基于VXI总线的某型导弹惯性平台自动测试系统

通过对某型导弹惯性平台测试系统现状的分析，提出基于VXI总线建导弹台自动化测试系统的理想设计方案，并对在IEEE－1394环境下用VXI总线标准组建导弹惯性平台自动化测试系统进行了较详细的论述。试验结果表明，该自动化测试系统具有测试速度快，测试精度高的优点，具有在本领域内推广应用的价值。     

An identification for GEMINGA: A review of all the available data

Dedicated X-ray, optical and radio observations aimed at the identification of the bright γ-ray source 2CG195+04 (GEMINGA) are presented. A very promising candidate is found and its properties are discussed in the context of possible astrophysical scenarios.     

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.     

基于IEEE1394的光纤通道技术

IEEE1394是一种高速串行总线数据传输标准,具有灵活、可扩展性和实时性好等特点,被认为是解决数字图像通信的理想方案之一。光纤通道作为适用于未来航空电子系统的一种高性能的总线技术,具有兼容性好、延迟低、可靠性高、传输速度快和传输距离远等优点,并可为其上层协议提供一种通用的高速率数据传输通道。本文基于IEEE1394的光纤通道的基本特性,提出了一种在光纤通道中进行IEEE1394通信协议映射的基本方案,为实现基于光纤通道的不同航电总线互连提供一种备选方案。     

Orbital corrections by a single-input impulsive control applied along the geomagnetic field

This paper examines the possibility of regular orbital corrections for a satellite controlled by an impulsive force applied along the induction vector of the local geomagnetic field. The main purpose of the correcting considered in the paper is to eliminate the drift in secular variation of the relative orbital parameters over the orbital period. The obtained results are applied to the formation flying problem. The developed method is tested using numerical simulation.     

XMM-Newton observations of the field of γ-ray burst 980425

The error box of GRB980425 has been observed by XMM-Newton in March 2002, with the aim of measuring the late epoch X-ray emission of the supernova 1998bw and of clarifying its supposed association with the GRB itself. We present here the preliminary results obtained with the EPIC PN camera. Our observations confirm the association between SN 1998bw and GRB980425. The EPIC PN measurement of the SN 1998bw flux is significantly below the extrapolation of the power-law temporal trend fitted to the BeppoSAX points and implies a faster temporal decay. We propose different physical interpretations of the SN X-ray light curve, according to whether it is produced by one or more radiation components.     

REM/ROSS: a powerful tool for monitoring the prompt afterglow of γ-ray bursts

Observations of the prompt afterglow of γ-ray burst events are unanimously considered of paramount importance for GRB science and cosmology. Such observations at NIR wavelengths are even more promising allowing the monitoring of high-z Ly- absorbed bursts as well as events occurring in dusty star-forming regions. In these pages we present rapid eye mount (REM), a fully robotized fast slewing telescope equipped with a high throughput NIR (Z, J, H, K) camera dedicated to detecting the prompt IR afterglow. REM can discover objects at extremely high redshift and trigger large telescopes to observe them. The REM telescope will simultaneously feed REM optical slitless spectrograph (ROSS) via a dichroic. ROSS will intensively monitor the prompt optical continuum of GRB afterglows. The synergy between the REM-IR camera and the ROSS spectrograph makes REM a powerful observing tool for any kind of fast transient phenomena. Beside its ambitious scientific goals, REM is also technically challenging since it represent the first attempt to locate a NIR camera on a small telescope providing, with ROSS, unprecedented simultaneous wavelength coverage on a telescope of this size.     

基于S3C44b0X服装绘图仪液晶显示开发

服装绘图仪的控制核心采用SAMSUNG公司S3C44b0X处理器,S3C44b0X为一般应用提供了高性价比和高性能的微控制器解决方案。介绍了将S3C44b0X内置LCD控制器进行重新配置,使其能驱动YXD-12864A液晶显示模块,并给出了该控制器与LCD硬件接口方法,经实验验证此方法的正确性。     

The iron Kα-line diagnostics of the rotating black hole metric in Seyfert galaxies

Observations of Seyfert galaxies in X-ray region reveal the wide emissive lines in their spectra, which can arise in inner parts of accretion disks, where the effects of General Relativity (GR) must be taken into account. A spectrum of a solitary emission line of a hot spot in Kerr accretion disk is simulated depending on the radial coordinate r and the angular momentum a = J/M of a black hole, under the assumption of equatorial circular motion of a hot spot. It is shown that the characteristic two-peak line profile with the sharp edges arises at a large distance (about r ≈ (3–10) r_g). The inner regions emit the line, which is observed with one maximum and extremely wide red wing. We present results of simulations for the isothermal and Shakura–Sunayev disks.     

IEEE-1394b总线等时传输性能分析

IEEE-1394b是一种高速数据总线,已成功应用于航空电子中.其等时传输保证数据传输具有确定的延时,广泛应用于多媒体数据的传输.为解决等时传输中的性能评价问题,基于确定与随机Petri网(DSPN,Determ inistic and Stochastic Petri Net),建立了IEEE-1394b总线等时传输的模型.模型考虑了对等时传输性能影响较大的带宽预留和仲裁机制的影响,精确描述了总线行为.通过对模型的仿真分析,得到了等时传输的吞吐量和平均等待时间等性能指标与节点数量、数据包大小以及数据包到达速率的关系,并得到了IEEE-1394b等时传输总线吞吐量的极限.