Venus observations from ENVISAT–SCIAMACHY: Measurements and modeling

This work shows the capability of observing Venus with a sensor originally designed for Earth remote sensing. SCIAMACHY (SCanning Imaging Absorption spectroMeter for Atmospheric CHartographY), onboard ENVISAT, successfully observed visible and near-infrared spectra from the Venusian atmosphere. The Venus spectra were simulated using a line-by-line radiative transfer model. The single scattering approximation was applied in order to consider the effects of an approximately 20 km-thick haze layer above the main cloud deck, which was considered as a reflecting cloud located in the upper atmosphere of the planet. CO₂ absorption lines could be distinguished in both observed and simulated spectra and a good agreement between them was also found.     

SerDes器件在遥感相机系统中的应用

基于当前遥感相机谱段数量的不断增加、分辨率的不断提升等方面造成的数据传输问题,分析了目前广泛应用的并行数据传输系统所面临的技术瓶颈,提出采用串行发送/解串(SerDes)方式加以替代的方案,通过对比分析,指出采用该方式传输数据的优点,进而阐述文章所采用的串行发送/解串芯片-TLK2711的工作原理、传输协议等,最终通过试验证明了其在遥感相机系统中应用的可行性,为后续遥感相机研制提供参考。     

基于北斗/GNSS精密时频量值传递综述

介绍了北斗/GNSS精密时间频率量值传递技术及其应用研究进展,通过对北斗共视比对技术的研究,设计出利用北斗共视与国家授时中心GNSS CV精密时间服务系统进行比对,从而实现用户与标准时间UTC的溯源完成基于GNSS CV技术的时间频率计量服务系统设计,创新性地提出提高北斗共视比对技术以及研制多模多频GNSS CV量值传递设备的研究方向。     

倾角对含油工质冷凝换热影响的实验研究

随着航天器热控制的发展,蒸气压缩热泵排热系统等热控方式逐渐受到人们的重视,其中冷凝换热对热泵的性能好坏有重要的影响。为了研究重力场对冷凝换热的影响,将紫铜直管冷凝器置于蒸气压缩热泵系统中,通过改变重力场与流动方向的夹角,测量得到了不同倾角下的冷凝换热系数和压降。实验结果表明,倾角对直管内冷凝换热系数的影响较大,不同倾角下的换热系数差别达30%,远大于不同倾角对直管内蒸发换热的影响;压缩机润滑油对冷凝换热的影响也很大,相比较无润滑油冷凝换热系数低30%以上。随着质量流量的增加,压缩机润滑油的影响逐渐减弱。
     

路由算法在LEO通信星座构型优化中的应用

低轨(LEO,Low Earth Orbit)通信星座的特殊功能决定了其构型优化需要综合考虑成本、覆盖和路由性能等因素.以往的研究往往忽略了路由性能,导致优化得到的构型不能很好的满足要求.首先给出了两个意义明确的星座路由性能的评价指标,然后通过将它们作为目标函数进行仿真,验证了其优化必要性和评价有效性.最后利用多目标遗传算法实现了星座的构型优化.仿真结果显示,将路由算法加入到星座的构型优化中,在仅对星座构型参数进行微调的前提下,不仅满足了成本、覆盖等基本要求,而且星座的路由性能大大提高.     

A novel system parameters design and performance analysis method for Distributed Satellite-borne SAR system

As a promising new technology emerged in recent years, the Distributed Satellite-borne SAR (DSS) system with Interferometric Synthetic Aperture Radar (InSAR) imaging capability has been recognized by the remote sensing community as an integrated part of the spaceborne earth observation system. However, most researches on DSS were focused on individual aspects of system design/analysis and data processing, while few studies have been dedicated to establishing a standard methodological framework for universal DSS system design. Aiming at this problem, the topics of DSS system error analysis and design method are investigated in this paper. Firstly, a rigorous error propagation model of height measurement is theoretically derived from the DSS InSAR imaging geometry, and the impact of each error sources in this model on the height measurement accuracy is analyzed individually. In particular, the baseline length and its measurement error in the InSAR imaging plane are identified as the dominant factors. Second, a new method for DSS system design is proposed based on our analyses with the error propagation model. This method consists of two important phases, namely collaboration design and monostatic design. The major objective of collaboration design is to determine the configuration and parameters for the coordination between satellites in the DSS system. Afterwards, the key parameters for single satellite and the payload are determined by the monostatic design. Thirdly, a system performance analysis method is developed to comprehensively evaluate the performance of the pre-designed DSS system. In the next section, a typical example of DSS system design is given to demonstrate the effectiveness of the proposed system design and analysis methods. The target DSS system has the same goal and hardware configuration as the TanDEM-X mission. Finally, the conclusion is drawn with our major findings are presented.     

