Polar format algorithm for bistatic SAR

Matched filtering (MF) of phase history data is a mathematically ideal but computationally expensive approach to bistatic synthetic aperture radar (SAR) image formation. Fast backprojection algorithms (BPAs) for image formation have recently been shown to give improved O(N/sup 2/ log/sub 2/N) performance. An O(N/sup 2/ log/sub 2/N) bistatic polar format algorithm (PFA) based on a bistatic far-field assumption is derived. This algorithm is a generalization of the popular PFA for monostatic SAR image formation and is highly amenable to implementation with existing monostatic image formation processors. Limits on the size of an imaged scene, analogous to those in monostatic systems, are derived for the bistatic PFA.     

UVCS/SOHO Observations of Spectral Line Profiles in Polar Coronal Holes

Ultraviolet emission line profiles have been measured on 15-29 September 1997 for H I 1216 Å, O VI 1032, 1037 Å and Mg X 625 Å in a polar coronal hole, at heliographic heights ? (in solar radii) between 1.34 and 2.0. Observations of H I 1216 Å and the O VI doublet from January 1997 for ? = 1.5 to 3.0 are provided for comparison. Mg X 625 Å is observed to have a narrow component at ? = 1.34 which accounts for only a small fraction of the observed spectral radiance, and a broad component that exists at all observed heights. The widths of O VI broad components are only slightly larger than those for H I at ? = 1.34, but are significantly larger at ? = 1.5 and much larger for ? > 1.75. In contrast, the Mg X values are less than those of H I up to 1.75 and then increase rapidly up to at least ? = 2.0, but never reach the values of O VI.     

ARALL层压板结构疲劳性能分析

目前在航空领域发展非常迅速的ARALL层压板结构和芳纶预浸料的制造工艺,预浸料在具有高的抗疲劳特性和拉伸特性的ARALL层压板结构中起到非常重要的承力和抗疲劳作用。本结构所采用的制造方法是纤维拉伸法,是一种能使ARALL结构的铝板层具有残余压应力,使纤维层具有残余拉应力的方法,从而改善了材料本体的抗疲劳性能。     

变几何喉道对超燃冲压发动机点火与燃烧性能的影响

1引言超燃冲压发动机能高速飞行且能利用空气中的氧气作氧化剂,增加了有效载荷,因而备受重视,但它需要在较高的飞行马赫数下才能工作,因此受到较大的限制。由于双模态超燃冲压发动机可以将工作飞行马赫数下限降低至Ma=3,发动机在飞行马赫数Ma=3~6时以亚燃冲压模态工作,在马赫数     

教师在大学生学风养成方面的影响与作用

面对当前高等教育从“精英教育”走向“大众教育”，高校面临许多新的现象和问题。学风问题是每一时期，每一层次的教育都存在的问题，针对当前高职高专学生的学风养成中教师所应发挥的作用，进行了调研和分析，以期对形成良好的学风有所裨益。     

2001 Mars Odyssey Mission Summary

The 2001 Mars Odyssey spacecraft, now in orbit at Mars, will observe the Martian surface at infrared and visible wavelengths to determine surface mineralogy and morphology, acquire global gamma ray and neutron observations for a full Martian year, and study the Mars radiation environment from orbit. The science objectives of this mission are to: (1) globally map the elemental composition of the surface, (2) determine the abundance of hydrogen in the shallow subsurface, (3) acquire high spatial and spectral resolution images of the surface mineralogy, (4) provide information on the morphology of the surface, and (5) characterize the Martian near-space radiation environment as related to radiation-induced risk to human explorers. To accomplish these objectives, the 2001 Mars Odyssey science payload includes a Gamma Ray Spectrometer (GRS), a multi-spectral Thermal Emission Imaging System (THEMIS), and a radiation detector, the Martian Radiation Environment Experiment (MARIE). THEMIS and MARIE are mounted on the spacecraft with THEMIS pointed at nadir. GRS is a suite of three instruments: a Gamma Subsystem (GSS), a Neutron Spectrometer (NS) and a High-Energy Neutron Detector (HEND). The HEND and NS instruments are mounted on the spacecraft body while the GSS is on a 6-m boom. Some science data were collected during the cruise and aerobraking phases of the mission before the prime mission started. THEMIS acquired infrared and visible images of the Earth-Moon system and of the southern hemisphere of Mars. MARIE monitored the radiation environment during cruise. The GRS collected calibration data during cruise and aerobraking. Early GRS observations in Mars orbit indicated a hydrogen-rich layer in the upper meter of the subsurface in the Southern Hemisphere. Also, atmospheric densities, scale heights, temperatures, and pressures were observed by spacecraft accelerometers during aerobraking as the spacecraft skimmed the upper portions of the Martian atmosphere. This provided the first in-situ evidence of winter polar warming in the Mars upper atmosphere. The prime mission for 2001 Mars Odyssey began in February 2002 and will continue until August 2004. During this prime mission, the 2001 Mars Odyssey spacecraft will also provide radio relays for the National Aeronautics and Space Administration (NASA) and European landers in early 2004. Science data from 2001 Mars Odyssey instruments will be provided to the science community via NASA’s Planetary Data System (PDS). The first PDS release of Odyssey data was in October 2002; subsequent releases occur every 3 months.     

37kW底盘测功机计算机控制系统

底盘测功机是检验汽车、摩托车输出功率及其相关参数的一种检测设备。本课题利用现代先进的计算机控制技术实现对37kW-CHDY底盘测功机的行驶阻力控制、测试数据自动采集,从而实现摩托车道路工况模拟运转以及整车动力性、燃料经济性等指标的测量。     

混合气体流动的一种数值模拟方法

本文建立一个数值模拟完全气体混合流动的理论模型.该模型首先应用混合气体的Euler方程和每种气体组分的质量分数方程来控制流动.为了消除混合网格内气体组分界面附近出现的非物理振荡,我们假定混合气体的每种组分达到了动力学平衡状态然而尚未达到热力学平衡状态.这种思想导致需要另外给定每种气体组分的总能量方程.为使用高分辨格式来求解这组双曲型偏微分方程并且简化对所需要的Jacobi矩阵的推导,混合气体的压力方程也被耦合起来.Godunov型的波传播方法被采用来离散求解所获得的控制方程.从典型算例结果来看,一维问题的数值解与精确解一致,二维问题的数值解与理论分析一致.这说明本文的理论模型是合理的.     

结构参数对圆转矩形喷管换热的影响

为了解结构参数对圆转矩形内喷管再生冷却换热的影响，设计了多个圆转矩形喷管，考虑了三种结构参数：转方位置、出口高宽比和出口圆角大小的影响。采用有限体积法求解三维可压缩的N-S方程对其内部流动和换热进行了数值模拟。湍流模型采用标准的k-ε双方程模型，壁面附近的流动和传热采用壁面函数法处理，速度与压力的耦合采用SIMPLE算法求解。结果表明：在型面一阶导数连续的情况下，转方位置对圆转矩形内喷管的换热影响不大；出口高宽比对圆转矩形内喷管的换热影响较大，出口高宽比不能太小，否则影响内喷管流场和换热；出口圆角大小影响内喷管周向上的温度分布，圆角太小造成周向温度分布不均匀。