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Peculiarities of artificial ionospheric radiation under the action of high-power HF radiowaves, emitted by the SPEAR facility, on the sporadic E layer of the polar ionosphere

机译:在SPEAR设施发射的高功率HF无线电波的作用下,人造电离层辐射在极地电离层零星E层上的特殊性

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The results of the experimental studies of the ionospheric effects originating under the action of high-power HF radiowaves, emitted by the SPEAR heating facility into the sporadic E (s) layer of the polar ionosphere, are presented. The experiment was performed on March 2, 2007, simultaneously at two spaced points: Barentsburg (Spitsbergen, a distance of about 40 km from the SPEAR facility) and Gor'kovskaya observatory near St. Petersburg, located at a distance of about 2000 km from SPEAR. The distributions of the heating signal intensity in the 100 kHz frequency band were measured in Barentsburg. Bistatic backscatter of diagnostic HF signals by small-scale artificial ionospheric irregularities was observed at Gor'kovskaya observatory. Based on an analysis of the experimental data obtained in Barentsburg, it has been found out that a broadband noise-like component originated and additional maximums appeared in the heating signal spectrum. The broadband emission intensity was a factor of 1.5-3 as high as the noise level. The additional maximums were formed in the regions of the positive and negative frequency shift relative to the heating signal frequency and were observed when the heating frequency was lower than the critical frequency of the E (s) layer; e.g., a high-power HF radiowave reflected from E (s) . The expression for determining the frequency shift of the additional maximum in the heating signal spectrum at altitudes of the ionospheric E region, taking into account the ion-electron collision frequency, has been obtained. The heating signal spectrum registration was compared with the observations of small-scale artificial ionospheric irregularities and the trajectory modeling of signals scattered by the considered irregularities. The observation results have been analyzed and interpreted taking into account the magnetic and ionospheric data characterizing the background geophysical conditions.
机译:给出了对由SPEAR加热设备发射到极地电离层零星E层中的高功率HF无线电波作用下产生的电离层效应的实验研究结果。该实验于2007年3月2日在两个间隔的地点同时进行:巴伦斯堡(Spitsbergen,距SPEAR设施约40公里)和圣彼得堡附近的戈尔科夫斯卡亚天文台,距距约2000公里矛。在巴伦斯堡测量了100 kHz频带内加热信号强度的分布。在Gor'kovskaya天文台观察到由小型人工电离层不规则性引起的诊断性HF信号的双基地反向散射。基于对在巴伦斯堡获得的实验数据的分析,发现宽带噪声样分量起源并且在加热信号频谱中出现了其他最大值。宽带发射强度是噪声水平的1.5-3倍。在相对于加热信号频率的正,负频移区域中形成了附加的最大值,并且当加热频率低于E(s)层的临界频率时,可以观察到其他最大值。例如,从E(s)反射的高功率HF无线电波。已经获得了考虑到离子-电子碰撞频率来确定电离层E区域的高度处的加热信号频谱中的附加最大值的频移的表达式。将加热信号频谱配准与小规模人工电离层不规则现象的观测结果以及由所考虑的不规则现象散射的信号轨迹模型进行了比较。考虑到表征背景地球物理条件的磁和电离层数据,对分析结果进行了分析和解释。

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