Beagle 2: a proposed exobiology lander for ESA's 2003 Mars Express mission.

The aim of the proposed Beagle 2 small lander for ESA's 2003 Mars Express mission is to search for organic material on and below the surface of Mars and to study the inorganic chemistry and mineralogy of the landing site. The lander will have a total mass of 60kg including entry, descent, and landing system. Experiments will be deployed on the surface using a robotic arm. It will use a mechanical mole and grinder to obtain samples from below the surface, under rocks, and inside rocks. Sample analysis by a mass spectrometer will include isotopic analysis. An optical microscope, an X-ray spectrometer and a Mossbauer spectrometer will conduct in-situ rock studies.     

偏置动量系统中的挠性天线指向控制研究

从工程实践角度,探讨了在目前广泛采用的偏置动量轮三轴姿态稳定卫星上,进行大尺寸（３～５ｍ）和高指向精度（０．０５°）的挠性天性指向控制问题。在建立具有挠性天线的星体动力学模型,以及在借鉴和改进有关抑制挠性天线振动研究的基础上,设计了三轴稳定卫星平台上的挠性天线指向控制系统的方案。最后,根据数值仿真结果,给出了影响挠性天线指向精度的主要因素。     

利用前缘旋转控制边条翼外翼分离

边条翼在边条较小时中等迎角以上外翼就会出现分离,现提出用转动前缘表面来控制边条翼外翼分离。通过测力、油流和烟丝实验研究了转动前缘对机翼气动特性的影响。结果表明,在这种机翼上转动前缘对控制分离是有效的,升力增量最大可达３０％。可以预期,转动前缘与边条的综合作用,机翼的分离特性将有较大的改善     

密闭舱压力控制特性

本文主要报告研制中的密闭舱压力控制系统的建模和特性分析。系统特性分析和计算机仿真结果表明此类系统的稳定性条件是容易满足的。理论分析和计算机仿真结果得到了试验结果的验证,证明该数学模型的正确性和可应用性。它对于今后的研制工作是有指导意义的。     

保证试验对陶瓷试件疲劳强度的影响

 应用断裂力学理论分析了保证试验对陶瓷试件造成的损伤及其对疲劳强度的影响。保证试验后试件的最低强度可根据材料的亚临界裂纹扩展参量、保证应力和保证试验的卸载速率估算。采用惰性试验环境和高的卸载速率可获得较高的试件最低剩余强度值。     

大型固体火箭发动机喷管故障诊断的流场计算

针对某大型固体火箭发动机的喷管喉道后烧穿的故障进行了数值模拟,运用ＴＶＤ（ＴｏｔａｌＶａｒｉａｔｉｏｎＤｉｍｉｎｉｓｈｉｎｇ）ＭａｃＣｏｒｍａｃｋ格式求解了喷管内流场的二维轴对称Ｎ－Ｓ方程,获得了流场的详细结构图谱,分析了故障的成因,指出喷管型面的导数不连续会导致当地壁温升高,是引发故障的直接原因。     

The Solar Isotope Spectrometer for the Advanced Composition Explorer

The Solar Isotope Spectrometer (SIS), one of nine instruments on the Advanced Composition Explorer (ACE), is designed to provide high- resolution measurements of the isotopic composition of energetic nuclei from He to Zn (Z=2 to 30) over the energy range from ∼10 to ∼100 MeV nucl−1. During large solar events SIS will measure the isotopic abundances of solar energetic particles to determine directly the composition of the solar corona and to study particle acceleration processes. During solar quiet times SIS will measure the isotopes of low-energy cosmic rays from the Galaxy and isotopes of the anomalous cosmic-ray component, which originates in the nearby interstellar medium. SIS has two telescopes composed of silicon solid-state detectors that provide measurements of the nuclear charge, mass, and kinetic energy of incident nuclei. Within each telescope, particle trajectories are measured with a pair of two-dimensional silicon-strip detectors instrumented with custom, very large-scale integrated (VLSI) electronics to provide both position and energy-loss measurements. SIS was especially designed to achieve excellent mass resolution under the extreme, high flux conditions encountered in large solar particle events. It provides a geometry factor of ∼40 cm2 sr, significantly greater than earlier solar particle isotope spectrometers. A microprocessor controls the instrument operation, sorts events into prioritized buffers on the basis of their charge, range, angle of incidence, and quality of trajectory determination, and formats data for readout by the spacecraft. This paper describes the design and operation of SIS and the scientific objectives that the instrument will address. This revised version was published online in June 2006 with corrections to the Cover Date.     

箔条云团的后向雷达散射截面积

用矩量法计算了３种箔条云团模型的后向雷达散射截面积。计算结果表明平均间距较大时（大于２λ）互耦对ＲＣＳ影响不大,后向散射截面积的概率分布无论考虑互耦与否都满足指数分布,只是其数学期望有所不同。     

REM measurements aboard Mir during 1995

Measurements of the South Atlantic Anomaly (SAA) made with the Radiation Environment Monitor (REM) aboard Mir from November 1994 to February 1996 are presented. During this period an increase of the SAA radiation by ≈25% is observed, which coincides with a lowering of the radio solar flux. Radio solar flux is one of the parameters controlling the earth's atmospheric distribution and with it the absorption of inner radiation belt protons forming the SAA. Due to the altitude gradient of the atmospheric density, the proton fluxes in the SAA are anisotropic (loss cone, east-west effect). The measured distribution can be accounted for by basic models.     

三点测距副站技术

设计和研制的两个副站（乌鲁木齐站和广州站）和北京的主站相互配合形成三点测距系统,可以完成对风云二号卫星的测距定轨任务。文章着重介绍了副站的组成、作用和功能技术指标等。它的设计方法与国外同类技术相比颇具特色。经过对日本气象卫星进行的几年跟踪测试,及最后通过对风云二号卫星执行任务的验证,确认了副站方案的可行性,设计的合理性。