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利用高频返回散射技术探测远地核爆炸电离层效应 总被引：3，自引：0，他引：3
本文叙述利用高频返回散射技术探测我国1976年的一次低空大当量核爆炸电离层效应的结果。返回散射探测设备设于离爆炸点2205km的新乡。本文得到了核爆炸产生的附加电离区和电离层扰动的参数。这些结果与爆炸区附近其他手段观测的结果相符。 相似文献
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高频天波返回散射探测作为重要的电离层探测手段,能够实现遥远区域电离层空间上的连续监测,探测获取的返回散射扫频电离图显示了探测频率-群路径-回波能量三者之间的关系.由于电离图包含了探测路径上的电离层状态信息,通过对其反演可以实时获取大面积范围的电离层参数.本文提出了一种基于解空间约束的返回散射前沿反演算法,能够重构电离层水平不均匀结构.针对反演非线性问题,采用Newton-Kontorovich方法进行求解,同时又引入了求解不适定问题的Tikhonov正则化方法,有益于解的稳定性和唯一性.利用模拟数据和实测数据分别对本文建立的算法进行了验证,并与Fridman和Fridman于1994年提出的反演方法进行了对比.结果表明,本文算法反演结果稳定,对返回散射前沿判读误差不敏感,与Fridman和Fridman 1994年方法相比,本文方法对电离层局部精细结构反演更加准确,具有较高的反演精度.本文提出的算法不但能够反演白天和夜间这种电离层较平稳时期的电离层状态,而且对于日出/日落时段等电子浓度分布变化较快情形下的电离层,也有很好的反演效果,表明了该算法在处理复杂多变的实际探测的返回散射电离图中的应用价值. 相似文献
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本文建立了一个中纬电离层E层理论模式. 该模式从NO+,O２＋,O+和N２＋这四种主要离子的连续性方程出发,通过数值模拟得到中纬电离层E层电子和各种离子密度随时间和高度的变化情况. 计算结果能较好地反映出E层电子密度峰值（NmE）或E层临界频率（foE）的日变化、季节变化以及随太阳活动的变化趋势. 将模式的计算结果与武汉地区测高仪的观测数据进行比较,结果证明模式能够较为客观地反映中纬电离层E层的实际形态. 针对以往电离层E层理论模式存在的主要问题,本文还进一步讨论了几种重要因素,包括二次离化源,λ<150?谱段的辐射通量,吸收截面以及NO分布对于模式计算结果的影响. 相似文献
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目前普遍认为Rg_S散射是地下核爆炸短周期Lg波的主要能量来源,其主要依据为由线性偶极补偿源（CLVD）激发的Rg波谱的低谷点随深度变化的特征与区域震相Lg波谱的低谷点随深度变化的特征具有一致性. 本文利用简正振型理论,分析了Rg波谱中低谷点的形成机理,给出了各种速度模型下CLVD源深度与低谷点频率之间的关系,并分析了利用公式hCLVD=V/(16fNull)估计震源深度的局限性. 本文的研究结果进一步支持了CLVD源是激发Lg波的主要因素的观点,并得到重要结论：CLVD源形式下的本征位移函数及其导数的叠加所形成的极小值,即源的空间分布特征,是形成Rg波低谷点的原因,而不能仅用水平向基频本征位移函数过零点来解释. 相似文献
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利用分别由Love波和Rayleigh波得到的S波速度结构的差值（VSH-VSV）对中国大陆及邻区海域（70°E～145°E，15°N～55°N）地壳上地幔中的偏振各向异性进行研究.初步研究结果表明，各向异性在空间分布上存在不均匀性：（1）在小于150 km的深度范围内，VSH>VSV的各向异性体占主导地位，反映出在地球的浅部岩石圈内的水平应力作用及软流圈顶部物质的水平向流动对各向异性的形成起主导作用.在大陆地区，各向异性的强度随深度有显著变化.上地壳和上地幔盖层中的各向异性普遍较弱，而在流变性较强的下地壳和软流圈存在较大范围的各向异性.这一现象说明下地壳在岩石圈变形中可能有解耦作用.（2）在大于200 km深度的软流圈下部主要表现为VSH<VSV的各向异性，说明地幔物质垂直运动相对占优势地位.（3）在中国大陆东部可以看出一个大致趋势：在构造比较稳定的地区，岩石圈中VSH>VSV的各向异性比较显著，而软流圈中VSH<VSV的各向异性较弱；在构造活动比较强烈的地区，软流圈中VSH<VSV的各向异性占主导地位.（4）印度板块低角度向青藏高原下俯冲影响了中国大陆西部地区各向异性的特征.印度板块向北运动水平挤压中国西部大陆，使得物质定向重结晶，从而在岩石圈下部产生显著的VSH>VSV各向异性. 相似文献
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运用台风移动涡旋影响域统计分析动态区域序列概念，采用 3个目标台风卫星TBB资料 ，对台风螺旋云带波列结构特征进行了功率谱合成分析。研究结果揭示出台风涡旋中心与周 边区域对流云的相关场呈螺旋带波状特征；台风影响域螺旋波亦表现出显著次天气、中尺度 波动特征，其波动周期尺度及其传播相速可类似重力内波与涡旋Rossby波，即周期呈双峰特 征，为大于6h与24h左右时间尺度；螺旋波高、低空流型特征与台风的维持、发展结构特征 相关；扰动TBB场时间偏差分布呈类似涡旋Rossby波螺旋波列，其波列路径与涡 旋Rossby波传播特征相似，并提出了台风涡旋螺旋波结构模型。 相似文献
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G.S. Bochkarev 《Journal of Atmospheric and Solar》1997,59(18):2295-2304
Variations of HF probe radio wave parameters caused by the influence on the ionosphere of oblique powerful HF radiowaves are analysed. The analysis is made on the data obtained from the original experiments carried out on single-hop paths in the middle and subauroral latitudes. Powerful and probe waves with some difference in frequency were chosen near MUF and were transmitted in the same direction. The polar diagrams of both transmitting systems overlapped in both the horizontal and vertical planes. The results obtained indicate that the ionospheric plasma parameters can be varied by powerful oblique HF radiowaves under certain geophysical conditions. 相似文献
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V. D. Tereshchenko E. B. Vasil’ev O. F. Ogloblina V. A. Tereshchenko 《Geomagnetism and Aeronomy》2006,46(5):661-666
