地球观测科学的发展以及空间站对地观测

综述了地球观测科学的发展以及空间站对地观测。对载人空间站在对地观测中的优势、类型和应用进行了重点论述。介绍了我国空间站对地观测应用的重要意义。最后，论述了以空间站为核心的天基信息网和遥感技术的快速发展是空间对地观测的主要发展趋势。     

ATC计算机系统的地线系统及机房防火措施

在计算机系统的接地系统中,一些问题至今尚无定论,本文结合几个计算机系统安装调试的经验,及现有的ATC雷达模拟系统实体,就机房屏蔽地线、防雷击地线、交流地线、系统地线给予介绍和简单的论述,并给出一些经验值,还说明了直流地悬空的危害和地桩的埋设方法。另外,简要介绍了机房的防火设施,以便有关单位参考。     

钛合金稀土阳极化成膜过程的电化学研究

 对钛合金稀土阳极氧化的电化学过程进行了研究;重点研究了钛合金稀土阳极氧化的成膜过程;分析了不同硫酸浓度,不同成膜电压条件下,电化学参数的变化,讨论了稀土阳极氧化膜的形成机理;通过对阳极氧化膜的 SEM微观形貌图及其他电化学参数的分析,推断氧化膜为分层结构;在一定温度和电压下,对电极电位的变化进行了研究,探讨了稀土阳极氧化膜的形成过程和导电机制;提出了稀土阳极氧化膜是由具有一定半导体特性和电容性的致密层与多孔层构成的,整个成膜过程中导电是由空穴、铈盐离子和溶液离子共同完成的。     

低空目标电波折射修正中地球半径计算方法

在防御体系中雷达对低空目标一般呈俯视状况,因此在电波折射修正中必须把地球视为椭球,而不能视为圆球体,否则会产生很大误差.本文通过雷达测量参数和大地坐标与空间坐标的转换,给出了计算雷达电波射线上任意一点对应地球半径的方法.     

Ti基钎料中添加混合稀土对TC4合金钎焊性能的影响

通过对钎料综合性能的对比,研究了混合稀土的添加对Ti-Zr-Cu-Ni系合金钎料性能,以及对真空钎焊TC4母材的钎缝的组织特征和机械性能的影响。研究结果表明:添加适当含量的混合稀土的钎料熔点降低,润湿性好,钎焊TC4的力学性能好,混合稀土的含量不应超过5%。     

定常幅值小推力登月飞行器轨道研究

 进行了基于平面三体模型的登月飞行器轨道控制方法的研究;研究了从近地低轨道到近月低轨道的飞行轨道;给出了在地球逃逸段、惯性漂移段和月球捕获段的运动轨迹和关键点的参数。提出使用“远地点可达”概念完成了地球逃逸段发动机推力终点的选择和使用飞行器相对月心能量完成了在月球捕获段止推发动机工作初始点的选择。     

基于飞行仿真平台的相关坐标变换模型

飞行力学中相关的飞行器运动方程都是在地面坐标系中建立的,地面坐标系的前提假设"平面大地"与地球表面具有曲率不符,经纬度能真实反映飞行器的飞行情况,但不能直接运用于飞行器运动方程.针对以上情况,提出了能够运用于地面坐标与经纬度相互转换的模型.在飞行仿真平台上,由飞行器运动方程建立相关的飞行机动动作模型,再由提出的坐标变换模型将运动方程中的相关参数转换为经纬度.实验结果表明,坐标变换模型是合理的,具有实用性,能运用于相关的飞行仿真平台中.     

地球非球形对卫星轨道的长期影响及补偿研究

首先建立了地球非球形引力摄动模型,通过对地球非球形引力摄动对卫星轨道的长期影响分析发现,地球非球形引力摄动对卫星轨道升交点赤经和沿迹角的漂移量与时间成近似线性关系;然后推导了通过主动偏置半长轴和倾角的方法来补偿摄动长期影响的计算公式,设计了基于仿真的地球非球形引力摄动补偿方法;最后对GlobalStar星座卫星进行仿真与试验.结果表明,设计的补偿方法是可行的,摄动补偿后在地球非球形引力摄动作用下卫星轨道的长期稳定性得到了很好的保持.     

