An analysis of low-frequency component in microacceleration measurements made onboard the <Emphasis Type="Italic">Foton M-2</Emphasis> satellite

The low-frequency component is investigated in the data of measurements performed onboard the Foton M-2 satellite with the three-component accelerometer TAS-3. Investigations consisted in comparison of this component with its calculated analog found from a reconstruction of the satellite’s attitude motion. The influence of the Earth’s magnetic field on the accelerometer readings is discovered by way of spectral analysis of the functions representing the results of determining the low-frequency microacceleration by two methods. After making correction for this influence, the results obtained by these two methods coincided within a root-mean-square error of less than 10^?6 m/s².     

Calculation of quasisynchronous orbits of a spacecraft around Phobos for solving the problem of landing on its surface

The problem of selecting quasi-synchronous orbits of a spacecraft around Phobos is considered. These quasi-synchronous orbits are far (with respect to the Hill’s sphere) quasi-satellite orbits with retrograde rotation in the restricted three body problem. The orbit should pass through a given point at a specified time instant. It should also possess a property of minimum distance from the Phobos surface at every passage above the region of planned landing. The equations of dynamics are represented in the form describing the orbit as a combination of motions in two drifting ellipses, inner and outer ellipses. The center of the outer ellipse is located on the inner ellipse. A formula is derived that relates averaged values of half-axes of the inner and outer ellipses. It is used for construction of the first approximation of numerically designed orbit, which makes it possible to simplify and speed up the computing process. The tables of initial conditions obtained as a result of calculations are presented.     

Proton fluxes measured by low-orbit satellites

In this paper we consider the fluxes of protons in the energy range from 30 keV to 140 MeV recorded by instruments onboard the Russian satellites KORONAS-F and UNIVERSITETSKII and on the American satellites GOES-11 and NOAA-17. In order to estimate the reliability of the obtained data, the comparison of measurements of separate energy channels of these instruments between themselves is performed. Experimental fluxes of trapped protons are compared with the fluxes predicted by the AP8 model.     

Turbulent fluctuations of plasma and magnetic field parameters in the magnetosheath and the low-latitude boundary layer formation: Multisatellite observations on March 2, 1996

The results of simultaneous analysis of plasma and magnetic field characteristics measured on the INTERBALL/Tail Probe, WIND and Geotail satellites on March 2, 1996, are presented. During these observations the INTERBALL/Tail Probe crossed the low-latitude boundary layer, and the WIND and Geotail satellites measured the solar wind’s and magnetosheath’s parameters, respectively. The plasma and magnetic field characteristics in these regions have been compared. The data of the Corall, Electron, and MIF instruments on the INTERBALL/Tail Probe satellite are analyzed. Fluctuations of the magnetic field components and plasma velocity in the solar wind and magnetosheath, measured onboard the WIND and Geotail satellites, are compared. The causes resulting in appearance of plasma jet flows in the low-latitude boundary layer are analyzed. The amplitude of magnetic field fluctuations in the magnetosheath for a studied magnetosphere boundary crossing is shown to exceed the magnetic field value below the magnetopause near the cusp. The possibility of local violation of pressure balance on the magnetopause is discussed, as well as penetration of magnetosheath plasma into the magnetosphere, as a result of magnetic field and plasma flux fluctuations in the magnetosheath.     

航天器研制全过程污染控制工程

污染控制体系的完善,控制技术的成熟,对航天器研制至关重要,本文简要说明了污染控制的重要性,以及由于污染造成航天器失效的例子,比较详细地介绍了航天器项目各阶段污染控制的一些方法,最后简要介绍了污染领域的发展方向和急需解决的问题。     

航天器污染检测新技术的研究

根据飞行时间二次离子质谱学的新进展,用当代最先进的仪器首次对三种典型的我国地面空间环境模拟污染样品进行了探索性实验研究。结果表明：由于极高的检测灵敏度,具备分析微量航天污染物成分的能力;由于很高的质量分辨本领,具备检测航天污染物包含的所有元素、同位素和各种化合物的指纹鉴别能力;成像分析可获得航天污染物各成分面分布及一定的分层信息,从而可望揭示出各类污染物的形成过程。与国内外现有的各类检测手段相比,飞行时间二次离子质谱是航天污染物检测强有力的一种新手段。讨论了需要进一步研究解决的主要问题,如果能开发出可避免二次污染并分阶段取样、保存样品的装置与之配合,该技术有望在迅速崛起的航天污染系统工程中发展成为一种独具特色的航天污染检测新技术。     

混合不确定系统鲁棒稳定性检验的数值方法

混合不确定系统的鲁棒稳定性问题可以转化为一有理函数簇边界的H_∞范数检验问题.为了减小计算复杂性,对一类线性部分仿射取决于变化参数的混合不确定系统,探讨了其数值求解方法.结果表明在固定的频率上边界对象的象是复平面上的一圆弧.对此文中获得了一个新的最大圆弧范数计算公式并诱导出一个可在有限频率范围内进行边界检验的算法.大大减小了计算量.     

双三角翼飞机气动力工程计算研究

 双三角机翼比三角机翼气动布局具有更优越的升阻特性.飞机空气动力的工程计算是用数值方法寻求飞机最优设计方案的基础.采用基于面积比思想的半经验工程算法计算了双三角翼飞机的升力系数曲线斜率、零升阻力系数和诱导阻力因子.结果经风洞试验数据校验,精度完全能满足飞机方案设计要求.算法在某改型飞机方案设计中得到了成功的应用.     

吸气式高超声速机体/推进一体化飞行器数值和试验研究

发展吸气式高超声速技术是实现可持续高超声速飞行(尤其是在大气层以内)的重要途径.吸气式高超声速飞行器为了获得良好的气动-推进性能,必须采用机体/推进一体化设计.笔者发展了针对一体化飞行器的气动力和推进力的划分体系和计算方法,发展了内外流数值计算软件.研究了机体/推进一体化设计的平头形高超声速飞行器在进气道关闭条件下的气动性能,并进行了试验验证;数值研究了进气道打开和发动机工作条件下一体化飞行器的气动-推进性能;研究了机体和推进系统的不同部件对飞行器气动-推进性能的贡献.     

通用加速计算在环幕失真校正中的应用研究

大规模场景的沉浸式投影系统大都以环幕作为显示设备,而由环幕造成的几何失真使系统真实感大大降低。从环幕产生失真的几何原理出发,通过建立投影平面和成像面之间的坐标映射关系,生成了一种几何失真校正的理论模型。同时,研究了一种适于通用加速计算的图形硬件架构CUDA,基于其多线程的硬件执行机制,通过将几何失真的校正矩阵组织成纹理进行多重纹理贴图映射,设计了预失真校正的硬件加速算法,该算法还利用基于权值的超采样技术对加速中的走样进行了设计。最后,对该方法的校正效率和效果进行了实验验证,证明该方法具有更高的场景交互速度和很好的校正效果。