N. Blagoveshchenskaya, T. D. Borisov, A. Kalishin, I. M. Egorov, G. A. Zagorskyi, A. S. Kovalev
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However, the results of experiments carried out by AARI researchers at the EISCAT/Heating facility (Tromsø, Norway) have clearly demonstrated for the first time that X-polarized HF pump waves are able to produce artificial ionosphere disturbances which may be much stronger compared with O-mode disturbances. This opens up new possibilities for the investigation of nonlinear phenomena and ionospheric disturbances in the upper ionosphere, leading to the development of technologies allowing one to observe the processes in the Arctic zone ionosphere. In contrast to the traditional investigations of artificial ionospheric disturbances induced by O-mode HF pump waves, X-mode disturbances in the upper ionosphere are poorly investigated, the mechanisms of their generation are not understood. Therefore, such investigations require serious experimental and theoretical development. We present investigation results of the influence of the HF Phased Array beam width at the EISCAT/Heating facility (Tromsø, Norway) on the features of artificial disturbances in the high latitude upper (F-region) ionosphere induced by powerful HF radio waves. The paper analyzes the features, behavior, and spatial structure of electron density and temperature (Ne and Te), Langmuir and ion-acoustic plasma waves, artificial field-aligned irregularities (AFAIs), and narrowband (±1кHz relative to heating frequency) stimulated electromagnetic emission (NSEE) induced by X-mode HF pumping by phased Arrays with a narrow beam width of 5–6° (A1) and a wide beam width of 10–12° (at — 3 dB level) (A3). It is shown that the spatial size in the north-south direction of the Neducts and HF-enhanced plasma and ion lines (HFPL and HFIL) depends on the width of the HF Heating facility antenna beam. It corresponds to the angle width of 7° for the A3 antenna and 4° for A1, which is approximately two times less than the width of th pattern of A3 and A1. The relationship between the Ne duct transverse size and the size of the region occupied by the X-mode artificial irregularities is found. It has been established that the intensities of all the discrete components in the NSEE spectra are 10–20 dB higher when a powerful X-wave is emitted to the antenna A1, providing ERP = 820 MW, compared to radiation to the antenna A3, providing ERP = 230 MW. A comparison is made of the influence of the radiation pattern width of the antennas A1 and A3 on the characteristics of disturbances during O- and X-mode HF pumping. It is shown that Ne ducts and narrow band stimulated electromagnetic emission during O-mode heating, at frequencies below the critical frequency of the F2 layer, are not excited at all when the pump wave is emitted by both antennas A1 and A3. However, perturbations in the electron temperature, AFAI intensity, and the size of the region occupied by AFAIs are greater during O-mode heating than during X-mode heating.","PeriodicalId":505647,"journal":{"name":"Arctic and Antarctic Research","volume":"28 6","pages":""},"PeriodicalIF":0.0000,"publicationDate":"2023-12-09","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"0","resultStr":"{\"title\":\"Comparison of features of phenomena in the high latitude ionospheric F-region induced by powerful HF radio waves radiated by antennas with narrow and wide beam patterns\",\"authors\":\"N. Blagoveshchenskaya, T. D. Borisov, A. Kalishin, I. M. Egorov, G. A. Zagorskyi, A. S. 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However, the results of experiments carried out by AARI researchers at the EISCAT/Heating facility (Tromsø, Norway) have clearly demonstrated for the first time that X-polarized HF pump waves are able to produce artificial ionosphere disturbances which may be much stronger compared with O-mode disturbances. This opens up new possibilities for the investigation of nonlinear phenomena and ionospheric disturbances in the upper ionosphere, leading to the development of technologies allowing one to observe the processes in the Arctic zone ionosphere. In contrast to the traditional investigations of artificial ionospheric disturbances induced by O-mode HF pump waves, X-mode disturbances in the upper ionosphere are poorly investigated, the mechanisms of their generation are not understood. Therefore, such investigations require serious experimental and theoretical development. We present investigation results of the influence of the HF Phased Array beam width at the EISCAT/Heating facility (Tromsø, Norway) on the features of artificial disturbances in the high latitude upper (F-region) ionosphere induced by powerful HF radio waves. The paper analyzes the features, behavior, and spatial structure of electron density and temperature (Ne and Te), Langmuir and ion-acoustic plasma waves, artificial field-aligned irregularities (AFAIs), and narrowband (±1кHz relative to heating frequency) stimulated electromagnetic emission (NSEE) induced by X-mode HF pumping by phased Arrays with a narrow beam width of 5–6° (A1) and a wide beam width of 10–12° (at — 3 dB level) (A3). It is shown that the spatial size in the north-south direction of the Neducts and HF-enhanced plasma and ion lines (HFPL and HFIL) depends on the width of the HF Heating facility antenna beam. 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引用次数: 0
