自由返回轨道的P平面参数快速设计方法

针对自由返回轨道求解过程中地心轨道类型变化造成的B平面参数方法计算失败问题,提出一种基于P平面参数的自由返回轨道快速设计方法。首先,基于轨道半通径参数的普适性,给出了不同轨道类型的P平面参数定义,建立了以P平面参数为求解目标量的自由返回轨道求解模型。其次,给出了基于P平面参数的自由返回轨道快速设计方法,在构建的瞬时地月惯性系下,以平面双二体自由返回轨道作为初值,实现了高精度力模型下的自由返回轨道快速求解。对8种构型自由返回轨道的设计结果表明,P平面参数具有类似于B平面参数的大收敛域,且有效解决了轨道类型变化对计算的影响,可直接应用于中国后续月球探测任务轨道设计。     

Dynamical evolution of high area-to-mass ratio debris released into GPS orbits

A large set of simulations, including all the relevant perturbations, was carried out to investigate the long-term dynamical evolution of fictitious high area-to-mass ratio (A/M) objects released, with a negligible velocity variation, in each of the six orbital planes used by Global Positioning System (GPS) satellites. As with similar objects discovered in near synchronous trajectories, long lifetime orbits, with mean motions of about 2 revolutions per day, were found possible for debris characterized by extremely high area-to-mass ratios. Often the lifetime exceeds 100 years up to A/M ∼ 45 m²/kg, decreasing rapidly to a few months above such a threshold. However, the details of the evolution, which are conditioned by the complex interplay of solar radiation pressure and geopotential plus luni-solar resonances, depend on the initial conditions. Different behaviors are thus possible. In any case, objects like those discovered in synchronous orbits, with A/M as high as 20–40 m²/kg, could also survive in this orbital regime, with semi-major axes close to the semi-synchronous values, with maximum eccentricities between 0.3 and 0.7, and with significant orbit pole precessions (faster and wider for increasing values of A/M), leading to inclinations between 30° and more than 90°.     

空间目标轨道确定专家系统

空间目标轨道确定专家系统的面向空间监测需求开发的大型交互式应用软件。它的功能面向空间监测和信息分析中广泛的业务需求，基础是轨道计算软件，数据库支持和一些辅助支持软件。本文详细地介绍了空间目标轨道确定专家系统软件的设计方案。     

简单二体引力模型用于空间目标轨道面交线确定的效果分析

在空间目标碰撞预警分析中，准确地计算出空间目标的轨道面交线是进行地心距筛选、时间差筛选的前提，目前较多使用的快速确定轨道面交线的方法为简单二体引力模型。深入分析该模型，比较了其计算的空间目标轨道面交线与STK计算结果的差异，指出了简单二体引力模型在计算空间目标轨道面交线时的局限性，认为轨道摄动是影响轨道面交线计算准确性的主要原因，应该采用更能反映空间目标实际运动规律的改进的二体引力模型的方法。     

WSO／UV（世界空间紫外天文台）的轨道特征与轨道保持

WSOO／UV(世界空间紫外天文台)需要发射到日-地(月)系的共线平动点L1附近进行巡天观测，相对日-地(月)要求其几何位置几乎不变，因此有必要阐明共线平动点的动力学特征及其附近的运动状况。本文基于这一点，对限制性三体模型下，日-地(月)系中共线平动点附近扰动运动的稳定性作了理论分析，给出了WSO／UV轨道保持的条件及其在运行阶段的轨控措施。     

直接解算轨道根数的轨道约束自校准定轨方法

应用轨道约束自校准技术能够有效地修正系统误差和提高定轨精度。本文为了适应各种航天试验任务要求,将轨道约束自校准技术推广应用到直接解算轨道根数的定轨方法中,并导出了解算开普勒根数的轨道约束自校准公式。     

太阳同步卫星双星组网维持策略

某准共面星座由两颗相位差为 180°的太阳同步卫星组成。在对其进行轨道维持时 ,需综合考虑相位差和地面轨迹范围两方面的限制。然而 ,由于这两颗卫星的轨道倾角存在差异 ,使得在轨道维持过程中不能同时满足相位差和地面轨迹的要求。为解决上述问题 ,本文提出了调整地面参考轨迹的方法 ,实践证明有效。     

First results from the LUCID-Timepix spacecraft payload onboard the TechDemoSat-1 satellite in Low Earth Orbit

The Langton Ultimate Cosmic ray Intensity Detector (LUCID) is a payload onboard the satellite TechDemoSat-1, used to study the radiation environment in Low Earth Orbit ($～$635?km). LUCID operated from 2014 to 2017, collecting over 2.1 million frames of radiation data from its five Timepix detectors on board. LUCID is one of the first uses of the Timepix detector technology in open space, with the data providing useful insight into the performance of this technology in new environments. It provides high-sensitivity imaging measurements of the mixed radiation field, with a wide dynamic range in terms of spectral response, particle type and direction. The data has been analysed using computing resources provided by GridPP, with a new machine learning algorithm that uses the Tensorflow framework. This algorithm provides a new approach to processing Medipix data, using a training set of human labelled tracks, providing greater particle classification accuracy than other algorithms. For managing the LUCID data, we have developed an online platform called Timepix Analysis Platform at School (TAPAS). This provides a swift and simple way for users to analyse data that they collect using Timepix detectors from both LUCID and other experiments. We also present some possible future uses of the LUCID data and Medipix detectors in space.     

低轨天基信息定向分发区域分割编码控制方法

为提高低轨指向性信息分发链路的频谱利用效率，从天基分发平台与地面用户的相对位置关系入手，建立了分发指向、编码增益与信道传输容量的量化关系。在此基础上，提出一种低轨天基信息定向分发区域分割编码控制方法，该方法针对不同信息分发区域，采用最小均方误差(MMSE)作为区域分割准则选择编码方式，既提升了信道传输效率也便于工程实现。最后，本文通过仿真分析了方法的效能和性能影响因素，并与现有自适应编码方法进行了对比，验证了本方法的有效性和可靠性。