Formation control using μ-synthesis for Inner-Formation Gravity Measurement Satellite System

Inner-Formation Gravity Measurement Satellite System (IFGMSS) is used to map the gravity field of Earth. The IFGMSS consists of two satellites in which one is called “inner satellite” and the other one is named as “outer satellite”. To measure the pure Earth gravity, the inner satellite is located in the cavity of the outer satellite. Because of the shield effect of the cavity, the inner satellite is affected only by the gravitational force, so it can sense Earth gravity precisely. To avoid the collision between the inner satellite and the outer satellite, it is best to perform a real-time control on the outer satellite. In orbit, the mass of the outer satellite decreases with the consumption of its propellant. The orbit angular rate of the inner satellite varies with time due to various disturbing forces. These two parameters’ uncertainties make the C–W function be not so accurate to describe the formation behavior of these two satellites. Furthermore, the thrusters also have some uncertainties due to the unmodelled dynamics. To cancel the effects caused by the above uncertainties, we have studied the robust control method based on the μ-synthesis. This μ-synthesis eliminates the conservativeness and improves the control efficiency comparing with the H_∞ method. Finally, to test the control method, we simulate an IFGMSS mission in which the satellite runs in a sun synchronous circular orbit with an altitude of 300 km. The simulation results show the effectiveness of the robust control method. The performances of the closed-loop system with the μ-controller are tested by the μ-analysis. It has found that the nominal performance, the robust stability and the robust performance are all achieved. The transient simulation results further prove the control response is fast and the accuracy of the relative position meets the demand of the gravity measurement.     

动态拖尾星图模拟算法研究

星图模拟技术是星图识别算法仿真和性能测试的基础.为了更好地模拟星敏感器在轨工作的情况,对星敏感器的软件开发以及自身性能进行有效的地面测试,提出一种动态拖尾星图模拟算法.该算法分为4个步骤:首先根据星敏感器指向在全天球范围内搜索导航星;接着利用小孔成像模型计算导航星在星敏感器成像面的投影位置;然后在考虑卫星运动引起的恒星拖尾的基础上,按照二维灰度分布规律置灰度值来模拟星像点像素;最后叠加杂散光背景及成像器件引起的噪声.提出的算法具有速度快、精度高及可实现性高等优点.     

载人登月绕月自由返回轨道与窗口精确快速设计

针对载人登月任务背景及工程约束,提出一种轨道与窗口一体化设计方法。通过两次坐标转化,将自由返回轨道设计参数解耦为近月点独立变量。在双二体假设下,通过4段二体轨道拼接完成自由返回轨道初值快速搜索及匹配近地停泊轨道(LEO)面的月窗口,其结果作为下一步采用序列二次规划（SQP）迭代求解高精度动力学模型轨道参数的初值,在该条精确轨道近月点时刻90 min邻域内产生可以匹配LEO地月转移入轨相位的零窗口轨道。算例表明,该流程能够精确快速地完成具有复杂任务背景及苛刻工程要求的载人登月绕月自由返回轨道与窗口设计问题。     

不同月球借力约束下的地月Halo轨道转移轨道设计

针对地月系L2点不同任务需求下的低耗能转移轨道设计问题,基于不变流形理论与混合优化技术,深入研究了不同月球借力约束与不同幅值Halo轨道的入轨点（简称HOI点）对转移轨道飞行时间与燃料消耗的影响,给出了HOI点选择策略。首先结合任务要求并考虑月球引力影响,在月球借力点施加不同约束条件,通过微分修正算法调整Halo轨道的稳定流形,设计月球到Halo轨道的转移轨道。采用遗传算法与微分修正算法相结合的混合优化策略,在同时考虑地球停泊轨道高度、倾角、升交点赤经与航迹角等多约束条件下,对燃料最优的地月转移轨道进行研究。最后,分析月球借力高度、借力方位角和不同HOI点对平动点转移轨道飞行时间与燃耗变化量的影响,对于考虑月球借力的地月平动点转移轨道设计与应用具有重要的参考价值。