, and the kinetic equation for ions is used. The equations are solved numerically, which makes it possible to avoid the problems inherent in the particle method. An important result obtained in this paper is that even a slight increase in the electron mass leads to a considerable variation of the instability development parameters. This variation manifests itself as an increase in the wavelength of plasma fluctuations and a decrease in the strength of the turbulent electric field.