船载多目标模拟器的构建与应用

船载统一S频段（USB）测控系统是我国航天测控网的重要组成部分,承担着一箭单星或一箭多星的海上测控任务。从航天测量船执行多目标测控任务的特点出发,分析了测量船船载飞行目标模拟器的现状以及对多目标模拟器的需求。提出了在船载USB联试应答机的基础上,通过改造应答机的部分模块,构成多目标模拟器的方法,并成功地在某次实战任务中得到了应用。     

Optimisation of X-ray proportional counters for Scanning Sky Monitor (SSM) on ASTROSAT

The Scanning Sky Monitor (SSM) on ASTROSAT is a position-sensitive gas-filled proportional counter with a wide field of view. The scientific objective of SSM is to scan the sky within few hours to detect and locate transient X-ray sources in the outburst phase. Once detected, this information will be provided for studies in all energy bands. The energy range of operation of SSM is 2–10 keV. The optimisation of the parameters of the proportional counter such as the cell size, the gas mixture and the gas pressure for the SSM are discussed here.     

机载雷达测控站性能分析CSCD

陆基、海基测控设备在跟踪低空特别是超低空飞行目标时受视距影响大,作用距离有限,而机载测控站作为空中测量平台,不受视距影响,有很大发展空间。介绍了机载测控站的组成、功能和工作原理,分析了机载测控站相关参数关系和工作能力,提出了提高跟踪能力的方法措施;给出了系统跟踪距离计算公式,通过几种典型目标速度分析了系统的跟踪能力,并与陆基、海基测控设备的跟踪能力进行了比对。结果表明,机载测控站在跟踪低空目标时作用距离较远,在低弹道大射程目标飞行试验中具有较大的应用空间。     

对测量雷达的一些新需求与精细测量技术

新一代测量雷达在发展各种先进武器平台与航空航天及空间技术方面有广泛的应用前景。本文讨论对测量雷达的一些新的需求及相关技术,对雷达精细测量的需求与有关技术是本文讨论重点。     

微波统一测控系统的电子防护能力分析与对策建议

通过对微波统一测控系统的电子防护能力和安全威胁分析,给出了进一步提高电子防护能力的对策建议。     

应用CFD方法的舰载直升机舰面气弹响应计算与分析

舰载直升机所处的环境恶劣,易出现旋翼桨尖过度挥舞及机身碰撞等事故,研究直升机舰面气弹响应可预防此类事故的出现。应用 CFD 方法获得舰船流场数据,结合桨叶动力学模型,综合提出旋翼气弹响应计算分析方法,研究不同来流速度、悬停位置与风向角下旋翼的气弹响应。结果表明：本文提出的气弹响应计算分析方法正确可行;舰船来流速度的增加...     

船舶电压表（电流表）现场检定技术可行性初探

分析了船用电压表（电流表）现场检定的必要性,并以XF30A-2多功能校准源为主标准器,研究了环境温湿度变化对其技术指标的影响,探讨了利用该标准器对船舶电压表（电流表）开展现场检定工作的可行性。     

The Radio Observatory on the Lunar Surface for Solar studies

The Radio Observatory on the Lunar Surface for Solar studies (ROLSS) is a concept for a near-side low radio frequency imaging interferometric array designed to study particle acceleration at the Sun and in the inner heliosphere. The prime science mission is to image the radio emission generated by Type II and III solar radio burst processes with the aim of determining the sites at and mechanisms by which the radiating particles are accelerated. Specific questions to be addressed include the following: (1) Isolating the sites of electron acceleration responsible for Type II and III solar radio bursts during coronal mass ejections (CMEs); and (2) Determining if and the mechanism(s) by which multiple, successive CMEs produce unusually efficient particle acceleration and intense radio emission. Secondary science goals include constraining the density of the lunar ionosphere by searching for a low radio frequency cutoff to solar radio emission and constraining the low energy electron population in astrophysical sources. Key design requirements on ROLSS include the operational frequency and angular resolution. The electron densities in the solar corona and inner heliosphere are such that the relevant emission occurs at frequencies below 10 MHz. Second, resolving the potential sites of particle acceleration requires an instrument with an angular resolution of at least 2°, equivalent to a linear array size of approximately 1000 m. Operations would consist of data acquisition during the lunar day, with regular data downlinks. No operations would occur during lunar night.     

Future Instrumentation for the Study of the Warm-Hot Intergalactic Medium

We briefly review capabilities and requirements for future instrumentation in UV- and X-ray astronomy that can contribute to advancing our understanding of the diffuse, highly ionised intergalactic medium.     

海上航天测控系统领域本体的构建研究

随着我国航天事业的高速发展,对海上测控系统提出了越来越高的要求。测量船执行任务时涉及飞行器、船载设备、测量船工况等任务要素。本文根据任务要素的主要层次关系及它们之间的约束关系,构建了海上航天测控系统领域本体TTC_Onto,其实现和应用可以有效地提高任务分析的灵活性和准确性。并给出了TTC_Onto的构建过程及其评价机制。