An autonomous celestial navigation method for LEO satellite based on unscented Kalman filter and information fusion

A reliable and secure navigation system and assured autonomous capability of satellite are in high demand in case of emergencies in space. Celestial navigation is a fully autonomous navigation method for satellite. To near earth satellite, the earth direction is the most important measurement and the horizon sensing accuracy is the most important factor which effects celestial navigation accuracy. According to the mode of acquiring horizon measurement, satellite celestial navigation methods can be broadly classified into two approaches: directly sensing horizon using earth sensor and indirectly sensing horizon by observation of starlight atmospheric refraction. For these two methods are complementary to each other, a new Unscented Kalman Filter (UKF) based information fusion method is proposed here for hybriding them. Compared to the traditional celestial navigation method, this method can provide better navigation performance and higher reliability. The hardware-in-loop test results demonstrate the feasibility and effectiveness of this method, in most cases the accuracy is sufficient for near earth civilian satellite and moreover it can be used as a backup system to provide redundancy.     

稀土元素及杂质在铝锂合金中的作用研究现状与发展

 综述了稀土元素和杂质对铝锂合金微观组织及力学性能的作用,概括了杂质致脆及稀土微合金化的规律与机制,根据已有研究结果,对目前铝锂合金的发展与应用中需要引起重视的问题,提出了某些观点与建议。     

Ce在钛合金阳极化中作用的研究

 研究了 Ce元素在钛合金阳极氧化中的作用。通过对普通工艺和稀土工艺之间氧化膜微观形貌的对比,讨论了 Ce元素对氧化膜完整性的影响。利用能谱分析,说明了 Ce元素加入可以使钛合金表面氧化较为充分,并且 Ce元素参与了氧化膜的组成。采用局部成分分析法确定了膜层的横向分布范围。对氧化膜截面的SEM图进行分析,讨论了 Ce元素对钛合金阳极氧化膜厚度的影响。利用动电位扫描,对普通氧化膜和稀土氧化膜的耐点蚀性进行了比较,表明 Ce盐的加入可以提高钛合金氧化膜抗点蚀的能力。     

The internal constitutions of the inner planets and the moon

The internal structures of the moon, Mars, Venus, and Mercury are examined in the light of what is known about the constitution of the earth. The gravitational figure of the earth as obtained from orbits of artificial satellites is used to estimate the possible deviations from hydrostatic equilibrium on other planets. Observations of the orbital and rotational motion of the moon are consistent with the hypothesis that the interior of the moon supports density inhomogeneities of the same order as those supported by the earth. The available data on the moon are insufficient to determine whether or not the moon is differentiated. The orbits of Phobos and Deimos yield an adequate value for the moment of inertia of Mars. The moment of inertia and the mass are consistent with a metallic core containing about 10 per cent of the mass of Mars. The observations of the possible magnetic field of Mars would be of importance both to the understanding of planetary magnetic fields and elucidating the internal structure of that planet. Seismic investigations on the earth yield an equation of state for silicates to pressures of about 1 × 10⁶ bars. This equation of state is used in determining density variation within Mars.The surface heat flow for the earth is consistent with the hypothesis that the concentration of radioactive elements is the same as that in chondritic meteorites. The observed ratio of potassium to uranium in surface and near-surface rocks is not consonant with the chondritic hypothesis. The moon can be of chondritic composition only if it is differentiated with the radioactivity concentrated in the upper few hundred kilometers. A chondritic composition for Mars would require a differentiation in excess of that consistent with its mass and moment of inertia. It is concluded that a chondritic composition is not a satisfactory chemical model for the inner planets.     

The earth gravitational potential derived from satellite motion

Recent works on the determination of the earth gravitational potential by its dynamical effects to the motion of artificial satellite are reviewed. Future programs to improve the results and to detect from observations effects due to earth tide and any other time variations of the potential to the satellite motions are discussed.     

