S波段振荡器的计算机辅助设计

介绍优化设计振荡器的全过程,阐述优化设计振荡器的原理和方法,分别从线性和非线性方面阐述设计和分析的过程。根据优化设计的结果对振荡器进行生产和试验,试验结果较好地符合仿真的结果,满足设计的要求,这也证明微波计算机辅助设计(CAD)对微波电路的设计是非常有用的     

卫星内部三维屏蔽计算模型

研究中构建了一些常用设备的形状模式,用来计算从不同位置、不同方向入射的粒子在设备中运行的径迹长度；另外构建了各种常见形态的卫星整体模式,可以计算不同位置上卫星舱壁和结构件所产生的屏蔽作用。这些模式构成了一个较为完整的模块,可以计算由卫星舱壁和仪器设备相互屏蔽所形成的屏蔽效果。已经利用这一软件计算了某卫星舱内某仪器内部关键元件的屏蔽情况,计算中涉及到了复杂的卫星舱壁、分布在不同位置的其他仪器、仪器盒、仪器内部的线路板等,取得了较好的效果。     

挠性空间结构变形的自适应辨识

本文以空间控制中的挠性结构变形的辨识为背景,以李雅普诺夫稳定性理论为基础,从辨识的一致性原则出发,给出时变参数的自适应辨识算法。该算法具有梯度型递推形式,结构简单、容易实现。计算机模拟结果表明该算法是解决时变参数辨识的一种有效方法。     

Infrared radiation from compact X-ray sources

Observations of the X-ray binaries 4U 0115+634 and A 0535+262 performed in 1981 – 1982 revealed significant IR variabilities of these sources. 4U 0115+634 was observed twice, in the state close to X-ray activity, and in the state of low activity, thus changing from K = 7^m.75 to K > 9^m. A 0535+262 shows the temporal variations ranged from tens minutes to some days. The regular variations of IR brightness are suspected with teh period close to 104 s that corresponds to the period of axial rotation of neutron star in A 0535+262. The results obtained present arguments in favour of hypothesis that IR radiation is generated near the accreting neutron star and is possibly of maser nature.     

红外气体分析中环境影响的补偿方法研究

环境温度、总压影响是红外气体分析中难以有效解决的主要问题之一，本文以二氧化碳气体为测量对象，采用实验手段，单片机和数据自理技术建立了环境温度、总压对红上气体分析影响的补偿数学模型和求解方法，并进行了实验验证，研究的内容为红外气体分析中影响影响的外补偿开始辟了一条新的途径，具有广阔的应用前景。     

科学视算──新的计算系统

一种新型的数学仿真系统一科学视算系统的特点、需要解决的问题、系统模型以及系统的构成在文中作了介绍和分析。     

平流层飞艇的能源技术和平衡分析

平流层飞艇作为近空间对地观测平台的一种实现方案，主要依靠自身庞大体积产生的静浮力而不像其它飞行器依靠相对空气运动产生升力，所以飞艇能够以较慢的速度飞行甚至能够在空中长期保持定点悬停即相对地面静止。具有长时间在平流层自主飞行的能力，是平流层飞艇设计的一个重要目标。文章对平流层飞艇能源系统的构成、部件及能源平衡分析方法作了介绍。     

红外地平仪姿态测量误差模型

分析得出地球扁率和红外辐射是扫描式红外地平仪测量误差的主要原因。针对地球扁率，基于方位角的确定，分别给出了滚动角和俯仰角的测量误差模型。在地球红外辐射方面，给出了确定地平仪扫人、扫出点位置的方法，进而给出地球红外辐射误差的计算方法。最后，通过算例，给出了有关仿真结果，对方法的有效性进行了验证。     

Spectral properties of backscattered solar Ly-α radiation in the heliosphere: A search for heliospheric boundary effects

We explore the imprints of the solar wind interaction with the local interstellar medium on spectral properties of backscattered solar Ly-α radiation. We employ a newly developed effective model for the interstellar H atom velocity distribution function in the heliosphere ( Katushkina and Izmodenov, 2011). The model takes into account both global effects of H atom perturbations at the heliospheric boundaries and local (i.e. within 10–20 AU from the Sun) effects of the solar ionization, charge exchange, solar gravitation and radiation pressure.     

Surface shape control of integrated paraboloid space reflector consisting of sub-reflectors exploiting modulated solar pressure

Reflectors are very critical space elements and can be used not only as solar collectors/reflectors, telecommunication radio antennas and telescopes but also for dual-usage such as solar sails and solar concentrators to probe and sublimate materials from asteroids when actively controlling the surface shape. In this paper, the surface shape of a slack reflector with negligible elastic deformations will be controlled to be a paraboloid by actively modulating the solar radiation pressure (SRP) force using reflectivity control devices (RCDs) across the reflector. Nonlinear static equilibrium equations for an arbitrary infinitesimal within the reflector along the radial, circumferential and transverse directions are established considering the external modulated SRP force and internal tensions respectively. The coupled radial stress differential governing equation and reflectivity algebraic equation are obtained for the paraboloid reflector by the help of the formulation of an inverse problem based on equilibrium equations previously established. Some analytical and numerical analysis for reflectors with ideal and non-perfect SRP force models are performed respectively. The conclusions concerning about how to control the reflector’s surface shape successfully using allowed reflectivity, resulting in reasonable stress range, moreover, how to get the feasible solutions influenced by the reflector’s size parameters, are all based on the presented analytical and numerical analysis.