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提出了一种地面数字电视单频网覆盖率预算方法,该方法考虑实际接收机干扰模型,采用k-LNM法进行信号合成,利用CCDF函数计算覆盖小区的地点概率,预算结果更实际,计算量小.单频网本身产生“人工多径”,为最小化自干扰区域,基于遗传算法求解单频网中各个发射机附加延时的最优组合,该方法无需改变发射台功率、站址、天线等参数,成本为0,克服了发射机数目较多时人工调整发射机附加延时的难点,且准确度高.将该方法应用于我国某地区地面数字电视单频网规划的实际场景中,优化后覆盖率明显提高,验证了该方法的有效性和可行性. 相似文献
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O.A. Molchanov O.A. Maltseva E.E. Titova V.I. Di F. Jirˇi´cˇek P. Trˇi´ska 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》1982,2(10):227-229
Signals of VLF transmitters of the Omega navigation system located in the auroral zone (66.4°N, 13.2°E, L= 5) were recorded by the VLF receiving equipment of the Interkosmos 19 satellite. Signals at frequencies between 10.2 and 13.6 kHz were received in a region above the transmitters, frequently with whistler-type echoes. An analysis of these echoes has shown their predominating occurrence in periods of low geomagnetic activity (Kp<2+). The occurrence region of these phenomena in the outer ionosphere has the dimension of about 1000 km and its position is betweenL= 2.5 and L= 4.4. The delay of echo-signals is practically the same during one satellite pass but its values for different satellite revolutions lie between 2.5 and 3.5 s. The frequency spectrum of these signals can be broadened up to 100 Hz. On the basis of calculations made, it can be shown that the experimental results are generally in accordance with the hypothesis of nonlinear ducting of VLF waves in the magnetosphere. 相似文献
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Paul Sava Erik Asphaug 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2018,61(8):2198-2213
Answering fundamental questions about the origin and evolution of small planetary bodies hinges on our ability to image their surface and interior structure in detail and at high resolution. The interior structure is not easily accessible without systematic imaging using, e.g., radar transmission and reflection data from multiple viewpoints, as in medical tomography. Radar tomography can be performed using methodology adapted from terrestrial exploration seismology. Our feasibility study primarily focuses on full wavefield methods that facilitate high quality imaging of small body interiors. We consider the case of a monostatic system (co-located transmitters and receivers) operated in various frequency bands between 5 and 15?MHz, from a spacecraft in slow polar orbit around a spinning comet nucleus. Using realistic numerical experiments, we demonstrate that wavefield techniques can generate high resolution tomograms of comets nuclei with arbitrary shape and complex interior properties. 相似文献
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S.R. Tojiev B.J. Ahmedov H.E. Eshkuvatov 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2014
Tashkent International Heliophysical Year (IHY) station is a member of Atmospheric Weather Electromagnetic System for Observation, Modeling and Education (AWESOME) network being operated globally to study the ionosphere and the magnetosphere with the help of electromagnetic waves in Very Low Frequency (VLF) band. Regular monitoring of the D- and F-layers of ionosphere over Central Asia territory is being performed on the permanent basis starting year 2008. We have studied VLF amplitude anomalies related to the EQs occurred in 2008–2009 years with magnitude more than 5 on the path way from the VLF transmitters to the Tashkent station assuming that propagation of VLF ground-based transmitters signals can be perturbed by EQ preparation detectable from the ground-based measurements in the VLF bands. For analyzing narrowband data we have used the nighttime fluctuation (NF) method paying attention to the data obtained during the local nighttime (20:00 LT–04:00 LT) in Tashkent where the VLF receiver is operating. The mean nighttime amplitude (or trend) and nighttime fluctuation are found to increase significantly before the EQ occurred on the path way from the transmitters to the receiver. The obtained results have revealed an agreement with VLF amplitude anomalies observed in Tashkent VLF station during the strong EQs occurred on the path way from the transmitters to the receiver. Some results are presented to show the probing potentiality of VLF waves to predict short term EQs with high magnitude. 相似文献
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V.V. Paznukhov V.G. Galushko B.W. Reinisch 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2012
