High-cadence Hα imaging of solar flares

The Hα observation is a powerful tool to study the high-energy aspect of solar flares. Spiky brightenings of flare kernels at the Hα center reflect the rapid fluctuation in particle acceleration; linear polarization of Hα emission might be evidence of accelerated protons; red-shifts of the Hα line are caused by the chromospheric evaporation. To study the spiky brightenings of flare kernels with high-cadence imaging at the Hα center, a high-speed Hα camera for the Solar Flare Telescope at Mitaka, NAOJ, had been developed and it started the regular observation in 2001 July. However, the polarimetry and the Dopplermetry are also important and they are required to be carried out in parallel with the high-cadence imaging at the Hα center. Then, we upgraded the original high-speed Hα camera to a new Hα camera system for the multi-aspect Hα observations, which performs all of the high-cadence imaging, the linear polarization measurements, and the off-band imaging for velocity measurements. The new system started the observation in 2002 July. In this paper, the multi-aspect Hα imaging system is described and sample Hα images are presented.     

萤火一号探测器有效载荷数据管理器设计

针对萤火一号探测器各有效载荷的需求设计出安全、可靠的载荷数据管理器(PDHU), 实现对其 进行数据采集、处理、存储以及供配电等; PDHU提供操作系统, 便于应用软件的 开发; 针对火星探测的实际情况, 对地通信采用无交错的RS码加卷积码的级连编码方式进行信道编码.      

Preliminary Scientific Results of Chang'E-1 Lunar Orbiter: Based on Payloads Detection Data in the First Phase

Chang'E-1 lunar Orbiter was launched by Long March 3A rocket from Xichang Satel-lite Launch Center at 18:05BT(Beijing Time) Oct.24,2007.It is the first step of its ambitious three-stage moon program,a new milestone in the Chinese space exploration history.The primary science objectives of Chang'E-1 lunar orbiter are to obtain three-Dimension(3D) stereo images of the lunar surface,to analyze the distribution and abundance of elements on the surface,to investigate the thickness of lunar soil,evaluate helium-3 resources and other characteristics,and to detect the space environment around the moon.To achieve the above four mission objectives,eight sets of scientific instruments are chosen as the payloads of the lunar orbiter,including a CCD stereo camera(CCD),a Sagnac-based interferometer spectrometer(ⅡM),a Laser Altimeter(LAM),a Microwave Radiometer(MRM),a Gamma-Ray Spectrometer(GRS),an X-ray spectrometer(XRS),a High-Energy Particle Detector(HPD),and two Solar Wind Ion Detectors(SWID).The detected data of the payloads show that all payloads work well.This paper introduces the status of payloads in the first phase and preliminary scientific results.     

The simulation of lunar gravity field recovery from D-VLBI of Chang’E-1 and SELENE lunar orbiters

The lunar gravity field is a foundation to study the lunar interior structure, and to recover the evolution history of the Moon. It is still an open and key topic for lunar science. For above mentioned reasons, it becomes one of the important scientific objectives of recent lunar missions, such as KAGUYA (SELENE) the Japanese lunar mission and Chang’E-1, the Chinese lunar mission. The Chang’E-1 and the SELENE were successfully launched in 2007. It is estimated that these two missions can fly around the Moon longer than 6 months simultaneously. In these two missions, the Chinese new VLBI (Very Long Baseline Interferometry) network will be applied for precise orbit determination (POD) by using a differential VLBI (D-VLBI) method during the mission period. The same-beam D-VLBI technique will contribute to recover the lunar gravity field together with other conventional observables, i.e. R&RR (Range and Range Rate) and multi-way Doppler. Taking VLBI tracking conditions into consideration and using the GEODYNII/SOVLE software of GSFC/NASA/USA [8 and 10], we simulated the lunar gravity field recovering ability with and without D-VLBI between the Chang’E-1 and SELENE main satellite. The cases of overlapped flying and tracking period of 30 days, 60 days and 90 days have been analyzed, respectively. The results show that D-VLBI tracking between two lunar satellites can improve the gravity field recovery remarkably. The results and methods introduced in this paper will benefit the actual missions.     

