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METHOD OF DETERMINATION OF PARAMETERS OF SOLAR WIND IN NEAR-EARTH SPACE

机译:地球空间太阳风参数的确定方法

摘要

The invention relates to methods for studying interplanetary plasma in near-Earth space. The purpose of the invention is to obtain, in addition to the usual parameters determined by the interplanetary plasma radio transmission method, the distance L from the Earth to the region of increased turbulence of the solar wind and perpendicular to the direction of the Moon. The invention relates to radar and communication, namely to radio physical interplanetary plasma studies. in near-Earth space, designed to control the region of increased turbulence of the solar wind at the outer boundary of the Earth’s magnetosphere and can be used l diagnosing disturbances of the solar wind on the Earth -Luna. The aim of the invention is to measure the distance to the region of increased turbulence of the solar wind and the perpendicular to the ray of sight of the component of the solar wind speed. The component of the solar wind velocity Vt in this region on the Earth-Moon route. This is ensured by the fact that radio signals are emitted from the surface of the Earth in the direction of the Moon in the range of frequencies at which the period of libration fluctuations of the intensity of signals reflected from the Moon exceeds the arrival time of the moon radio echo. The intensity of the lunar radio echo is measured, its autocorrelation function is calculated, its fluctuations are determined, and L and Vi are determined by the formulas: LD - 0.5 С С Т0 Vi -57- (D - 0.5 С TO) / fD where D is the distance from Earth to the Moon; C is the speed of light; T0 is the ACF side maximum argument; Ar is the width of the lateral maximum of the ACF at 0.5; f is the frequency of the emitted radio signal. 1 il. CO FIG. 1 shows the structural electrical circuit of the device. The device contains a transmitter 1, antenna 2, receiver 3, antenna 4, quadratic detector 5, correlometer 6, unit 7, synchronization. The essence of the invention is as follows. Radio signals are emitted from the Earth in the direction of the Moon, radio signals reflected from the Moon are received, their autocorrelation function (ACF) of intensity fluctuations is measured. ACF intensity fluctuations reflected from the moon by radio signals of the ground VI
机译:本发明涉及在近地空间中研究行星际等离子体的方法。本发明的目的除了获得由行星际等离子体无线电传输方法确定的通常参数之外,还获得从地球到太阳风湍流增加的区域并垂直于月球方向的距离L。本发明涉及雷达和通信,即涉及无线电物理行星际等离子体研究。在近地空间中,该系统旨在控制地球磁层外边界处太阳风湍流增加的区域,可用于诊断太阳风对月球-月神的干扰。发明内容本发明的目的是测量到太阳风湍流增加的区域的距离以及垂直于太阳风速分量的视线的距离。地月路线上该区域中太阳风速Vt的分量。这是通过以下事实保证的:无线电信号是从地球表面沿月球方向发射的,其频率范围是从月球反射的信号的强度的自由度波动的周期超过了到达时间。月球广播回声。测量月球无线电回波的强度,计算其自相关函数,确定其波动,并通过以下公式确定L和Vi:LD-0.5СТ0Vi -57-(D-0.5СTO)/ fD D是从地球到月球的距离; C是光速; T0是ACF侧的最大自变量; Ar是ACF的横向最大值的宽度,为0.5; f是发射的无线电信号的频率。 1升CO图。图1示出了装置的结构电路。该设备包括发射机1,天线2,接收机3,天线4,二次检波器5,相关仪6,单元7,同步。本发明的实质如下。无线电信号从地球沿月球方向发射,接收到从月球反射的无线电信号,并测量其强度波动的自相关函数(ACF)。地面VI的无线电信号从月球反射的ACF强度波动

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