The beginning of cosmic ray astrophysics

A short history of the beginning of cosmic ray (CR) astrophysics is considered: from the hypothesis on CR origin as a result of Supernova explosions in the Metagalaxy, to a model of solar origin of CR, galactic origin based on the stochastic mechanism of charged particle acceleration in interstellar space, to extragalactic and hierarchical models of CR origin, as well as galactic CR origin taking into account radio-astronomical data. We consider also the first balloon results on the chemical contents of primary CR (especially of the contents Li, Be, B), important for any model of CR origin. Investigations of the injection problem, CR drift and diffusion acceleration by shock waves, and CR generation in Supernova remnants were also important steps in the beginning of CR astrophysics.     

基于随机时隙的RFID读写器防冲突方法

针对密集读写器环境下的无线射频识别(RFID,Radio Frequency Identification)多读写器冲突情况,提出了一种基于随机时隙并通过中央计算机协调的读写器防冲突方法.首先,中央计算机发送每轮起始命令和时隙指令,读写器根据当前利用率随机选择时隙.选择当前时隙的读写器若没有接收到忙信号则发送信标并侦听,若无邻近读写器发送信标则开始读写标签,否则该轮回停止工作.若时隙末存在没有接收到忙信号的读写器则在额外时隙发送二次信标.与现有的分布式防冲突方法相比,该方法具有较好的吞吐量和公平性.     

First millimetric detections of AE Aquarii

We report the first millimetric detections of the magnetic cataclysmic variable AE Aquarii, accompanied by contemporaneous microwave observations. These data show that the time-averaged spectrum is well fit by a power-law which extends to mm wavelengths. We suggest that the spectrum is consistent with that expected from a superposition of flare-like events.     

通信系统电磁兼容性设计

一个设计不好的无线电发射机, 工作时产生的谐波十分严重, 而接收设备又对电磁干扰非常敏感。本文介绍了发射机谐波的抑制方法和接收机抗干扰技术体制, 实现自适应通信, 确保通信质量。     

软件无线电中FSK信号解调的一种快速算法

本文介绍了采用差分检波解调算法实现软件无线电中移频键控信号(FSK)快速解调方祛，并通过数字信号处理技术验证了该解调方祛。     

Imaging diagnostics of solar non-thermal particles

Non-thermal hard X-ray, gamma-ray and radio emission are the most direct signatures of the presence of energetic particles in the solar atmosphere. This paper lays emphasis on hard X-ray and radio imaging data, obtained during and outside flares, which reveal the sites where particles interact with the ambient medium. These observations, which provide more or less direct information on the topology and dynamics of the magnetic structures in which particles are accelerated and propagate, are discussed in the framework of the statistical flare scenario.     

碟形升力体的低速气动特性研究

为改善升力体的低速气动性能,探讨各种措施对升力体低速气动特性的影响,在风洞中对一个碟形低速升力体半模型进行了实验研究.试验结果表明,采用适当的气动设计与附面层控制相结合,可以明显改善升力体的低速气动性能,其最大升阻比达到18.7,与原来相比提高了86%,而且零升阻力降低56%,大迎角气动特性也有一定的改善.实验中还对2种附面层控制方案进行了对比,给出了相应的试验结果,对其控制机理进行了初步的探讨.实验证明该碟形低速升力体气动性能优秀,并且已经成功进行了模型空中试飞.     

射频辉光放电法沉积类金刚石碳膜

研究了碳氢气体通过射频辉光放电沉积类金刚石碳膜。研究了射频电压和沉积时间对膜厚和维氏显微硬度的影响。此外,还进行了微动磨损试验。本实验所用的碳氢气体为C_2H_2,基体材料为TC4钛合金(Ti-6％Al-4％V)和45钢(Fe-0.45％C)。     

利用通信和广播电视卫星定位干扰源的技术

简要介绍了利用通信和广播电视卫星对地面干扰辐射源进行定位的必要性和基本工作原理、技术难点及解决方法,以及提高定位精度的主要技术途径。     

亚角秒分辨率射电观测的数据处理

使用英国多单元联线干涉网(MERLIN), 及美国甚大阵(VLA)对河外射电源进行了多频观测, 获得了亚角秒分辨率的图象. 使用自核准技术及洁化技术, 改善了成图的动态范围. 哈勃空间望远镜(HST), 也对该河外射电源进行了光学观测. 本文介绍了射电图和光学图进行重叠的方法, 用以比较射电发射的等离子体和光学线发射云之间的物理联系.