A comparative study of ionospheric IRIEup and ISP assimilative models during some intense and severe geomagnetic storms

Three-dimensional (3-D) electron density matrices, computed in the Mediterranean area by the IRI climatological model and IRIEup and ISP nowcasting models, during some intense and severe geomagnetic-ionospheric storms, were ingested by the ray tracing software tool IONORT, to synthesize quasi-vertical ionograms. IRIEup model was run in different operational modes: (1) assimilating validated autoscaled electron density profiles only from a limited area which, in our case, is the Mediterranean sector (IRIEup_re(V) mode); (2) assimilating electron density profiles from a larger region including several stations spread across Europe: (a) without taking care of validating the autoscaled data in the assimilation process (IRIEup(NV)); (b) validating carefully the autoscaled electron density profiles before their assimilation (IRIEup(V)).The comparative analysis was carried out comparing IRI, IRIEup_re(V), ISP, IRIEup(NV), and IRIEup(V) foF2 synthesized values, with corresponding foF2 measurements autoscaled by ARTIST, and then validated, at the truth sites of Roquetes (40.80°N, 0.50°E, Spain), San Vito (40.60°N, 17.80°E, Italy), Athens (38.00°N, 23.50°E, Greece), and Nicosia, (35.03°N, 33.16°E, Cyprus). The outcomes demonstrate that: (1) IRIEup_re(V), performs better than ISP in the western Mediterranean (around Roquetes); (2) ISP performs slightly better than IRIEup_re(V) in the central part of Mediterranean (around Athens and San Vito); (3) ISP performance is better than the IRIEup_re(V) one in the eastern Mediterranean (around Nicosia); (4) IRIEup(NV) performance is worse than the IRIEup(V) one; (5) in the central Mediterranean area, IRIEup(V) performance is better than the IRIEup_re(V) one, and it is practically the same for the western and eastern sectors.Concerning the overall performance, nowcasting models proved to be considerably more reliable than the climatological IRI model to represent the ionosphere behaviour during geomagnetic-ionospheric storm conditions; ISP and IRIEup(V) provided the best performance, but neither of them has clearly prevailed over the other one.     

机载系统NANDFlash存储技术

为了发挥NANDFlash在机载环境中非易失性、体积小、固态性、重量轻、低功耗、抗震动等特点,介绍了NANDFlash的存储特性,对NANDFlash存储的关键技术进行了改进,提出了基于域机制的地址映射方式和基于阈值的损耗均衡方法,为机载系统能够更加可靠、实时和安全地进行数据存储提供了选择。     

星载相控阵GNSS-R测高系统设计与实验

星载GNSS-R测高系统采用多波束相控阵天线和干涉互相关处理方式,接收北斗导航卫星和GPS导航卫星发射的L波段导航直射信号与海面反射信号,进行海面高度探测。详细介绍GNSS-R测高系统设计与实现、集成和外场试验等,外场试验不仅验证了相控阵GNSS-R测高系统功能,更重要的是验证了核心软件算法的正确性。GNSS-R测高系统适用于中尺度海洋现象的观测,可在时间和空间尺度上扩展雷达高度计的观测能力,并与之相互补充,有利于对复杂海面的中尺度结构进行较高时间分辨率的观测。GNSS-R测高仪为星载高精度海面高度探测提供了新型载荷。     

面向月球科研站任务的地月准实时遥操作模拟验证系统设计与关键技术研究

针对月球科研站任务地月遥操作需求和特点,设计地月准实时遥操作模拟验证系统,对其中的关键技术海量多尺度遥感数据环境感知、空地协同高精度定位、基于混合现实的预测仿真等进行了研究。提出了基于海量多尺度遥感数据的联合处理方法,环境感知数据融合可处理米级至厘米级环境感知结果;设计基于空地多运动平台协同定位的原型软件,空地协同地标约束下,定位精度不低于轨道器影像1个像素;开发了带有力觉反馈的预测仿真验证平台,在2~3 s变时延约束下可在仿真环境下协同演示遥操作过程,真实还原从端的遥操作作业场景,提高遥操作的执行效率和安全性。为地面人员的方案设计、操作手训练、故障处置等提供实时支持,为我国未来实施月球科研站任务筑牢基础。     

内压缩通道几何参数对高超声速进气道性能的影响

用N-S方程模拟了一系列不同收缩比、不同波系配置的内压缩通道内流动,研究了内压收缩通道几何参数对进气道性能的影响,发现对于相同的外压段,内压面积收缩比对进气道内压缩通道温升比、压比和起动性能具有较好的相似规律,且随着内压面积收缩比增加,进气道温升比、压比增加,出口流场畸变下降,起动马赫数增大。通过对相同压比下不同内外压缩比的进气道性能的研究,得到了内外压缩比对进气道效率和起动性能的影响规律,发现压缩程度相同时,进气道效率和起动马赫数均随内外压缩比有先增大后减小再增大的规律。     

