Information extraction from thematic mapper data

The Landsat-4 spacecraft, launched on July 9, 1982, is equipped with a new electro-optical sensor expected to advance the remote sensing capabilities of Earth resources satellites. An experimental instrument, the thematic mapper (TM), provides data in seven discrete energy bands with greatly improved spectral, spatial and radiometric resolution, relative to previous Landsat satellite systems. Scientists at NASA, National Space Technology Laboratories (NSTL), Earth Resources Laboratory (ERL) conducted an evaluation of Landsat-4 TM data, soon after its launch, to examine the potential of this new electro-optical sensor for providing improved information for renewable resources and land cover studies. Investigations of TM data included forested wetland, urban and agricultural land covers using a scene of data collected over Arkansas and Tennessee on August 22, 1982. Standard digital information extraction techniques were employed, and the classification accuracies achieved with a single date TM data set exceeded a 90% correct confidence level. While only spectral analysis techniques were utilized for this initial evaluation, the results clearly indicate the improved performance provided by the experimental TM sensor over previous Earth observing capabilities.     

水声管中传感器灵敏度标定的新方法

对声管双传感器传递函数法测量中由传感器灵敏度差异带来的误差进行了分析.根据已知确定界面反射系数可确定传感器传递函数,并可求其灵敏度比的原理提出了声管中双传感器灵敏度标定的新方法.空气声管中对刚背衬下已知传递函数进行了实验验证;水声管中气体背衬时,分别在常压和打压情况下对新方法进行了实验验证,说明了新方法的可靠性,克服了水声管中无法用交换传感器获得灵敏度补偿的困难.     

绕任意轴旋转的管道流动和换热特性研究

当管道绕任意轴旋转时，管道内的轴向速度分布发生改变，截面上产生二次流动，管道的对流换热特性将引起变化。本文对绕任意轴旋转的管道流动与换热进行了数值模拟，研究结果表明：绕任意轴旋转管道内的对流换热特性主要由Re（雷诺数），Ro(Rossby数），Pr（普朗特数）数，和α（旋转轴与管道轴线的夹角）四个参数决定。文中分析了在不同情况下流场结构与摩擦系数比以及温度场与管道Nu数比率随Re数和Ro数的变化规律，为工程实际应用提供了理论依据。     

刚体转动惯量的测量及数据处理

本文采用一元线性回归法进行刚体转动惯量实验的数据处理,对通常在测量中运用的简化条件作了分析,从而提高了实验课的教学水平,并使该实验具有实用价值。     

充气式月球居住舱蒙皮结构设计及其材料研究进展

综述国外充气式月球居住舱（ILH）蒙皮结构设计及其相关材料研究的进展：对ILH的发展历史、蒙皮结构设计方案及其材料选型等方面进行介绍;重点介绍高分子材料在ILH蒙皮微流星体与空间碎片（MMOD）防护层、热微流星体遮蔽层（TMC）、纤维织物阻挡层、多层绝热毯（MLI）以及气囊结构设计中的应用。最后对我国未来月球居住舱及其关键高分子材料的发展提出建议。     

Shock acceleration of energetic particles in the heliosphere

The theory of shock acceleration of energetic particles is briefly discussed and reviewed with an emphasis on clarifying the apparent distinction between the V × B and Fermi mechanisms. Attention is restricted to those situations in which the energetic particles do not themselves influence the given shock structure. In particular, application of the theory to the acceleration of energetic particles in corotating interaction regions (CIR) in the solar wind is presented. Here particles are accelerated at the forward and reverse shocks which bound the CIR by being compressed between the shock fronts and magnetic irregularities upstream from the shocks, or by being compressed between upstream irregularities and those downstream from the shocks. Particles also suffer adiabatic deceleration in the expanding solar wind, an effect not included in previous shock models for acceleration in CIRs. The model is able to account for the observed exponential spectra at Earth, the observed behavior of the spectra with radial distance, the observed radial gradients in the intensity, and the observed differences in the intensity and spectra at the forward and reverse shocks.Calculations and resulting energy spectra are also presented for shock acceleration of energetic particles in large solar flare events. Based on the simplifying assumption that the shock evolves as a spherically symmetric Sedov blast wave, the calculation yields the time-integrated spectrum of particles initially injected at the shock which eventually escape ahead of the shock into interplanetary space. The spectra are similar to those observed at Earth. Finally further applications are suggested.An invited paper presented at STIP Workshop on Shock Waves in the Solar Corona and Interplanetary Space, 15–19 June, 1980, Smolenice, Czechoslovakia.     

大学生就业报道的内容分析——以《中国青年报》为例

通过《中国青年报》关于大学生就业报道内容的分析,得出其立足点与政府立场和就业政策的高度一致,注重报道和反映大学生自主创业和到基层就业的内容,并在报道中呈现出其报道的服务性、实用性等特点。     

介质涂覆位置对球面收敛喷管电磁散射特性影响

外形设计和隐身材料使用是缩减目标雷达散射截面积(RCS)的两种常用方法。为了研究雷达吸波材料(RAM)对于球面收敛矢量喷管(SCFN)的RCS减缩效果,采用引入阻抗边界条件后的迭代物理光学(IPO)法,研究了球面收敛二元喷管及8种吸波材料涂覆方案的电磁散射特性,并获得了X波段下9种模型的后向RCS随探测角度的变化规律。研究结果表明:吸波材料涂覆可以有效地缩减球面收敛喷管的RCS;合理的涂覆方案可以在保证RCS缩减效果的基础上,降低吸波材料的使用量;相比全涂覆方案,仅在喷管出口和球面段进行涂覆,可以在吸波材料减少30%使用量的情况下,达到全涂覆方案80%的缩减效果。     

FC-AE-1553网络的“并发交换式”动态带宽调度机制

为提高航天航空网络传输性能,针对低轨空间舱内有效载荷系统的特点及有效载荷系统数据传输的要求,将空间有效载荷系统的数据分为周期性业务、突发性业务及强时效性业务3种业务类型,并综合分析3种业务特征,提出了一种可应用于FC-AE-1553网络的“并发交换式”动态带宽调度（DBA）机制,即突发性业务传输采用“并发交换式”的动态带宽分配,周期性业务采用静态固定带宽分配,强时效性业务采用抢占式带宽分配的方案。采用理论分析和仿真验证的方式分析了该调度机制的可行性,并通过OPNET仿真软件建立了FC-AE-1553网络仿真平台。结果表明,相比FC-AE-1553网络传统的“总线式”调度机制,所提机制可将FC-AE-1553网络的吞吐量提高10倍以上,且当网络节点数为32时,FC-AE-1553网络的吞吐量可从2.8 Gb/s提高到46 Gb/s,突发性业务的平均时延可降低1个数量级。      

Shock acceleration of energetic particles in corotating interaction regions

A simple shock model for the acceleration of energetic particles in corotating interaction regions (CIR) in the solar wind is presented. Particles are accelerated at the forward and reverse shocks which bound the CIR by being compressed between the shock fronts and magnetic irregularities upstream from the shocks, or by being compressed between upstream irregularities and those downstream from the shocks. Particles also suffer adiabatic deceleration in the expanding solar wind, an effect not included in previous shock models for acceleration in CIR's. The model is able to account for the observed exponential spectra at earth, the observed behavior of the spectra with radial distance, the observed radial gradients in the intensity, and the observed differences in the intensity and spectra at the forward and reverse shocks.