H.264变换编码与量化原理分析

详细分析了 H .2 64视频编码标准中的整数变换和量化过程。 H .2 64采用 4× 4整数变换 ,并将尺度调整融合在量化过程中 ,降低变换算法复杂度和减少乘法次数 ,相对于以前的编码标准更加有效     

二氧化锡溅射工艺研究

SnO2 是最早使用也是目前使用最广泛的一种气敏材料 ,使用该材料设计制作的气敏传感器具有许多优点。在简要介绍溅射镀膜的成膜过程和特点的基础上 ,着重介绍了SnO2 膜的制备流程 ,分析了功率和温度变化对成膜质量的影响     

嵌入式操作系统在HDTV机顶盒中的应用

介绍一个高清晰度电视机顶盒方案中软件系统的系统结构，阐述了机顶盒软件中使用的嵌入式操作系统STLite/OS20的原理及其特点，并举例说明了这个嵌入式操作系统在机顶盒系统中的使用。     

经济实用的DSP电源解决方案

笔者介绍了两种低纹波的DSP电源解决方案:一为采用MAX1793和大电流EMI静噪滤波器NFM41P;二为改进的去耦p型滤波电路和大电流EMI静噪滤波器NFM41P。并对方案的特点及其实现进行了详细的解析。试验结果表明:所述方案的纹波小,仅100 mV左右;成本低,仅几十元;适用范围广,通过改变MAX1793芯片的输出电压,可将本方案移植到TI的C5000,C6000系列,且还可用于其他的脱机工作系统。     

声光效应拉曼-内斯方程矩阵级数解法及声光调制器优化设计

提出一种求解正常声光相互作用拉曼 内斯 (Raman Nath)方程的矩阵级数解法 ,该解法直观方便且具有普遍性。计算结果表明 ,对Q =4 1π ,Bragg衍射的效率只有 97 5 % ;对非对称入射 ,以往的Raman Nath近似解误差较大 ;指出提高Bragg衍射效率的有效途径在于提高声光频率比并给出计算声光器件最优长度的计算公式。     

Recording of volume hologram using a beam pattern from taperedoptical fiber

A photorefractive volume hologram was recorded and probed using light diffracted from a tapered optical fiber as a reference beam. A single-mode fiber (SMF) was chemically etched and tapered to give a complicated beam pattern, and it is shown that the tapered optical fiber can be utilized to increase the storage density of the volume hologram. Spatial selectivity of the volume hologram with this method was increased by two times compared to the normal SMF referencing, which is due to the fact that the complicated beam pattern has little correlation with its shifted version     

一种多晶硅高温压力传感器

制作压力传感器时，在二氧化硅层上淀积多晶硅膜，既可利用优良的机械特性，又可保证压敏电阻与衬底间具有良好的绝缘性，由此可大大提高器件的温度特性。介绍了一种多晶硅压力传感器的原理和设计。实验结果表明，这类传感器具有灵敏度好，精度高等特点，电路工作范围为０－２５０℃，且具有良好的温度稳定性。     

a-Si/poly-Si叠层太阳能电池的空间电荷效应和稳定性分析

基于pin结构的a-Si∶H太阳能电池中的空间电荷效应,讨论了a-Si/poly-Si叠层太阳能电池的稳定性.结果表明,在光照射下,光生空穴俘获造成了a-Si∶H中正空间电荷密度的增加,从而改变了电池内部的电场分布,提高了a-Si∶H薄膜中的电场强度.空间电荷效应不会给a-Si/poly-Si叠层结构中的a-Si∶H薄膜带来准中性区(低场"死层"),也没有发生a-Si/poly-Si叠层太阳能电池的光诱导性能衰退,因而a-Si/poly-Si叠层结构太阳能电池具有较高的稳定性.     

The polar ionosphere at Zhongshan station on May 11, 1999, the day the solar wind almost disappeared

The solar wind almost disappeared on May 11, 1999: the solar wind plasma density and dynamic pressure were less than 1cm⁻³ and 0.1 nPa respectively, while the interplanetary magnetic field was northward. The polar ionospheric data observed by the multi-instruments at Zhongshan Station in Antarctica on such special event day was compared with those of the control day (May 14). It was shown that geomagnetic activity was very quiet on May 11 at Zhongshan. The magnetic pulsation, which usually occurred at about magnetic noon, did not appear. The ionosphere was steady and stratified, and the F₂ layer spread very little. The critical frequency of day-side F₂ layer, f₀F₂, was larger than that of control day, and the peak of f₀F₂ appeared 2 hours earlier. The ionospheric drift velocity was less than usual. There were intensive auroral E_s appearing at magnetic noon. All this indicates that the polar ionosphere was extremely quiet and geomagnetic field was much more dipolar on May 11. There were some signatures of auroral substorm before midnight, such as the negative deviation of the geomagnetic H component, accompanied with auroral E_s and weak Pc3 pulsation.

     

Analysis of Aperture Field of Circular Groove Guide Horn Antenna by Using FD-TD Method

This paper presents an instance of using FD-TD method to analyze the aperture field of circular groove guide horn antenna. This process is one part of a hybrid method to solve the radiation field of aperture antenna. To verify the calculated aperture field the radiation pattern is computed from it and compared with the measured one. Good agreement is reached.