FEATURES OF THE LARGE-SCALE IONOSPHERIC DISTURBANCES GENERATED UNDER THE ACTION OF MONOPULSE OR PERIODIC RADIO-FREQUENCY EMISSIONS FROM A HEATING FACILITY

Q4 Physics and Astronomy
L. Chernogor, Y. Zhdanko, Y. Luo
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Abstract

Subject and Purpose. Considerable attention has traditionally been given to the interaction of high-power radio-frequency emissions with the ionosphere. The great many physical effects taking place within the limits of a powerful (heating) facility’s antenna pattern are subjected here to a thorough and detailed analysis. Also, the application of high-power radio emissions provides a convenient means for studying subsystem coupling in the Earth-atmosphere-ionosphere-magnetosphere system, as well as of generation and propagation of disturbances well beyond the antenna pattern of the transmitter. The present paper has been aimed at analyzing the features revealed by the large-scale ionospheric disturbances as these are generated under the impact of either monopulse or periodic radio-frequency emissions from an HF heating facility. Methods and Methodology. In the course of the experiments, the ionosphere was affected with high power radio frequency emission from the heating facility Sura. The disturbances were diagnosed at a distance of 960 km from the heater, with the aid of a vertical incidence Doppler radar. Results. It has been found that through the period of minimal solar activity the ionospheric disturbances observable at a range about 103 km from the heater did arise as the effective radiated power of the latter approached to 25 MW. The duration of the ionospheric response to the impact of an incident monopulse was equal to the length of that latter, while the quasi-periodic variations shown by the Doppler frequency shift just started to appear. The apparent horizontal speed of the propagating disturbances was found to vary from about 300 m/s to 420 m/s. Note that speed to increase at higher altitudes. The periodic mode of heater operation was accompanied by generation of quasi-periodic disturbances in the electron density, of relative amplitudes about 1% and periods close to the Brunt–Väisälä period. Conclusions. The basic features of Doppler spectrum variations, contained in the signals from a diagnostic radar, have been identified in connection with high-power HF radiation incident on the ionosphere
在加热设备的单脉冲或周期性射频发射作用下产生的大规模电离层扰动的特征
主题和目的。传统上,人们对高功率射频发射与电离层的相互作用给予了相当大的关注。在一个强大的(加热)设施的天线模式范围内发生的许多物理效应,在这里都要进行彻底和详细的分析。此外,高功率无线电发射的应用为研究地球-大气-电离层-磁层系统中的子系统耦合以及远超发射机天线方向图的干扰的产生和传播提供了方便的手段。本文旨在分析在高频加热设备的单脉冲或周期性射频发射的影响下产生的大规模电离层扰动所揭示的特征。方法和方法论。在实验过程中,电离层受到来自加热设备Sura的高功率射频辐射的影响。在垂直入射多普勒雷达的帮助下,在距离加热器960公里处诊断出干扰。结果。已经发现,在太阳活动最小的时期,当加热器的有效辐射功率接近25兆瓦时,在距离加热器约103公里的范围内观测到的电离层扰动确实出现了。电离层对入射单脉冲影响的响应持续时间等于后者的长度,而多普勒频移所显示的准周期变化才刚刚开始出现。发现传播扰动的表观水平速度在300 ~ 420 m/s之间变化。注意,高度越高,速度越快。加热器的周期运行模式伴随着电子密度的准周期扰动的产生,其相对振幅约为1%,周期接近Brunt-Väisälä周期。结论。诊断雷达信号中所包含的多普勒频谱变化的基本特征,已与电离层上的高功率高频辐射有关
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来源期刊
Radio Physics and Radio Astronomy
Radio Physics and Radio Astronomy Physics and Astronomy-Physics and Astronomy (miscellaneous)
CiteScore
0.60
自引率
0.00%
发文量
18
审稿时长
8 weeks
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