环境减灾-1A、1B卫星供配电测试系统设计

描述了环境减灾-1A、1B卫星供配电测试系统的设计与构建方法,系统采用一套设备完成了双星的测试任务,具有集成度、可靠性高等特点。文章首先介绍了HJ-1A、1B双星供配电测试系统的硬件架构,主要包括数字量采集与控制集成化措施,基于星地隔离与卫星安全的内部功能模块设计方法,以及作为自动化测试对测试设备统筹管理的远程控制功能实现方法;其次介绍了控制与采集软件的结构与功能设计,以及软件设计过程中所采取的抗干扰措施;最后提出了供配电测试系统的设计原则,可为后续测试设备的设计提供理论与工程基础。     

Aerodynamic design of three-stage vaneless counter-rotating turbine

An aerodynamic design criterion was discussed for the 1+3/2 counter-rotating turbine by analyzing the velocity triangles. There are 8 key aerodynamic parameters in the criterion, based on the consideration of aerodynamic efficiency and some strength requirements. Then, an aerodynamic design for the 1+3/2 counter-rotating turbine was made according to the criterion, and a three-dimensional simulation was conducted for it. Finally, the conclusions were obtained. The criterion containing 8 key aerodynamic parameters is verified rationally and the efficiency of the turbine reaches 91%. The aerodynamic characteristics of 1+3/2 counter-rotating turbine are mainly decided by the load coefficient, and due to an optimal power distribution coefficient of the low pressure turbine, the efficiency of the low pressure turbine can be best.     

基于遗传算法与神经网络微电阻点焊工艺参数优化

文摘微电阻点焊工艺参数的设置对焊点力学性能有着至关重要的作用,通过正交试验极差分析研究了工艺参数对0.05 mm厚TC1箔材焊点剪切力和剥离力的影响程度。通过赋予剪切力和剥离力相应的权值将双优化目标转化为单一的混合优化目标,结合神经网络与遗传算法,对工艺参数进行了优化,建立了基于BP神经网络的焊点力学性能预测模型。结果表明预测模型的误差小于4%,预测模型具有较高的精度和预测能力,可以准确地预测焊点的力学性能。同时通过gatool工具箱对各项工艺参数进行了优化,获得焊接参数的最优组合:焊接电流800 A、电极压力8.89 N、爬坡时间1.608 ms、焊接时间8 ms,混合优化目标为55.73 N。通过与正交试验优化结果对比,遗传算法寻优可以获得更好的综合力学性能。     

江苏海涂围垦最优决策

根据江苏省海涂资源的特点及开发利用现状，从全局和长远经济效益现值最大的观点出发，对各片海涂的上地利用作了优化和最优开发决策，从而进一步对多片海涂匡围进度进行最优决策。解决了海涂开发与匡围过程中的最优投资分配问题，建立了解决这一问题的通用数学模型。该模型将复杂的决策优化过程化为线性规划与０～１规划相结合的层次体系，通过协调求解。方法简便、实用。     

香港国际机场航空交通量的无偏灰色马尔科夫预测

针对香港国际机场航空交通量的灰色性和随机波动性,本文采用无偏灰色GM(1,1)代替传统灰色GM(1,1)模型,分析了2001—2012年香港机场航空交通量的数据,预测出2013年香港机场的航空交通量,然后用加权马尔科夫模型对预测结果进行优化。利用Matlab计算得后验差检验C值小于0.35,P值为1,拟合精度等级为好,表明动态无偏灰色马尔科夫能消除传统灰色GM(1,1)模型的固有误差,提高预测精度。加权马尔科夫模型对灰色预测结果优化得2013年香港航空交通量在352 241~370 780架次之间。     

基于IRIG106 Chapter 10标准的数据记录系统

IRIG106 chapter 10是一种数据获取与记录标准,用较经济的方法实现多种数据的数字化和有效组合。本文探讨了IRIG106 chapter 10标准、STANAG4575文件系统的关键特征,针对机载数据记录系统的需求,提出了一种基于IRIG106 chapter 10标准的数据记录系统设计架构,对于机载数据记录系统的设计和研究有一定的价值。