The results of the observations, using partial reflections, of the lower ionosphere over Tumannyi station in the Murmansk region (69.0° N, 35.7° E) during strong solar flares on January 15–20, 2005, are presented. The structure of the D region of the polar ionosphere and the effects of X-ray flares and fluxes of high energy protons on this region are considered. The anomalous values of electron density in the lower part of the D region, unusually low values of the height of the lower ionospheric boundary, complete or partial absorption of short and medium radiowaves, and bursts of the meter cosmic radio emission were detected during solar disturbances. 相似文献
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Response of mesospheric ozone to the heating of the lower ionosphere by high-power HF radio emission
Yu. Yu. Kulilov V. L. Frolov G. I. Grigor’ev V. M. Demkin G. P. Komrakov A. A. Krasilnokov V. G. Ryskin 《Geomagnetism and Aeronomy》2013,53(1):96-103
We detected a decrease in the intensity of microwave radiation at the atmospheric ozone line at a frequency of 110836.04 MHz during ionospheric modification by high-power HF radiowaves radiated by the Sura Ionospheric Heating Facility. The obtained experimental data allowed us to hypothesize that this effect was caused by the fact that mesospheric ozone was affected by internal gravity waves generated in the E region of the ionosphere during its high-power HF radiowave heating. 相似文献
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N. P. Danilkin G. A. Zhbankov S. V. Zhuravlev N. G. Kotonaeva 《Geomagnetism and Aeronomy》2014,54(4):468-479
Further development of the method of transionospheric radiosounding of the ionosphere in the range of its plasma frequencies is presented. The trajectories of radiowaves with a reflection from the Earth are newly included in the consideration. A modeling of the transionospheric radiosounding was performed in conditions of an irregular ionosphere including moderate-dimensional irregularities with drawing possible trajectories, as well as the obtainment and analysis of the corresponding transionograms. 相似文献
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T. D. Borisova N. F. Blagoveshchenskaya V. A. Kornienko M. T. Rietveld 《Geomagnetism and Aeronomy》2007,47(1):76-84
The method for estimating the behavior of the ionospheric irregularity motion vector in the artificially disturbed HF ionospheric region has been proposed, and this behavior has been analyzed based on the simultaneous Doppler observations performed on several paths using the method of bi-static backscatter of diagnostic HF signals by small-scale artificial ionospheric irregularities. The Doppler measurements were performed during the modification of the auroral ionosphere by powerful HF radiowaves emitted by the EISCAT heating facility (Tromsø, Norway). It has been obtained that the dynamics of the ionospheric irregularity directions in the F region, calculated based on the Doppler measurements of the total vector of the ionospheric irregularity velocity above the Tromsø EISCAT radar at a frequency of 931 MHz, is in satisfactory agreement with such calculations performed using the three-position method. 相似文献
