飞机驾驶舱自动调光系统中光照传感器布局设计

为满足飞机驾驶舱自动调光系统中环境光检测需要,本文提出一种光照传感器布局方法,该布局方法首先利用SPEOS光学仿真软件分析驾驶舱各区域在不同季节、航向、时间点时的环境光分布;其次,结合各区域发光器件分布情况,确定出光照传感器安装的候选位置;最后,在自然光环境下验证光照传感器候选位置的合理性,并根据验证结果确立光照传感器安装位置。该布局设计方法结合了光分布仿真分析的快速性、可重复性和自然光环境验测真实性的优点,能实现驾驶舱光照传感器的合理布置,为驾驶舱自动调光系统提供准确的环境光信息。     

Estimation of the Love and Shida numbers: h2, l2 using SLR data for the low satellites

In this paper we present results for the global elastic parameters: Love number h₂ and Shida number l₂ derived from the analysis of Satellite Laser Ranging (SLR) data. SLR data for the two low satellites STELLA (H = 800 km) and STARLETTE (H = 810 km) observed during 2.5 years from January 3, 2005 until July 1, 2007 with 18 globally distributed ground stations were analyzed. The analysis was done separately for the two satellites. We do a sequential analysis and study the stability and convergence of the estimates as a function of length of the data set used.     

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.     

Wireless sensor networks for planetary exploration: Experimental assessment of communication and deployment

Planetary surface exploration is an appealing application of wireless sensor networks that has been investigated in recent years by the space community, including the European Space Agency. The idea is to deploy a number of self-organizing sensor nodes forming a wireless networked architecture to provide a distributed instrument for the study and exploration of a planetary body. To explore this concept, ESA has funded the research project RF Wireless for Planetary Exploration (RF-WIPE), carried out by GMV, SUPSI and UPM. The purpose of RF-WIPE was to simulate and prototype a wireless sensor network in order to assess the potential and limitations of the technology for the purposes of planetary exploration.     

高阶带谐摄动下卫星相对运动精确动力学模型

在考虑J 2 项摄动的卫星相对运动精确动力学模型基础上,推导了可以精确到任意阶带谐非球形引力摄动的卫星相对运动精确动力学模型,还给出了一组简洁的基于参考卫星轨道要素（Reference Satellite Variables）的微分方程,能够描述精确到任意阶带谐非球形引力的卫星地球轨道运动。由于在模型推导过程中没有引入任何简化,新推导的结果适用于任意偏心率的地球轨道。     

改进高斯混合粒子滤波的纯方位目标跟踪算法

针对纯方位跟踪系统非线性较强、传统跟踪滤波方法收敛速度慢且容易发散的问题,提出了一种基于改进高斯混合粒子滤波的纯方位跟踪算法。该算法基于Sigma点卡尔曼滤波(SPKF)和粒子滤波的特点,用有限的高斯混合模型来近似后验状态密度、系统噪声和观测噪声的分布。利用贪心EM算法实现模型的降阶,一定程度上克服了EM算法假定混合成分数为已知、迭代的结果需要依赖初始值、可能收敛到局部最大点和可能收敛到参数空间的边界的缺点,从而改善粒子枯竭的问题。仿真实验结果表明在纯方位跟踪领域,与传统粒子滤波(PF)和基于EM的高斯混合粒子滤波相比,该算法在保持高精度估计能力的同时,具有较强的鲁棒性,是解决非线性系统状态估计问题的一种有效方法。     

改进的卫星广播星历参数模型及其算法

考虑导航卫星受地球周期性的摄动力影响,提出了一种改进的导航卫星星历参数模型,给出了模型参数的计算方法和用该模型外推卫星轨道的计算步骤。仿真计算结果表明：该广播星历参数模型外推能力强,可较好地拟合卫星运动轨道。     

An alternative computation of a gravity field model from GOCE

GOCE is the first satellite with a gravitational gradiometer (SGG). This allows to determine a gravity field model with high spatial resolution and high accuracy. Four of the six independent components of the gravitational gradient tensors (GGT) are measured with high accuracy in the so-called measurement band (MB) from 5 to 100 mHz by the GOCE gradiometer. Based on more than 1 year of GOCE measurements, two gravity field models have been derived. Here, we introduce a strategy for spherical harmonic analysis (SHA) from GOCE measurements, with a bandpass filter applied to the SGG data, combined with orbit analysis based on the integral equation approach, and additional constraints (or stabilization) in the polar areas where no observation is available due to the orbit geometry. In addition, we combined the GOCE SGG part with a set of GRACE normal equations. This improves the accuracy of the gravity field in the long-wavelength parts, due to the complementarity of GOCE and GRACE. Comparison with other models and with external data shows that our results are rather close to the GPS-levelling data in well-selected test regions, with an uncertainty of 4–7 cm, for truncation at degree 200.     

基于动态框搜索的星图中星点获取算法研究

分析星图中星点获取算法的具体流程,针对传统星体目标聚类方法的不足,提出了动态框搜索算法。首先采用固定像素框搜索区域最大灰度值点,然后以该点为中心,结合星图图像中真实星点的分布情况,采用大小可变的像素框进行星体目标聚类,最后采用加权质心法得到星点的中心位置。仿真实验表明,该算法能达到良好的效果。     

船岸网络时延测量误差原因分析

简单介绍了测量船船岸通信网络组成,重点介绍了NTP（网络时间协议）和PTP（精密时间协议）这2种网络时间同步协议。针对改建后的船岸网络时延测量误差进行分析和研究,提出基于TWSTFT（卫星双向时间频率传输）技术模型的网络时延测量方法,测量结果误差小于3ms,满足测控任务实时性要求,为提高测控网的测控精度提供有益参考。