电磁环境评估中传播模型的对比分析与修正方法研究

根据电磁环境评估的需要,对常用的电波传播模型进行对比分析,通过电磁环境的实例测试,选择适合广州市区的电波传播模型,并提出一种基于线性回归的K参数修正方法。     

可变参数AWGN深空信道模型特性分析及其仿真

文章在研究深空通信信道的统计特性的基础上,建立了可变参数AWGN（VPAWGN）模型来模拟深空通信信道,主要考虑噪声功率、多普勒频移和路径损耗等参数对信道特征的影响。进一步在Visual C＋＋环境下搭建VPWAGN模型,并对各参数对信道的影响进行验证。     

多数传电台信息传输的设计和实现

应用星形结构思想,提出了建立“一对多”数传电台信息传输的技术途径及实现方案,并开发出了具体的应用软件。提出的方法可应用于无通信基础情况下静止或低动态多目标间的信息交换,具有很大的实际应用价值。     

GMRT monitoring of Cyg X-1 and Cyg X-3

We present the results of low frequency radio observations of the X-ray binaries, Cygnus X-1 and Cygnus X-3, during different X-ray states. The low frequency observations were made for the first time for these sources at 0.61 and 1.28 GHz using the Giant Meter-wave Radio Telescope (GMRT) between 2003 and 2004. Both Cyg X-1 and Cyg X-3 are highly variable at low radio frequencies. We also compare our data with the observations at 15 GHz conducted by the Ryle telescope. Spectral turnover is seen for both the sources below 2 GHz. The data suggest that the change in the radio flux density in both the sources is correlated to the X-ray hardness ratio and follows a similar behavior pattern.     

Shumann resonances and electromagnetic transparence in the atmosphere of Titan

Among the multiple questions that the CASSINI/HUYGENS mission tries to answer is the likelihood of electric discharges in Titan's atmosphere. The instruments “Huygens Atmospheric Structure Instrument” and “Radio and Plasma Wave Science” will probe the electromagnetic emissions during the Huygens descent and Cassini flybys, respectively. Although no lightning was observed during Voyager's encounters with Titan in 1980 and 1981, this does not exclude the existence of lightning phenomena. Recent investigations show that lightning discharges could occur in the lower atmosphere, such as the detection of methane condensation clouds in the troposphere and the theoretical prediction of an electric field that would be sufficient enough to cause lightning. We present a numerical model of Titan's atmosphere with the aim of calculating the resonance frequencies and the atmospheric transparency to electromagnetic waves. The detection and measurement of these resonances, Schumann frequencies, by the Huygens probe, would show the existence of electric activity connected with lightning discharges in the atmosphere. As it happens with the Schumann frequencies of Earth, losses associated with the electric conductivity will make these frequencies to be lower than the theoretically predicted, the fundamental one being located between 11 and 15 Hz. An analytical study shows that the strong losses associated with the high conductivity make it impossible that an electromagnetic wave generated near the surface with a frequency of 10 MHz or lower reaches the outer part of Titan's atmosphere. Therefore the detection of electromagnetic waves coming from Titan's lower atmosphere by the RPWS instrument is very unlikely.     

P波段SAR射频干扰信号分析及抑制方法研究

分析了实测P波段SAR静默接收数据,研究了模拟电视信号的频谱特性。针对P波段SAR回波中的模拟电视干扰信号,提出了一种新的干扰抑制方法。通过在时域拼接多个脉冲的回波数据增加模拟电视信号的观测时间以提高频率分辨率,进而在距离频域对其准确识别。根据模拟电视信号的频谱特征,在距离频域构造滤波器组滤除模拟电视信号的离散谱线,保留了谱线间SAR回波信号的频谱分量。实际回波数据的成像处理结果验证了方法的有效性。     

多带通UWB信号光子学产生方法

基于多个不同权重与时延的doublet脉冲叠加,提出一种新的多带通超宽带（ MB-UWB）信号光学产生与传输的方法。射频（ RF）信号对光载波进行强度调制后,电高斯脉冲对光信号进行相位调制并利用标准单模光纤（ SMF）进行传输。 SMF实现相位调制-强度调制（ PM-IM）转换,产生doublet脉冲;实现多个doublet信号的时延差,产生叠加的UWB信号。通过调节RF信号源的频率可以实现UWB信号中心频率和带宽的改变;通过调节RF信号源的幅度可以实现边带抑制比的改变。仿真实现了边带抑制比大于25dB,中心频率5~8GHz,带宽2.9~3.8GHz的UWB的信号产生。     

不规则地形条件下的双向抛物方程模型研究

在传统SSFT抛物方程模型基础上,针对传统算法忽略电波后向传播与散射,造成不规则地表边界条件下电波传播预测误差较大的问题,提出了可计算任意不规则地形剖面下前向和后向传播场的递归双向抛物方程模型,并给出了具体实现步骤,提高精度的同时弥补了传统算法的不足。仿真分析了双向抛物方程模型计算标准大气条件下单刃峰、双刃峰及实际地形的电波传播场分布特性,并与传统宽角抛物方程与几何绕射理论进行比较,验证了算法及模型的正确性与有效性。