兆瓦级空间核电源碱金属朗肯循环热电转换系统设计

为解决火星探测任务中存在的星表供电问题,制定了以空间液态金属朗肯循环作为星表基地热电转换模块的任务规划,采用Simulink模块化建模方法对空间液态金属朗肯循环模型进行程序化描述.根据空间朗肯循环各部件的耦合标准,建立系统部件及总体控制仿真模型,重点研究变运行条件下循环输出功率的波动.研究表明:在本文各工况下,朗肯循环...     

基于拉丁超立方抽样的五孔探针标定方法

为提高五孔探针的标定效率,研究了一种采用拉丁超立方抽样技术开展变马赫数五孔探针标定的试验方法.马赫数在0.2～0.5范围内的对比试验结果表明:采用改进的拉丁超立方抽样标定技术可使攻角与侧滑角的拟合误差较一般拉丁超立方抽样方法下降14.3％～28.6％,且攻角与侧滑角的拟合方均根误差均在1°以内,马赫数的拟合方均根误差不...     

低成本卫星测控系统性能改进方法研究

首先针对TLE更新不及时、轨道递推准确性低的问题,提出低成本卫星测控系统(LCTTC)采用卫星GPS实测数据修正站心坐标系下目标轨道方法,提高跟踪精度;其次利用接收机的RSSI功能,给出了远程获取无人值守LCTTC灵敏度、评估其性能的方法,以及获取信噪比、发射功率等状态信息的方法,对卫星实时任务过程进行监测和异常诊断,减少了故障排查时间。     

基于萤火一号技术的自主火星探测器方案

提出了基于萤火一号（YH-1）火星探测器技术的自主火星探测器方案,可携带多种有效载荷在准太阳同步圆轨道上对火星进行科学探测。该方案具有可实现性强、成本低、研制周期短等特点,并能满足火星探测后续工程中的环绕器设计要求,利于我国火星探测的长远发展。利用长征三号乙运载火箭,在西昌卫星发射中心就可实现2013/2016年的我国自主火星探测。     

连续式跨声速风洞短轴探管设计与试验

为深入研究不同类型短轴探管的测值特性，设计了多种无需张线固定的短轴探管，通过风洞试验开展了相关探索研究。试验结果表明:不同外形参数的短轴探管与长轴探管在马赫数在0.95以下时马赫数方均根偏差量差异不超过0.000 3，马赫数修正量差异不超过0.000 8，测值曲线无明显变化；马赫数在1.0~1.4区间时，不同形式的短轴探管与长轴探管的测试结果存在明显差异，优化短轴探管头部外形参数、增加柱段长度可不同程度地降低头部对试验段流场的干扰。      

Distributed satellite autonomous navigation using X-ray pulsars

Distributed X-ray pulsar-based navigation (DXNAV) is an effective method to realize earth-orbit satellite positioning under weak pulsar signal conditions. In this paper, we propose a new DXNAV method based on multiple information fusion. The DXNAV system principle and the pulse phase estimate Cramér-Rao lower bound are deduced. To suppress the calculation complexity and the error source, the X-ray pulsar photon time-of-arrival detected by each satellite is equivalently converted to the leading satellite directly using the inter-satellite link ranging and starlight angular distance measurement. A high precision estimate model of the pulse phase is built using pulsar standard profile, observed profile, and star-geocentric angular distance from distributed satellites. The estimated pulse phase is real-time supplied to the navigation system, which is established in the form of a deviation equation. The two-stage Kalman filter is designed to estimate the pulse phase in profile histogram bin step and the leader position in real-time step. Compared separately with the maximum likelihood phase estimate method and the celestial navigation method using only the star-geocentric angular distance, the simulation analysis shows that the estimation precisions of position and velocity are improved by 29% and 25%.