全球导航卫星系统的测高研究

以美国全球定位系统为代表的全球导航卫星系统具有广泛的应用领域，特点是能够在全球范围和近地空间，全天候地提供飞行器的位置、速度和时间信息。     

GEO卫星地敏自主干扰保护失效实时处置方法

地球同步轨道卫星在每年春分、秋分前后25d左右一般会出现地敏探头太阳干扰,可以采用星上自主方式进行地敏干扰保护,以防御此种干扰的影响。星上自主干扰保护失效时,需要通过地面发送卫星遥控指令处置。由于当前GEO(Geostationary Earth Orbit,地球同步轨道)卫星地球敏感器自主干扰保护失效的实时处置占用遥控平台时间过长,会严重影响卫星有效载荷应用。所以,针对此问题,在地敏确定卫星姿态原理的基础上,分析了地敏自主干扰保护失效的机理,提出了基于软件进程的地敏太阳干扰保护流程和操作计划,设计了基于遥控指令序列的卫星实时判断脚本。经验证,此方法可将遥控平台占用时间从4h缩短至30min以内,为卫星有效载荷应用留出了时间窗口。     

火星自然卫星分析历表的建立

为了解环火星探测器的运动规律,就要构造环火星探测器的轨道分析解,这会涉及2个火星自然卫星的分析历表,因而需要首先构造它们的轨道分析解。由于火星与地球类似,参照建立人造地球卫星轨道摄动解的方法,构造火星自然卫星轨道的摄动分析解,分离出短周期项,即可给出所需要的历表计算公式。将其与JPL网站上提供的历表进行比对,结果表明,所采用的数学模型以及构造轨道摄动解的方法均有效,能够达到期望的精度。     

降低卫星地面站供电中零线对地电压的措施

通过对民航卫星通信网TES/PES设备供电系统的分析,阐述了零地电压的产生及其对设备造成的潜在危害;通过对具体事例的分析,给出3种强电接地保护方式以及电容降压电路的设计。实际应用表明,该方法能有效地降低零地电压的波动,保证设备的稳定运行。     

舱外航天服的轨道空间外热流计算方法

分析了舱外航天服在轨道空间环境的辐射换热热流。采用蒙特卡罗(MonteCarlo)法,计算了航天服及飞船处于各种相对位置时,航天服对飞船的红外辐射角系数;航天服相对于地球位于各种位置时,航天服对地球的红外辐射角系数;在一定太阳照射方向下,飞船及地球对航天服的太阳反射角系数。与文献数据比较,证明此方法计算舱外航天服空间外热流适用性强,结果准确、可靠,能满足工程使用要求。     

Origin of planetary atmospheres

The near absence of noble gases on earth, other than those of radioactive origin, indicates that the earth was formed by the accumulation of planetesimals; this process systematically excluded all constituents that did not enter into the solid phase. The atmosphere and the ocean with many of its dissolved salts have arisen from gases emitted from the earth's interior, a process that continues today. The oxygen in the earth's atmosphere plus a greater quantity that has been removed from the atmosphere to oxidize geologic materials, has arisen mainly from a small excess of photosynthesis over decay of organic material. The atmospheres of Mars and Venus have probably arisen in a manner similar to the atmosphere on earth, by emission from the planetary interiors. However, they have not received any oxygen from photosynthesis and so are nearly oxygen free. Mars has very little water in its atmosphere, and this can be explained by its lower than freezing average surface temperature. Venus also has very little water, and this requires an ad hoc explanation; one possibility is that Venus was formed from much drier planetesimals than was the earth. Mercury and the moon are virtually without atmospheres. Although some gases may be emitted from their interiors, they are presumably rapidly lost by escape. Whatever atmosphere they possess is probably due to the neutralized solar wind that impinges upon them. The outer planets retained volatiles, including hydrogen and helium, to a much greater extent than did the terrestrial planets.     

参考系选择对Kepler广播星历参数拟合精度的影响

通过对MEO、IGSO、GEO三类导航卫星广播星历的开普勒轨道根数拟合方法及其拟合精度的分析研究,得出结论:开普勒轨道根数拟合导航卫星广播星历的方法,能很好吸收坐标变换过程中岁差、章动、极移、地球自转等因素对卫星星历拟合精度的影响。