雷达散射截面积的计算研究

 采用矢通量分裂法在网格加密后对电磁散射场和雷达散射截面积RCS进行了检验.根据矢通量分裂法将特征值分解为正负两部分,每一部分抑制了各自的误差.目前计算RCS大都采用频域方法,运用时域方法在实际网格下进行差分运算还较少见.计算结果与网格加密前的情况基本一致.     

弹翼角反射器效应的雷达散射截面分析

分析了弹翼与一般直两面角的角反射器效应的不同,从等效截面法分析一般直两面角角反射器效应的雷达散射截面(RCS),推导出用等效截面法分析弹翼角反射器效应的工程计算公式,通过计算弹翼、弹体组合的侧向散射特性进行了验证;引入涂敷吸波材料的平板RCS的反射系数计算方法,采用两个反射系数表示角反射器效应的两次吸收/反射效应,最后用反射系数法分析了涂敷吸波材料后的弹翼散射特性.     

雷达散射截面对飞机生存力的影响

飞机的雷达散射截面(RCS)是影响飞机生存力的重要因素之一.建立了飞机对由预警雷达、截击机和地空导弹组成的现代化空防系统的生存概率的计算方法.其中包括发现概率、击中概率和击毁概率的计算.在计算发现概率时,考虑了天线方向图传播因子和大气损耗的影响;在计算击中概率时,考虑了信噪比对脱靶距离的影响.通过计算,分析飞机的RCS对生存力的影响.研究结果表明,减缩飞机的RCS不仅可以显著降低飞机被探测的概率,而且还可以缩短截击机和地空导弹对飞机的最远拦截距离.为提高飞机的生存力必须降低飞机的RCS.     

有涂覆层的导体圆柱空间散射特性的数值计算

文中根据带有涂覆层的导体圆柱在平面波的照射下的散射场表达式,进行了全面的数值计算,说明了虚宗量的Bessel函数和Hankel函数的计算方法,分别给出了平行极化波和垂直极化波入射时双站RCS的计算曲线,包括不同涂覆层厚度的影响、入射波频率、涂覆层介质的相对介电常数、导磁率变化时双站RCS的变化规律,获得了有参考意义的结果.     

星载 ScanSAR 特性研究

论述了星载波束扫描合成孔径雷达（ＳｃａｎＳＡＲ）的扫描覆盖特性,指出在满足观测带远端模糊性约束条件下,最大观测带宽度与雷达波长和实际天线孔径的形状无关;阐述了观测带宽度与雷达分辨率、天线面积、发射功率和回波数据率等参数之间的约束关系;给出了数值计算例子。     

隐身卫星的现状及其在空间攻防中的应用

空间攻防是空间技术的一个主要研究内容。隐身卫星正以独特的优势在空间对抗领域中发挥重要作用。首先论述了卫星隐身的主要手段,其次分析了国内外隐身卫星的发展现状,最后详细介绍了隐身卫星在未来空间攻防中的应用前景。     

Detection of regolith buried water stream channels on Mars with the help of synthetic aperture radar

A major theme in the study of Mars is the search for evidence that water was present in the past or is present today, either at or below the surface. Biological life is connected to water. Hence much research is focused on the detection of water stream channels, which in the past flowed on Mars. In these areas, the petrified remains of the former life on Mars may be found. These channels may be under the regolith layer; however, the radio wave penetrating ability allows for the detection of these channels under the regolith.     

NOVEL RADAR SIGNAL SORTING METHOD BASED ON GEOMETRIC COVERING

With the increase of complexity of electromagnetic environment and continuous appearance of advanced system radars, signals received by radar reconnaissance receivers become even more intensive and complex. There- fore, traditional radar sorting methods based on neural network algorithms and support vector machine （SVM） cannot process them effectively. Aiming at solving this problem, a novel radar signal sorting method based on the cloud model theory and the geometric covering algorithm is proposed. By applying the geometric covering algo- rithm to divide input signals into different covering domains based on their distribution characteristics, the method can overcome a typical problem that it is easy for traditional sorting algorithms to fall into the local extrema due to the use of complex nonlinear equation to describe input signals. The method uses the cloud model to describe the membership degree between signals to be sorted and their covering domains, thus it avoids the disadvantage that traditional sorting methods based on hard clustering cannot deinterleave the signal samples with overlapped param- eters. Experimental results show that the presented method can effectively sort advanced system radar signals with overlapped parameters in complex electromagnetic environment.     

An overview of radar soundings of the martian ionosphere from the Mars Express spacecraft

The Mars Express spacecraft carries a low-frequency radar called MARSIS (Mars Advanced Radar for Subsurface and Ionosphere Sounding) that is designed to study the subsurface and ionosphere of Mars. In this paper, we give an overview of the ionospheric sounding results after approximately one year of operation in orbit around Mars. Several types of ionospheric echoes are commonly observed. These include vertical echoes caused by specular reflection from the horizontally stratified ionosphere; echoes from a second layer in the topside ionosphere, possibly associated with O⁺ ions; oblique echoes from upward bulges in the ionosphere; and a variety of other echoes that are poorly understood. The vertical echoes provide electron density profiles that are in reasonable agreement with the Chapman photo-equilibrium model of planetary ionospheres. On the dayside of Mars the maximum electron density is approximately 2 × 10⁵ cm⁻³. On the nightside the echoes are often very diffuse and highly irregular, with maximum electron densities less than 10⁴ cm⁻³. Surface reflections are sometimes observed in the same frequency range as the diffuse echoes, suggesting that small isolated holes exist in the nightside ionosphere, possibly similar to those that occur on the nightside of Venus. The oblique echoes arise from upward bulges in the ionosphere in regions where the crustal magnetic field of Mars is strong and nearly vertical. The bulges tend to be elongated in the horizontal direction and located in regions between oppositely directed arch-like structures in the crustal magnetic field. The nearly vertical magnetic field lines in the region between the arches are thought to connect into the solar wind, thereby allowing solar wind electrons to heat the lower levels of the ionosphere, with an attendant increase in the scale height and electron density.     

半主动雷达寻的空空导弹作战技术运用研究

导弹的攻击区是衡量导弹的攻击能力的最重要的指标之一。通过仿真计算得出不同情况下半主动雷达寻的空空导弹的攻击区。具体分析了不同因素对攻击区的影响，以此为依据，讨论了在战术上如何运用该导弹，给出了充分发挥导弹作战能力的有效途径。可为飞行员使用该种导弹进行空空作战提供正确的理论指导和参考。