A technique for studying ionospheric wavelike phenomena, primarily AGW/TID events, is developed based on the solution of the problem of radio wave propagation in ionospheric plasma disturbed by wavelike processes. A perfectly reflecting surface model is used for representing TIDs propagating at ionospheric heights. This technique is a generalization of the Frequency-and-Angular Sounding (FAS) method developed earlier for oblique TID diagnostics using transmitters of opportunity. Trial measurements were made in November 2003 with two DPS-4 systems at Millstone Hill Observatory, providing experimental validation of the developed method by comparing the results of disturbance diagnostics to those simultaneously obtained with the original (oblique) FAS method. The TID parameters recovered during the November 2003 campaign suggest that the observed disturbances predominately propagated equatorward which likely indicates their sources to be in the auroral region. The equatorward propagating AGW/TIDs are typical for disturbed geomagnetic conditions which were observed during the campaign. Implementation of the generalized FAS technique in the DPS sounder allowed development of a dedicated data acquisition system for ionospheric disturbance diagnostics. Routine measurements with the developed technique using the existing world-wide network of Digisondes (GIRO) will make it possible to conduct large-scale studies of the AGW/TID phenomena. 相似文献
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本文阐述了用同轴双六端口自动网络分析仪测量非互易二端口器件的原理,以及所用的计算机软件数学模型。出了100~1000MHz频段内测量铁氧体隔离器参数的实验结果。 相似文献
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借鉴复合材料结构建模中的均匀化处理方法建立了压电网络板机电耦合动力学方程并对其进行求解,获得了耦合系统的频率特征方程;通过求解频率特征方程发现压电网络板的固有模态以耦合模态对的形式存在;在此基础上对耦合系统的频率特性进行了分析,表明耦合模态对的特征频率值随着电感的变化会出现频率转向现象.进一步通过对系统在频率转向区能量转换规律的研究,揭示了压电网络板中频率转向的意义.最后,分析了压电网络板设计参数对频率转向区特性的影响,为压电网络板的合理设计提供了理论参考. 相似文献
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HP85016A/B系统软件适用于在射频─—微波频段中使用HP8757C/HP8350B标量网络分析仪测试无源网络(部件)的传输/反射。讨论了确定在遥测系统广为使用的有源网络(部件)的线性区域的方法,提出了利用HP8757C标网本身进行1dB增益压缩的测试,以实现NP85016A/B自动化测试系统延伸到有源网络(部件)测试的设想,程序的实施及勺HP85016A/B完命地接融,从而关键性地扩大了HP85016A/B在遥测分系统测试的使用。 相似文献
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S. Montebugnoli G. Pupillo E. Salerno S. Pluchino M. di Martino 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2010
An accurate measurement of the position and trajectory of the space debris fragments is of primary importance for the characterization of the orbital debris environment. The Medicina Radioastronomical Station is a radio observation facility that is here proposed as receiving part of a ground-based space surveillance system for detecting and tracking space debris at different orbital regions (from Low Earth Orbits up to Geostationary Earth Orbits). The proposed system consists of two bistatic radars formed by the existing Medicina receiving antennas coupled with appropriate transmitters. This paper focuses on the current features and future technical development of the receiving part of the observational setup. Outlines of possible transmitting systems will also be given together with the evaluation of the observation strategies achievable with the proposed facilities. 相似文献
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针对复杂环境下空地数据链正交频分复用(OFDM)系统信道估计精度不足的问题,提出了一种基于调制卷积神经网络(MCNN)和双向长短时记忆网络(BiLSTM)结合的信道估计算法。利用最小二乘算法(LS)提取初始信道状态信息(CSI);利用MCNN网络提取初始CSI的深度特征,并对网络模型进行压缩;利用BiLSTM网络对最终CSI进行预测,实现信道估计。利用构建的空地信道模型生成信道系数数据集,实现神经网络模型的训练与测试。仿真结果表明:与传统算法和现有深度学习方法相比,所提出的信道估计算法具有更小的估计误差,高信噪比条件下的系统误码率(BER)性能提升接近一个数量级;由于引入了调制滤波器技术,随着神经网络层数增加,网络模型参数量大幅减少。 相似文献
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G.J. Sofko J.A. Koehler J. Gilmer A.G. McNamara D.R. McDiarmid 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》1982,2(7):149-152
During August 1981, a 50 MHz c.w. radar system was operated in central Canada to measure auroral scatter amplitudes and Doppler spectra from a scattering region centered near 66° magnetic invariant latitude (L ≈ 6.0). Narrow beams from 3 transmitters, differing in frequency by 1 KHz, were directed to cover a common volume of the ionosphere over a ground location at 56.3°N, 103.5°W. The scattered signals were received on narrow beam antennas at two receiving sites, and recorded in analog form on magnetic tape under the control of an AIM65 microcomputer. The analog tapes were digitized later and FFT-processed to obtain Doppler spectra and amplitudes.The 6 transmission paths were designed to provide several magnetic aspect angles varying by 1.5°-7° from perpendicularity with the earth's field B and two streaming aspect angles differing by ~38°. The objective was to employ controlled geometric factors to study the functional dependency of signal amplitudes and Doppler shifts on magnetic and streaming aspect angles. Several hundred hours of excellent data were obtained in continuous operation during the month of August 1981. Preliminary results will be reported. 相似文献
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