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。     

航天发射任务测量船应急测控海域设计方法

针对某些航天发射任务中测量船任务海域纬度高、气象复杂多变的特点,提出了测量船应急测控海域的设计方法,为预定任务海域出现危害性以上海况时实施快速正确船舶机动和应急测量工况设计提供依据,给出了设计实例。     

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。     

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。     

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。     

船体变形对航天测量船外弹道测量的影响

简要介绍了航天测量船船体变形测量系统的基本构成、测量原理和测量元素,分析了变形测量数据的基本特性,给出了船载外测数据船体变形修正的方法和计算公式;重点考察研究了船体变形数据对航天测量船外测数据和外测定轨的影响。     

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。     

舰船空气尾流场特性研究

舰船空气尾流场是舰载直升机在非航空型舰船上起降或者在这类舰船附近作业时的主要环境条件，是危及舰载直升机飞行安全的主要因素之一。现以机－舰动态干扰为研究目的。通过各种试验结果的相互比较，验证，综合分析了舰船空气尾流场特性。着重研究了尾流场中涡流区的及变化规律，下洗速度的大小、下洗范围及变化规律，为机－舰动态配合的试验提供了可靠的依据，另外，还结合飞行实践简要地分析了直升机进入尾流场后的反应。     

Numerical study on flow control of ship airwake and rotor airload during helicopter shipboard landing

A numerical study on flow control of ship airwake during shipboard landing is carried out to address the effect of flow control devices on helicopter rotor airload. The in-house Reynolds Averaged Navier-Stokes (RANS) based solver Rotorcraft AeroDynamics and Aeroacoustics Solver (RADAS), with combination of momentum source approach is employed to conduct the helicopter shipboard landing simulation. The control effects of three aerodynamic modifications of ship superstructure, i.e. ramp, notch and flap, in different Wind-Over-Deck (WOD) conditions are discussed. From the steady simulation results, the effect of spatial variation of ship airwake on rotor airloads is concluded. The aerodynamic modifications reduce the strength of shedding vortex and increase rotor normal force through delaying and relieving flow separation, and therefore are beneficial to alleviate the limitation of control inputs. By contrast, the perturbation of unsteady ship airwake can cause the serious oscillation of rotor forces during shipboard landing. The unsteady simulations show that the turbulence intensity of ship airwake and oscillatory rotor airloading, represented by Root-Mean-Square (RMS) loading, can be remarkably reduced by the ramp and notch modifications, while the flap modification has adverse effect. It means that flow control devices have large potential benefits to alleviate the pilot’s workload and improve the shipboard landing safety, but they should be well designed to avoid the introduction of more vortex, which leads to increase in disturbance of flow field.     

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.