红外地球敏感器测量误差分析及修正方法

红外地球敏感器作为卫星平台重要设备，在对地指向、姿态测量和天文自主导航等方面发挥着重要作用，高精度的地球敏感器量对于提高卫星姿态控制和天文自主导航精度具有重要意义。本文通过分析地敏测量误差的影响因素，提出随季节变化的地球CO2辐射特性是影响地敏测量精度的重要因素;根据地球辐射模型构建了地敏测量修正方法，结合在轨实测数据分析验证，证明可以大大降低由地球辐射不均匀引发的误差，有效压缩地敏在轨测量误差。     

航空航天用高强度Mg-RE系合金的研究进展

近年来，镁稀土合金由于其高强度、低密度和高温性能良好等特点，在追求轻量化的航空航天产业当中受到越来越多的关注。总结当前主流的2系高强度Mg-RE合金(Mg-Gd和Mg-Y系合金)的性能特点、强化机制和研究进展，简要介绍其他Mg-RE合金的研究情况，最后回顾镁稀土合金在航空航天领域的应用。     

StarLink星座对空间安全态势的影响

针对StarLink星座部署后带来的空间安全问题，对StarLink星座构型仿真，利用碰撞概率的算法，从碰撞风险的角度分析了StarLink星座部署后对其他卫星在轨安全的影响。结果表明:StarLink星座部署对低轨航天器将带来较大的碰撞风险，碰撞风险比部署前提升一个量级，对535~555 km空间区域的航天器影响尤为突出，一旦产生碰撞碎片将带来更大的碰撞风险。通过分析提出了警示，并针对大型卫星星座带来的碰撞危险提供了应对建议。     

Advanced analytical model for orbital aerodynamic prediction in LEO

The growing interest in low earth orbit (LEO) applications demands for accurate modeling of orbital aerodynamics. But classical analytical models of aerodynamic coefficients in free molecule flow, such as the Sentman’s model, Schamberg’s model and Schaaf-Chambre model, were built upon over simplistic gas-surface interaction models, which degrade the fidelity of aerodynamic prediction. This work presents a new analytical model of orbital aerodynamic coefficients based on the state-of-the-art Cercignani–Lampis–Lord (CLL) gas-surface interaction model, where lobular quasi-specular scattering pattern and separate accommodation degree for different velocity components can be well captured. A key component of the new model is a rigorous function approximation solution of the reflected normal momentum flux based on the CLL model which is derived for the first time and is validated within 1% for any hypothermal flow and surface accommodation conditions. Closed-form analytical solutions of aerodynamic coefficients for simple convex geometries are obtained and exhibit high accuracy (within 0.1%) in typical LEO scenarios. The new analytical model surpasses the classical models in some important aspects, such as overcoming the diffuse scattering hypothesis constraint, considering the variation of normal momentum exchange with the surface incidence angle and being applicable in any hypothermal flow situation. In virtue of the advanced CLL model and feasibility of coupling with the panel method technique, the new analytical model is promising to provide more accurate predictions on the orbital aerodynamic coefficients for LEO applications.