机载单站只测向定位最优机动研究

概述了机载单站只测向定位最优机动求解算法，研究了基于最大方位角变化率准则下的观测机机动轨迹，得到理论上的最优定位机动，并结合实际运用，分析出两种近似最优的机动：“一”形（直线形）机动和S形机动，通过仿真，验证了这2种机动方式在一定条件下可以等效于最优机动，具有良好的定位效果。     

R-PP改性沥青侧缠绕管道防腐作业线的研制与应用

本文着重介绍R-PP改性沥青侧缠绕管道防腐作业线的工作原理及研制过程.通过防腐实验,对作业线存在的若干技术问题进行了改进和调整,为作业线应用于管道防腐提供了必要的技术依据.     

廊坊市体育健身娱乐市场现状调查与对策分析

本文采用问卷调查、文献资料、观察、数理统计、逻辑分析等研究方法,对廊坊市体育健身娱乐经营单位的基本情况、经营状况和居民体育健身娱乐消费情况进行了调查研究,揭示了市场供求的现状特征及存在的问题,并据此提出了拓展廊坊市体育健身娱乐市场的若干对策.     

关于高校学生干部队伍建设的几点思考

本文明确了指导高校学生干部队伍建设的重要性,并提出以科学发展观建设高校学生干部队伍的办法,以求进一步提高学生干部的综合能力,为学校的学生工作管理提供一些参考.     

圆柱形霍尔推力器的内磁极刻蚀研究

由实验后的圆柱形霍尔推力器来看,内磁极刻蚀是影响霍尔推力器寿命以及效率的主要因素之一.主要结合实验结果,从理论卜分析刻蚀以及刻蚀形貌形成的原因.并利用PIC粒子模拟跟踪离子的轨迹来解释内磁极的刻蚀问题.结果表明:推力器的工作状态、电磁场位形是影响内磁极刻蚀及刻蚀形貌的主要囚素.最后针对刻蚀原因提出了相应的减小刻蚀的方法,并比较了各种方法所起的作用.     

考虑轨道摄动的外热流计算分析

为改进传统外热流算法未考虑外热流经多次反射后的吸收和国外商业软件未考虑轨道摄动及太阳矢量变化对外热流的影响等不足,重新定义了外热流角系数和外热流辐射传递因子,综合SGP4轨道模型和Gebhart方法,给出了考虑摄动等因素的辐射传递因子和轨道外热流计算模型,以及相应的计算流程。通过仿真分析论证了考虑多次反射及摄动等因素的重要性。     

Studies of vegetation and soils from aerospace measurements

The problem of soil and vegetation recognition with the use of satellite-derived digitized images and sub-satellite spectral brightness measurements at test sites data is discussed. A technique for retrieval of soil humus content is suggested.     

基于干扰观测器的四旋翼无人机离散时间容错控制

为了飞行控制方案便于在计算机上实现，针对具有外部干扰和执行器加性故障的四旋翼无人机（UAV）角度运动方程，给出一种基于干扰观测器的离散时间跟踪控制方案。通过设计离散时间干扰观测器抑制外部干扰和执行器故障的不利影响，并结合干扰观测器设计离散时间控制器。通过数值仿真验证了基于干扰观测器的离散时间容错控制方案的有效性。仿真结果表明，设计的离散控制器能够保证外部干扰和执行器故障综合作用下的四旋翼UAV系统跟踪控制性能。     

The RadioAstron project: Measurements and analysis of basic parameters of space telescope in flight in 2011–2013

The results of a large number of the antenna radiometric measurements at bands of 92, 18, 6.2, 1.35, and 1.7-1.2 cm are presented by the data of the standard telemetry system of the Spektr-R spacecraft. Both special sessions of calibration object observations in the mode of a single space radio telescope (SRT) operation and numerous observations of researched sources in the mode of the ground-space interferometer were used. The obtained results agree with the first results of Kardashev et al. (2013), i.e., within 10–15% at bands of 92, 18, and 6.2 cm and 20–25% at the band of 1.35 cm. In the main, the measurements for the eight subbands at wavelengths of 1.7-1.2 cm indicate a monotonic increase in the spectral system equivalent flux density (SEFD) of noise radiation with a frequency consistent with the calculated estimates for the discussed model. The sensitivity of the ground-space interferometer for the five subbands at wavelengths from 1.35 to 1.7 cm can be higher by a factor of 1.5, and for the three subbands from 1.35 to 1.2 cm lower by a factor of 1.5 than at the band of 1.35 cm. The SRT contribution to the interferometer sensitivity proportional to the square root of SEFD is close to the design one at the bands of 92 and 18 cm and decreases the design sensitivity approximately by a factor of 1.5 and 2 at the bands of 6.2 and 1.35 cm, respectively. These differences of implemented values from the design ones were not significantly affected the scientific program implementation.