无线电波透视仪输入输出阻抗检测分析理论方法

介绍了本质安全电气设备,首次提出了无线电波透视仪的输入、输出阻抗（电阻、电容、电感）的检测方法。通过理论分析,论证了检测方法的可行性,探讨性提出了实际测量方法。     

流动环境中圆孔水平热射流三维数值模拟

根据计算流体动力学理论,采用Realizable k-ε紊流模型和SIMPLEC算法,考虑浮力作用,利用有限体积法来离散求解流动环境中圆孔水平热射流的流动与传热控制方程,对流动环境中圆孔水平热射流进行了三维数值模拟,比较了不同流速比和不同射流出口温度条件下的流动特性和温度分布特性,得到了热射流轨迹的速度和温度衰减规律,分析了流速比和射流出口温度对热射流轨迹温度分布的影响。     

Noise reduction methods in the analysis of near infrared lunar occultation light curves for high angular resolution measurements

A lunar occultation （LO） technique in the near-infrared （NIR） provides angular resolution down to milliarcseconds for an occulted source, even with ground- based 1 m class telescopes. LO observations are limited to brighter objects because they require a high signal-to-noise ratio （S/N ~40） for proper extraction of angular diameter values. Hence, methods to improve the S/N ratio by reducing noise using Fourier and wavelet transforms have been explored in this study. A sample of 54 NIR LO light curves observed with the IR camera at Mt Abu Observatory has been used. It is seen that both Fourier and wavelet methods have shown an improvement in S/N compared to the original data. However, the application of wavelet transforms causes a slight smoothing of the fringes and results in a higher value for angular diameter. Fourier transforms which reduce discrete noise frequencies do not distort the fringe. The Fourier transform method seems to be effective in improving the S/N, as well as improving the model fit, particularly in the fainter regime of our sample. These methods also provide a better model fit for brighter sources in some cases, though there may not be a significant imorovement in S/N.     

Low‐frequency heliographic observations of the quiet Sun corona

We present new results of heliographic observations of quiet‐Sun radio emission fulfilled by the UTR‐2 radio telescope. The solar corona investigations have been made close to the last solar minimum (Cycle 23) in the late August and early September of 2010 by means of the two‐dimensional heliograph within 16.5–33 MHz. Moreover, the UTR‐2 radio telescope was used also as an 1‐D heliograph for one‐dimensional scanning of the Sun at the beginning of September 2010 as well as in short‐time observational campaigns in April and August of 2012. The average values of integral flux density of the undisturbed Sun continuum emission at different frequencies have been found. Using the data, we have determined the spectral index of quiet‐Sun radio emission in the range 16.5–200 MHz. It is equal to –2.1±0.1. The brightness distribution maps of outer solar corona at frequencies 20.0 MHz and 26.0 MHz have been obtained. The angular sizes of radio Sun were estimated. It is found that the solar corona at these frequencies is stretched‐out along equatorial direction. The coefficient of corona ellipticity varies slightly during above period. Its mean magnitudes are equal to ≈ 0.75 and ≈ 0.73 at 20.0 MHz and 26.0 MHz, respectively. The presented results for continuum emission of solar corona conform with being ones at higher frequencies. (© 2013 WILEY‐VCH Verlag GmbH & Co. KGaA, Weinheim)     

Analyzing the capability of a radio telescope in a bistatic space debris observation system

A bistatic space debris observation system using a radio telescope as the receiving part is introduced. The detection capability of the system at different working frequencies is analyzed based on real instruments. The detection range of targets with a fixed radar cross section and the detection ability of small space debris at a fixed range are discussed. The simulations of this particular observation system at different transmitting powers are also implemented and the detection capability is discussed. The simulated results approximately match the actual experiments. The analysis in this paper provides a theoretical basis for developing a space debris observation system that can be built in China.     

地震-电离层扰动探测技术的研究进展

回顾了地震-电离层扰动机理的研究进展和主要的数据观测方法,总结了地震电磁卫星观测电离层扰动的应用发展情况以及基于卫星测量数据对异常辐射源定位的研究进展,介绍了无线电探测方法的实验情况和数据分析方法,为未来中国探测电离层扰动进行短临地震预测工作提出了建议.     

空间GPS无线电掩星反演大气参数方法及其应用

给出了空间无线电掩星反演大气参数的原理及其误差估计方法,介绍了国内外在该领域的研究进展。并针对该技术的一些特点,指出了若干尚需解决的问题。     

载波相位差分技术在馈源舱动态定位中的应用

针对ＦＡＳＴ项目馈源舱扫描跟踪设计,作者根据ＧＰＳ载波相位差分精密动态定位原理,讨论了馈源舱位置和姿态的ＧＰ动态检测系统的组成,按照我国贵州ＫＡＲＳＴ地形的地理位置给出了动态检测时需要使用的馈源舱位姿转换矩阵和求解方程,与ＧＰＳ动态定位系统相结合就可以完成对馈源舱位姿的跟踪检测,实现舱体的闭环控制。     

广州(珠江三角洲)数字遥测地震台网建设回顾

广州（珠江三角洲）数字无线遥测地震台网是我国第一个全套引进的数字无线遥测地震系统的数字地震台网,采用２４位数字地震采集、无线数据传输、地震数据处理等先进技术,对增强广东省特别是珠江三角洲地区的地震监测能力发挥了重要作用,为发展和推动我国数字地震观测技术进行了有益的探索和实践。系统介绍了广州台网的建设过程和技术特色。