一种航天测控系统可靠性定量化计算方法

航天测控系统具有动态性、复杂性、可维修性、阶段间相关性等显著特征,作为航天器安全在轨运行的重要保障,其可靠性至关重要。针对航天测控系统可靠性精确计算的难点,提出了综合马尔可夫（Markov）模型和全概率思想的复杂、动态系统可靠性定量化计算方法,给出了计算流程。按照系统的动态组成特性,将任务进程划分为多个阶段,阶段内参试状态不变,不同阶段之间参试状态不同。借鉴Markov模型描述阶段内状态转移过程,通过求解Kolmogorov后向方程得到本阶段结束时的状态概率,利用全概率思想实现阶段间状态映射,体现阶段间的依赖性,依次对各阶段求解获取整个任务可靠性,具有求解准确度高、结果可信度高等特点。最后给出算例,通过与蒙特卡洛仿真结果的比对校验Markov方法的准确性。     

基于高分卫星姿态监测的姿态参数算法优化

目前航天测绘相机几何参数的在轨标定通常经由地面检校场数据处理完成。然而,由于一次摄影中难以保证获取的地面检校场影像完整,使得在轨标定周期较长,进而导致实时监测与标定非常困难。“高分十四号”卫星搭载了一种新的姿态测定系统,利用高精度的相机光轴监测实现对相机几何参数的在轨实时标定。文章在此基础上对高分卫星星地相机间夹角在轨解算方案进行了优化,并基于数值仿真和在轨实测数据进行了分析,结果显示优化算法可以进一步提高影像内定向稳定度和最终的定位精度,未来有望在高精度立体测绘应用中发挥重要作用。     

Manifold dynamics in the Earth–Moon system via isomorphic mapping with application to spacecraft end-of-life strategies

Recently, manifold dynamics has assumed an increasing relevance for analysis and design of low-energy missions, both in the Earth–Moon system and in alternative multibody environments. With regard to lunar missions, exterior and interior transfers, based on the transit through the regions where the collinear libration points L₁ and L₂ are located, have been studied for a long time and some space missions have already taken advantage of the results of these studies. This paper is focused on the definition and use of a special isomorphic mapping for low-energy mission analysis. A convenient set of cylindrical coordinates is employed to describe the spacecraft dynamics (i.e. position and velocity), in the context of the circular restricted three-body problem, used to model the spacecraft motion in the Earth–Moon system. This isomorphic mapping of trajectories allows the identification and intuitive representation of periodic orbits and of the related invariant manifolds, which correspond to tubes that emanate from the curve associated with the periodic orbit. Heteroclinic connections, i.e. the trajectories that belong to both the stable and the unstable manifolds of two distinct periodic orbits, can be easily detected by means of this representation. This paper illustrates the use of isomorphic mapping for finding (a) periodic orbits, (b) heteroclinic connections between trajectories emanating from two Lyapunov orbits, the first at L₁, and the second at L₂, and (c) heteroclinic connections between trajectories emanating from the Lyapunov orbit at L₁ and from a particular unstable lunar orbit. Heteroclinic trajectories are asymptotic trajectories that travels at zero-propellant cost. In practical situations, a modest delta-v budget is required to perform transfers along the manifolds. This circumstance implies the possibility of performing complex missions, by combining different types of trajectory arcs belonging to the manifolds. This work studies also the possible application of manifold dynamics to defining suitable, convenient end-of-life strategies for spacecraft orbiting the Earth. Seven distinct options are identified, and lead to placing the spacecraft into the final disposal orbit, which is either (a) a lunar capture orbit, (b) a lunar impact trajectory, (c) a stable lunar periodic orbit, or (d) an outer orbit, never approaching the Earth or the Moon. Two remarkable properties that relate the velocity variations with the spacecraft energy are employed for the purpose of identifying the optimal locations, magnitudes, and directions of the velocity impulses needed to perform the seven transfer trajectories. The overall performance of each end-of-life strategy is evaluated in terms of time of flight and propellant budget.     

基于分层神经网络的航天器故障诊断技术

为了提高卫星、飞船等复杂系统的故障诊断速度和精度,文章提出了一种基于分层神经网络的整星故障诊断模型。模型中的上层神经网络采用自组织特征映射网络,完成整星故障的初步定位与辨识;下层神经网络采用广义回归神经网络,实现整星各分系统故障的精确定位和定因。引入主元分析法实现原始状态变量的降维,减少神经网络神经元数量。该模型已成功应用于某卫星各分系统的故障诊断,提高了诊断效率,并能精确给出诊断结果。