低空目标电波折射修正中地球半径计算方法

在防御体系中雷达对低空目标一般呈俯视状况,因此在电波折射修正中必须把地球视为椭球,而不能视为圆球体,否则会产生很大误差.本文通过雷达测量参数和大地坐标与空间坐标的转换,给出了计算雷达电波射线上任意一点对应地球半径的方法.     

准互易光学电压传感器的电场计算与误差分析

针对一种新型的具有准互易反射式光路结构的光学电压传感器,设计了基于锗酸铋(BGO,Bi₄Ge₃O₁₂)晶体横向调制方式的高压探头.采用ANSYS有限元分析软件对所设计的高压探头进行电场计算,得到了探头内的电场及电势分布;讨论了探头内电场分布不均匀及干扰电场导致的测量误差.计算结果表明:标准条件下探头的最高可测电压不低于15 kV;电场分布不均匀导致光沿着晶体内不同路径传输时,电场强度对路径的积分结果即测量电压不同,影响传感器的稳定性和测量精度;探头内干扰电场导致0~5 kV范围内最大测量误差达1.2‰,这一测量误差对于2‰精度的电压传感器是不可忽略的.      

基于三维光场的静态场景前景分割

为解决复杂场景中的前景提取问题提出一种基于三维光场分析的静态场景前景分割方法.首先,通过在一条直线等间距的不同视点上拍摄场景的序列图像构建密集采样的三维光场.其次,用线段检测(LSD)直线检测算法从对极平面图(EPI)中分析提取出场景边缘及其深度信息.借助分段三次Hermite多项式(PCHIP)快速插值算法恢复整个场景的深度信息.最终,通过阈值法实现对不同深度的前景物体的分割.初步实验结果表明,本方法能够较准确地恢复场景中多个物体之间的空间关系,前景分割结果较好地克服了现有基于区域聚类和数学形态学等方法在复杂场景应用中存在的过分割问题.      

基于IRS-P6的岷江上游裸地变化特征研究

以汶川地震干扰作用下岷江上游裸地变化特征为依据,选取岷江上游地形资料及2006年和2009年两个时期IRS-P6多光谱影像数据,通过对岷江上游地区裸地特征地类进行特征分析,在监督分类和聚类分析模块下提取出该区域裸地与非裸地范围,定量界定出岷江上游流域地震前后裸地变化范围。结果表明:岷江上游震前(2006年)裸地面积为2 196km2,震后(2009年)裸地面积为3 680km2,扩大了1 484km2;裸地分布高程从2 200m升高至2 800m,其面积增加较多区域主要集中在汶川县至茂县交界地带、理县的杂谷脑流域一带及黑水县部分区域,该区域亦是人口密度相对集中、地质灾害频发、生态环境相对薄弱的区域。该方法的实现为利用IRS-P6界定生境系统特征提供参考价值,也为环境脆弱性区综合评价分析提供技术支撑。     

Effects of various dissipation range onset models on the 26-day variations of low-energy galactic cosmic-ray electrons

The effect of various models presented by Leamon et al. (2000) for the dissipation range cutoff wavenumber on the 26-day variations of galactic cosmic-ray electrons in a Fisk-Parker hybrid field is investigated, by means of a three-dimensional steady-state numerical modulation code. Analytical expressions for the mean free paths parallel and perpendicular to the heliospheric magnetic field are adapted from the works of 31 and 28, respectively. Note that only solar minimum conditions are considered, and that only qualitative agreement with data is sought. Effective diffusion for galactic electrons pertaining to 26-day variations is found to be dominated by the ratio of the perpendicular to parallel mean free paths at low energies, and the relationship between changes in cosmic-ray intensities and the modulation parameter postulated by Zhang (1997) is found to no longer hold when this ratio drops below a critical value. Use of ion inertial scale dependent models for the dissipation range cutoff leads to possible second linearities in the relative amplitudes as functions of latitude gradient.     

On high-altitude electric fields in the auroral downward current region and their coupling to ionospheric electric fields

The downward field-aligned current region plays an active role in magnetosphere–ionosphere coupling processes associated with aurora. A quasi-static electric field structure with a downward parallel electric field forms at altitudes between 800 km and 5000 km, accelerating ionospheric electrons upward, away from the auroral ionosphere. Other phenomena including energetic ion conics, electron solitary waves, low-frequency wave activity, and plasma density cavities occur in this region, which also acts as a source region for VLF saucers. Results are presented from high-altitude Cluster observations with particular emphasis on the characteristics and dynamics of quasi-static electric field structures. These, extending up to altitudes of at least 4–5 Earth radii, appear commonly as monopolar or bipolar electric fields. The former occur at sharp boundaries, such as the polar cap boundary whereas the bipolar fields occur at softer boundaries within the plasma sheet. The temporal evolution of quasi-static electric field structures, as captured by the pearls-on-a-string configuration of the Cluster spacecraft, indicates that the formation of electric field structures and of ionospheric plasma density cavities are closely coupled processes. A related feature of the downward current is a broadening of the current sheet with time, possibly related to the depletion process. Preliminary studies of the coupling of electric fields in the downward current region, show that small-scale structures are typically decoupled from the ionosphere, similar to what has been found for the upward current region. However, exceptions are also found where small-scale electric fields couple perfectly between the ionosphere and Cluster altitudes. Recent FAST results indicate that the degree of coupling differs between sheet-like and curved structures, and that it is typically partial. The electric field coupling further depends on the current–voltage relationship, which is highly non-linear in the downward current region, and still unrevealed, as to its specific form.     

母弹飞行稳定性及尾部流场分析

为了得到航弹母弹飞行稳定性及尾部流场特性,通过模拟试验和数值计算进行了研究.试验和模拟结果均表明该母弹飞行稳定,且两结果吻合较好.另外,采用数值计算对尾部流场进行了分析,得到了尾部压力分布特性,表明弹尾部存在涡流区,该区范围和流速随弹飞行速度的增加而增大.      

再入航天器陶瓷拐角环防热计算与结构适用性分析

文章基于近地轨道及探月返回再入热环境,应用超高温陶瓷到再入航天器的典型防热结构,计算分析了再入过程中的防热结构温度场。利用温度场计算结果,再结合超高温陶瓷抗烧蚀性能以及结构设计与工艺性分析,就超高温陶瓷作为再入航天器防热结构的适用性进行了深入探讨。结果表明,由于超高温陶瓷的优良耐高温及耐烧蚀性能,在近地轨道及探月返回再入航天器防热结构上具有良好的应用前景。     

火星空间磁场结构特征

在火星空间模拟的单流体MHD模型的基础上, 研究了火星空间磁场结构及火星表面局部磁异常对磁场结构的影响. 在太阳风与火星相互作用的过程中, 形成弓激波和磁堆积区, 行星际磁场弯曲并向两极移动且被拖拽变形, 大部分磁力线从火星两极绕过, 通过火星之后在磁尾留下V字形结构. 火星表面附近局部磁异常也对火星磁场结构产生不可忽视的影响. 不同位置和强度的磁异常与太阳风相互作用形成结构及形态各异的微磁层, 如被拖拽的微磁层和存在开磁力线的微磁层等. 局部磁异常改变了近火磁场结构, 并可能改变等离子体的分布.