摘要
在天然自由等离子体(电离层)中进行物理实验,利用向高纬度上电离层(F 区)有控制地注入强大的高频无线电波(高频泵波),可以研究各种非线性现象。通常使用普通(O 模)极化的高频泵波来改变上电离层(F 区)。这是由于非凡(X 模)极化高频泵浦波的反射高度大大低于 O 极化高频泵浦波的反射高度和静电等离子体波的高度。因此,它们无法产生这种波,也就无法引起人造等离子体湍流和伴随现象。然而,AARI 研究人员在 EISCAT/加热设施(挪威特罗姆瑟)进行的实验结果首次清楚地表明,X 极化高频泵波能够产生人工电离层扰动,这种扰动可能比 O 模式扰动强得多。这为研究电离层上部的非线性现象和电离层扰动提供了新的可能性,有助于开发能够观测北极区电离层过程的技术。与对 O 模式高频泵波引起的人工电离层扰动的传统研究不同,对上电离层 X 模式扰动的研究很少,对其产生机制也不了解。因此,这类研究需要认真的实验和理论发展。我们介绍了 EISCAT/加热设施(挪威特罗姆瑟)的高频相控阵波束宽度对强力高频无线电波诱发的高纬度上层(F 区)电离层人工扰动特征的影响的研究结果。论文分析了电子密度和温度(Ne 和 Te)、朗缪尔和离子声等离子体波、人工场对齐不规则现象(AFAIs)以及窄带(相对于加热频率为 ±1кHz)刺激电磁辐射(NSEE)的特征、行为和空间结构,这些特征、行为和空间结构是由相控阵(X-mode HF pumping by phased Arrays with a narrow beam width of 5-6° (A1) and a wide beam width of 10-12° (at - 3 dB level) (A3))诱发的。结果表明,在南北方向上,Neducts 和高频增强等离子体和离子线(HFPL 和 HFIL)的空间大小取决于高频加热设施天线波束的宽度。A3 天线的角宽为 7°,A1 天线的角宽为 4°,大约是 A3 和 A1 图案宽度的两倍。发现了 Ne 管道横向尺寸与 X 模式人工不规则所占区域大小之间的关系。已经确定,与向天线 A3 辐射(ERP = 230 MW)相比,向天线 A1 辐射(ERP = 820 MW)时,NSEE 频谱中所有离散成分的强度要高 10-20 dB。比较了天线 A1 和 A3 的辐射模式宽度对 O 模式和 X 模式高频抽运期间干扰特性的影响。结果表明,在 O 模式加热过程中,频率低于 F2 层临界频率的 Ne 管道和窄带受激电磁发射在天线 A1 和 A3 发射泵波时根本不会受到激励。然而,在 O 模式加热期间,电子温度、AFAI 强度和 AFAI 所占区域大小的扰动要大于 X 模式加热期间。
Comparison of features of phenomena in the high latitude ionospheric F-region induced by powerful HF radio waves radiated by antennas with narrow and wide beam patterns
Physical experiments in natural free plasma (ionosphere) using controlled injection of powerful HF radio waves (HF pump waves) into the high latitude upper (F-region) ionosphere allow the investigation of various nonlinear phenomena. HF pump waves with ordinary (O-mode) polarization are commonly used for the modification of the upper ionosphere (F-region). This is due to the fact that extraordinary (X-mode) polarized HF pump waves are reflected from altitudes significantly below the reflection altitude of the O-polarized HF pump wave and the altitude of electrostatic plasma waves. Because of that they are not able to generate such waves or, as a consequence, cause artificial plasma turbulence and accompanying phenomena. However, the results of experiments carried out by AARI researchers at the EISCAT/Heating facility (Tromsø, Norway) have clearly demonstrated for the first time that X-polarized HF pump waves are able to produce artificial ionosphere disturbances which may be much stronger compared with O-mode disturbances. This opens up new possibilities for the investigation of nonlinear phenomena and ionospheric disturbances in the upper ionosphere, leading to the development of technologies allowing one to observe the processes in the Arctic zone ionosphere. In contrast to the traditional investigations of artificial ionospheric disturbances induced by O-mode HF pump waves, X-mode disturbances in the upper ionosphere are poorly investigated, the mechanisms of their generation are not understood. Therefore, such investigations require serious experimental and theoretical development. We present investigation results of the influence of the HF Phased Array beam width at the EISCAT/Heating facility (Tromsø, Norway) on the features of artificial disturbances in the high latitude upper (F-region) ionosphere induced by powerful HF radio waves. The paper analyzes the features, behavior, and spatial structure of electron density and temperature (Ne and Te), Langmuir and ion-acoustic plasma waves, artificial field-aligned irregularities (AFAIs), and narrowband (±1кHz relative to heating frequency) stimulated electromagnetic emission (NSEE) induced by X-mode HF pumping by phased Arrays with a narrow beam width of 5–6° (A1) and a wide beam width of 10–12° (at — 3 dB level) (A3). It is shown that the spatial size in the north-south direction of the Neducts and HF-enhanced plasma and ion lines (HFPL and HFIL) depends on the width of the HF Heating facility antenna beam. It corresponds to the angle width of 7° for the A3 antenna and 4° for A1, which is approximately two times less than the width of th pattern of A3 and A1. The relationship between the Ne duct transverse size and the size of the region occupied by the X-mode artificial irregularities is found. It has been established that the intensities of all the discrete components in the NSEE spectra are 10–20 dB higher when a powerful X-wave is emitted to the antenna A1, providing ERP = 820 MW, compared to radiation to the antenna A3, providing ERP = 230 MW. A comparison is made of the influence of the radiation pattern width of the antennas A1 and A3 on the characteristics of disturbances during O- and X-mode HF pumping. It is shown that Ne ducts and narrow band stimulated electromagnetic emission during O-mode heating, at frequencies below the critical frequency of the F2 layer, are not excited at all when the pump wave is emitted by both antennas A1 and A3. However, perturbations in the electron temperature, AFAI intensity, and the size of the region occupied by AFAIs are greater during O-mode heating than during X-mode heating.