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Ya. V. Drobzheva V. M. Krasnov O. I. Sokolova 《Journal of Atmospheric and Solar》2003,65(16-18):1385-1392
In this paper we present a model, which describes the propagation of acoustic impulses produced by flight of rockets through a model terrestrial atmosphere, and effect of these impulses onto the ionosphere above a rocket. We show, that experimentally observed ionospheric disturbances with duration about 300 s cannot be explained by effect of acoustic impulses onto the ionosphere. We have calculated parameters of a blast wave produced by launch vehicle on the ionospheric heights. It was shown that the blast wave is intense and this wave can generate great disturbance of electron density. The disturbance of electron density can exceed the ambient electron density in 2.6 times. We supposed that the observed ionospheric disturbances might be produced by propagation of delayed magnetoacoustic wave, which, in turn, was produced by the blast wave. 相似文献
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基于低电离层自洽加热模型,综合考虑了低电离层中电子的复合效应及典型吸附效应,本文数值仿真了大功率高频无线电波持续加热低电离层所产生的电子温度、电子密度的扰动,并且首次模拟分析了由于电子温度扰动造成的加热电波自吸收效应.结果表明：电子吸收大功率加热电波能量导致了电子温度的增加,同时改变了电离层的吸收指数,引起了加热电波的自吸收效应.加热电波的自吸收效应对低电离层较高区域的电子温度扰动有重要的抑制作用.因此,随着加热频率的减小或有效辐射功率的增大,低电离层较低区域的电子温度增量明显增大而在高度100 km以上区域的电子温度增量始终较小.另一方面,随着电子温度的增加,电子的复合系数减小而电子的吸附系数增加,导致了电子密度在低电离层中较高区域出现正扰动而在较低区域出现负扰动.当饱和电子温度较大时,继续减小加热频率或增大有效辐射功率对电子密度扰动所造成的改变较小,尤其当电子温度超出复合系数和吸附系数的温度敏感区间.此外,电子温度与电子密度的饱和时间相差较大,电子温度的饱和时间为微秒量级而电子密度的饱和时间为秒量级. 相似文献
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Based on data from ground-based vertical sounding stations, the behaviors of the ionosphere F region before a strong M 6.8 earthquake off the coast of Hokkaido, Japan, and during the moderate magnetic storm before this earthquake are compared. It was found that the critical frequency of the ionosphere F region (foF2) above the Wakkanai ground-based ionosphere vertical sounding station, which was located in the preparation zone of this earthquake, suffered a long-term disturbance of slightly more than an hour nearly half a day before the earthquake. The magnitude of earthquake-induced disturbance is comparable to that caused by a magnetic storm. 相似文献
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L. F. Chernogor 《Geomagnetism and Aeronomy》2013,53(1):19-31
Aperiodic and quasi-periodic variations in the critical frequency of the F2 layer and Doppler frequency shift of radiowaves at vertical paths on the day of a partial (the magnitude was ～0.78) solar eclipse and on background days are analyzed. According to the experiment, the relative decrease in the electron concentration was 0.41 (0.46 according to calculations) and 0.50 (0.53 according to calculations) in the E region and in the lower part of the F region of the ionosphere. At a height of the main maximum of the electron concentration, the relative decrease in the electron concentration was 0.52 (0.51 according to calculations). It is shown that on the day of the eclipse and on the background day, the characteristics of wave disturbances within the height range 160–240 km were substantially different. Changes in the spectral composition began 30 min after the eclipse occurrence and, depending on the period, lasted from 2 to 4 h. The calculation results of the main parameters of the medium and signal correspond to the observational results. 相似文献