Interpretation of solar microwave C type burst spectra in terms of magnetic nonhomogeneity

The solar radio spectra of the gyro-synchrotron radiation without absorption from mildly relativistic non-thermal electron have been presented using the model with the spherical symmetric nonhomogeneity. These spectra have the following features: (i) Twists and turns of the spectra, which appear at the joint between the medium and high frequencies, (ii) Flux density drop at the lower frequencies. Even if there are no absorption in the radio sources, flux density drop at the lower frequencies is still present because of magnetic nonhomogeneity. (iii) These theoretical spectra belong to C type. This provides us a new interpretation for the observed solar burst C type spectra. Project supported by the National Natural Science Foundation of China.     

列车感应通信信道的建模分析

首先建立了具有屏蔽导体的多导体传输线和地面上方单传输线的数学模型,在此基础上建立列车感应通信信道的模型,并利用矩量法进行数值分析。     

Y掺杂Al2O3高k栅介质薄膜的制备及性能研究

利用射频反应共溅射方法制备了Y掺杂Al₂O₃电介质薄膜，用掠入射x射线衍射检测了薄膜的结构，用高分辨率扫描电子显微镜(HRSEM)、原子力显微镜(AFM)观察了薄膜断面和表面形貌，用高频C-V和变频C-V及J-V测量了样品的电学特性. 结果表明，Y的掺入使电介质薄膜的介电常数k有了很大提高(8.14—11.8)，并体现出了较好的介电特性. 分析认为：与氧具有较大电负性差的Y离子的加入，增大了薄膜中的金属—氧键(M—O)的强度；同时，Y的加入使Al₂O₃的结构和原子配位发生了改变，从而提高了离子极化对薄膜介电常数的贡献. 退火前后的XRD谱均显示薄膜为非晶态；HRSEM断面和AFM形貌像显示所制备的薄膜非常平整，能够满足器件要求. 关键词： 高k栅介质 掺杂氧化铝 射频反应溅射     

基于软件无线电的船舶通信设备功能的综合

针对当前船舶配备的通信设备种类较多且驾驶舱操作台有限的状况，提出了基于软件无线电的船舶通信设备功能的综合。     

软件无线电及在调制技术中的应用研究

本文简要地介绍了软件无线电的发展和基本概念,详细地叙述了软件无线电的体系结构,讨论了FM调制的数字化实现方法。     

用DS1302实现无线广播的播放定时

在概述DS1302功能的基础上,介绍了DS1302的结构和操作程序,并对利用DS1302解决无线广播播放定时的操作规程进行了论述。     

Millimeter wave radio telescopes: Gain and pointing characteristics

The basic gain and pointing characteristics of millimeter-wave radio telescopes are described in this paper. Formal definitions of relevant telescope parameters are given. Performance limits set by conventional technology are discussed and compared with measurements of existing telescopes. Methods are also suggested for minimizing pointing errors.     

Detection and analysis of radio pulses from extensive air showers

Radio pulses from extensive air showers (EAS) at 30, 44, and 60 MHz frequencies have been studied, using wide band broad-side arrays of half-wave dipole antenna systems. The experimental results support the theoretical prediction that the field strength of radio emission depends on the shower size. An asymmetry has been noticed in the pulse height distributions of radio pulses detected by North-South and East-West directed arrays. These observations are in agreement with the theory that the charge separation mechanism is predominant in generating radio pulses from EAS and radio emission is polarised in the East-West direction. Experimental data are compared with those of earlier workers.     

微量Mg掺杂ZnO薄膜的光致发光光谱和带隙变化机理研究

利用射频磁控溅射(RF-MS)法在450℃玻璃基底上制备了Mg掺杂量分别为0.81at%,2.43at%和4.05at%的ZnO薄膜,对其微观结构、室温光致发光光谱(PL)、光学和电学性质进行了研究.结果发现,微量Mg掺杂ZnO薄膜晶体具有六方纤锌矿结构并保持高结晶质量;掺杂0.81at%和2.43at%Mg的ZnO薄膜室温PL谱中近带边发射(NBE)峰的短波方向出现了高能发射带与NBE峰同时存在;随着Mg掺杂量增加至4.05at%,这个高能发射带逐步将NBE峰掩盖.推测在Mg掺杂ZnO薄膜中,Mg2+替代Zn2+附近核外电子的能量增大并产生了一个高能级.而未被Mg2+替代的Zn2+周围的核外电子能量状态不变,带间能级依然存在,随着Mg掺杂量的增加处于高能级的电子数目逐步增加并占绝对优势.因此,ZnO薄膜随着Mg掺杂量增加薄膜禁带宽度增大,这是由于Mg掺杂后周围电子能量增大与Burstein-Moss效应共同作用的结果.另外,薄膜在可见光区域的平均透射率均大于85%,随着Mg掺杂量的增加,薄膜禁带宽度增大并在3.36—3.52eV内变化;Mg掺杂量为0.81at%,2.43at%和4.05at%时,薄膜电阻率分别为2.2×10-3,3.4×10-3和8.1×10-3Ω.cm.     

认知MIMO系统频谱检测与吞吐量折中

 研究了认知MIMO系统频谱检测与吞吐量折中问题,以最大化SU(Secondary User)吞吐量为目标,求解出最佳的频谱检测时间和最优功率分配方案。仿真结果表明,存在最佳检测时间使SU的吞吐量达到最大,并且通过注水法功率分配,能进一步提高SU的吞吐量。此外,通过仿真比较了能量检测和基于特征值的频谱检测算法对SU吞吐量的影响,结果表明,采用两种算法SU的吞吐量几乎相等,由于基于特征值的频谱检测算法更具有健壮性,因而更适合应用于认知MIMO系统。