Going to Alpha Centauri B and setting up a Radio Bridge

How to exploit the Sun as a gravitational lens has been studied extensively during the last 20 years, especially by this author (Refs. 1, 2, 3, 4, 5, 6 and 7). In essence, a spacecraft dubbed FOCAL (an acronym for “Fast Outgoing Cyclopean Astronomical Lens”) should be launched in the direction of the sky opposite to the area of the sky we wish to see highly magnified both at radio and other frequencies. After FOCAL reached the minimal focal distance of 550 AU from the Sun, highly magnified radio images of celestial objects located on the opposite side of the Sun will automatically be produced. In this paper we apply the FOCAL mission concept to the goal of exploring the neighborhood of the Alpha Centauri B star, where the nearest exoplanet to the Solar system was recently discovered. We suggest that:     

Validation of B0 and B1 in the IRI 2001 model at low solar activity for Ilorin an equatorial station

A new set of data obtained at low solar activity from Ilorin, Nigeria (geog. latitude 8.5°N, geog longitude, 4.6°E, dip 4.1°S) is used to validate the IRI 2001 model at low solar activity. The results show in general a good agreement between model and observed B0 at night but an over estimation during daytime. The overestimation is greatest during the morning period (0600LT–1000LT). The model prediction for B1 is fairly good at night and during the day. A dependence of B0 on solar zenith angle χ is observed during the daytime. A formulation of the form B0 = A[cos(χ)ⁿ] is therefore proposed. Values of the constants n and A were determined for the period of low solar activity for this station.     

多路传输数据总线监控器的设计

介绍一种用于航空电子综合化系统的1553B总线监控器的设计.讨论了总线监控器的结构、功能及相应的软件设计.     

电离层f_0F_2参数提前24小时预测

利用中国9个垂测站(海口、广州、重庆、拉萨、兰州、北京、乌鲁木齐、长春、满洲里)一个太阳周(1976-1986年)的数据资料,采用三层前向反馈神经网络(BP网络)实现了电离层F2层临界频率(f0F2)参数提前24h预测.通过对f0F2参数的时间序列及其与日地活动之间进行相关分析,确定f(t)(当前时刻f0F2)、经过变换的F10.7指数等5个参数作为神经网络的输入参数,并通过同时段训练法获得不同时刻的预测值,本文与自相关分析法进行了预测性能比较.结果表明,上述方法构建的神经网络可以达到较高的预测精度.针对暴时数据,对神经网络算法进行了改进,提高了神经网络法对暴时数据的适用性.     

An inversion approach for lunar regolith layer thickness using optical albedo data and microwave emission simulation

An approach to inversion of the lunar regolith layer thickness by using multi-channel brightness temperature observation in passive microwave remote sensing is developed. To first make simulation of brightness temperature from the lunar layered media, the lunar regolith layer thickness (d) is proposed being constructed by available lunar DEM (digital elevation mapping) and on site measurements. The physical temperature distribution (T) over the lunar surface is also empirically assumed as a monotonic function of the latitude. Optical albedo of the lunar nearside from the telescopic observation is employed to construct the spatial distribution of the FeO+TiO₂ content (S) in the lunar regolith layer. A statistic relationship between the DEM and S of the lunar nearside is further extended to construction of S of the lunar farside. Thus, the dielectric permittivity (ε) of global lunar regolith layer can then be determined. Based on all these conditions (d,T,ε), brightness temperature of the lunar regolith layer in passive microwave remote sensing, which is planned for China's Chang-E lunar project, is numerically simulated by a parallel layering model using the strong fluctuation theory of random media.Then, taking these simulations with random noise as observations, an inversion method of the lunar regolith layer thickness is developed by using three- or two-channels brightness temperatures. When the S is low, and the four channels brightness temperatures in China's Chang-E project are well distinguishable, the regolith layer thickness and physical temperature of the underlying lunar rock media can be inverted by the three-channels approach. When the S becomes high that the brightness temperature at high frequency channels such as 19.35, 37 GHz are saturated, the regolith layer thickness is alternatively inverted only by the two-channels approach.Numerical simulation and inversion approach in this paper make an evaluation of the performance for lunar passive microwave remote sensing, and for future data calibration and validation.     

涡桨发动机总体性能优化设计

为提高非设计状态下发动机总体性能预估精度,发展了0D/2D耦合总体性能预估方法。针对某型3轴涡轮螺旋桨发动机建立了基于T-MATS平台的涡桨发动机总体性能0D仿真模型。对涡桨发动机可用功分配提出了2种优化方案。对原方案和2种优化方案的自由涡轮、尾喷管2个部件进行了2D流道和叶型设计,通过S_1流面与通流CFD计算验证了所设计部件的气动性能满足发动机总体性能指标要求。为提高非设计状态下发动机总体性能预估精度,采用0D/2D耦合总体性能预估方法分析了3种方案。结果表明:优化方案1使发动机当量耗油率在设计、巡航、地面状态分别降低2.1%、1.2%、2.0%。     

B／S模式下ASP编程的数据传输及接口

论述了B／S模式下ASP编程中数据传输问题的重要性，分析了基本数据传输的工作原理及ASP接口在编程中的作用，结合本人参与的“比一比”网站（www.cwm168.com)建设实例，说明对数据传输问题的研究有助于更好地发挥ASP技术在Web应用中的作用。     

1773光纤数据总线技术与应用研究

讨论了4种光调制技术,利用其中的一种最优方法设计了基于1553B/1773总线的网关电路,并组成含4个站点的无源星型网络拓扑结构的1773总线多路数据传输网进行试验验证。试验结果表明,以光纤替代屏蔽双绞线作为传输介质的1773光纤数据总线能够使1553B总线系统具有更强的性能和更高的可靠性。     

航天器总线管理系统的SOC设计与研究

高速、高可靠、低功耗的智能型串行系统总线是航天器进一步发展必须解决的一个关键问题。以1553B总线控制器为例,采用SOC设计方法,研究了航天器系统总线的设计和实现。首先按照1553B总线标准设计了总线管理SOC的系统结构,然后重点解决了SOC设计中的IP开发应用、可靠性设计、容错机制及低功耗实现等关键技术。采用这些SOC设计方法的1553B总线协议处理器取得了一次流片成功,为今后更高速率的航天器总线管理系统的SOC研究提供了一种思路和方法上的借鉴。     

电机控制系统的软件设计与解决方案

为防止电机输出轴因意外信号或者人为过失导致电机输出轴偏离预想位置,提出一种基于1553B总线数据传输的电机控制系统解决方案.本系统包括测试仪模块、控制盒、被控电机及位置传感器等.主要实现电机1输出轴锁紧、解锁及采集电机2电压反馈功能.