基于无线通信的城市路灯监控系统

通过多种通信技术和计算机对城市路灯实现集中监控，监督级、监控级与现场控制级形成三级分布式计算机控制系统。监督级与监控级之间通过Intranet／Internet交互；监控级与现场控制级之间采用无线电台、GPRS及SMS等多种通信技术。     

Difficulties in the study of cosmic radio noise absorption at 30 MHz using riometer at low latitude station,Kolhapur (Lat-16.8°N,Long-74.25°E)

A dual dipole antenna has been installed at low latitude station Kolhapur (Geographic 16.8°N, 74.25°E), Maharashtra, India for the study of cosmic radio noise absorption using Solid State Riometer (which operates at 30 MHz) during pre phase of 24th solar maxima. The aim for this type of study over Kolhapur was to know the response of lower (D region) ionosphere over low latitude by cosmic radio noise absorption using riometer technique during quite period as well as sudden ionospheric disturbances (SID). The observations are being taken for 3 years. Two different sites (∼40 km away from each other) were used for the installation of riometer equipment assuming minimum local noise. It is found that solar noise to cosmic radio noise hence resulting in signal saturation. The night time signal is relatively free of interference but sometimes local noise is responsible for spike-like signatures. Hence it is concluded that Kolhapur (a low latitude station) is not suitable for the study of cosmic radio noise absorption on 30 MHz with riometer and dual dipole antenna. Proper choice for operating frequency of riometer and antenna gain is suggested for low latitude use of this technique for ionospheric deviative and nondeviative absorption studies.     

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。     

特大展弦比机翼的特性与设计

大展弦比机翼有明显的升/阻(L/D)优势。但随着机翼展弦比的增大,在机翼结构重量控制条件下,机翼成柔性机翼,飞行中机翼的弹性变形量随速压(1/2ρV2)增大而增大,出现了严重的气动/结构耦合的问题。本文阐述了耦合问题的成因和解决途径,为特大展弦比机翼飞机(长航时无人机)的设计提供参考。     

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。     

无人机气动特性改进及风洞试验研究

为延长某无人机的留空时间，加大航程和提高升限，用适当加大机翼展弦比和加装翼尖小翼的办法对原型机的气动特性进行了改进，以期能使该无人机的升阻比有较大提高。在工程估算的基础上，对改进后的气动特性和几十种翼尖小翼的组合方案进行了风洞试验研究和优化分析，得出了可供该无人机使用的气动特性改进的最佳方案。风洞试验结果表明：和原型机相比，改型机的最大升阻比可提高20．6％。     

Observing the Sun at 20–650 MHz at Thermopylae with Artemis

Fine structure of type IV radio solar bursts with a great variety and complexity often give much information in different ways and enable estimation of various coronal characteristics. In this work, we expose our new method for fine structure revealing and separation of two basic kinds of type IV fine structure, as fibers and pulsations. We also estimate frequency drift of fibers from dynamic spectra, clean from continuous background, with a prototype method using 2-D Fourier transform and we estimate periodicities of fibers as well as pulsations with continuous wavelet transform. Working with the last method we found periodicities close to 3 min umbral oscillations and 5 min global solar oscillations.