两种实时视频压缩算法DSP嵌入式框架方案比较

在DSP上实现中高分辨率的实时视频数据压缩系统,首先要解决的问题就是选择实现高效率的运行系统框架。本文介绍并讨论了两种适用于在TMS320DM642多媒体处理芯片上实现实时视频压缩算法应用的嵌入式软件实现框架,即TI公司推荐的RF5多任务参考框架和单任务框架。实验分析表明,两种框架的效能是相同的,单任务框架更适合于定制DSP压缩算法的实现与调试。     

基于DSP的钢琴调音仪的研制

探讨了以TI公司的TMS320LF2407A数字信号处理器为硬件核心的钢琴调音仪的实现方法,并就钢琴发音及调音的原理、TMS320LF2407A芯片特点及功能、钢琴调音仪硬件的原理、软件编写思想及算法实现等进行了介绍。该钢琴调音仪实现了对钢琴信号的自动AD采集,对数据进行FFT以及滤波处理、频率测量以及频率值的LCD显示等。     

武器用光纤捷联惯导系统温度模型的研究

本文从光纤陀螺仪和加速度计两方面,对武器用光纤陀螺捷联惯导系统温度模型进行研究.论文首先对光纤陀螺仪温度模型构建的一般过程进行研究,并对加速度计及其I/F转换电路板串联系统的物理模型和数学模型进行了分析,最后对组合温度模型进行了实物验证和适应性验证,验证效果良好.     

针对机载环境应用的视频编码器的优化与实现

本文针对机载航空视频记录的特点,介绍了在 TMS320DM6467平台上实现 H.264视频编码器的算法设计与优化方法.在软件整体设计优化的基础上,结合 TMS320DM6467的平台特点,给出了一套结构优化方法,主要包括提高代码并行性及高效利用协处理器 HDVICP 的算法运算子模块.测试结果表明,通过优化,在保证图像质量损失较小的情况下,编码器的编码速率有显著提高     

基于TMS320C5402的温度监测及调节系统

本文详细介绍了一种利用TI公司生产的16位定点DSP芯片TMS320C5402以及数字式温度传感器DS1820实现的温度监测及调节系统的硬件和软件实现方法。该系统以TMS320C5402为核心,配以检测电路、显示电路、报警电路、控制电路,从而实现智能温度监测及控制服务。由于系统硬件开销小,实时处理能力强,因此具有较高的应用价值。     

TMS320C6678 多级程序加载模式的实现

为了对实地、多单元部署的TMS320C6678 产品同时提供独立启动、就地调试、远程加载功能,利用TMS320C6678 片上多种通讯接口和资源,联合片上固化的内置加载核,设计和实现了一种灵活可配置的多级程序加载模式,满足应用需求。     

F1方程式赛车后升力翼的气动特性

以比例为1∶3的F1方程式赛车后升力翼为研究对象,研究了后升力翼攻角变化对F1方程式赛车气动阻力和气动升力的影响规律.在攻角为12°时,气动升力与气动阻力的比值的绝对值达到最大,此攻角就是F1方程式赛车后升力翼的最佳攻角,模型风洞试验验证了这一结论.      

The post sunset equatorial F- region zonal drift variability and its linkage with equatorial spread F onset and duration over Indian longitudes

The seasonal and solar activity variation of the post sunset F- region zonal plasma drift, at the magnetic equatorial region over Indian longitudes is analyzed using the Republic of China Satellite-1 data from January 2000 to April 2004. The post sunset F- region zonal drifts are observed to be higher in the years of high solar activity in comparison with low solar activity, while seasonally the drifts are minimum in summer with much higher values in other seasons. The seasonal and solar activity variations of zonal plasma drift are attributed to the corresponding variations in the neutral winds. The dependences of the F region peak vertical drift on the zonal plasma drift at 18.5 IST (Indian Standard Time) and the time difference of the conjugate points sunset times, are quantitatively analyzed. Further an integrated parameter (incorporating the above mentioned two independent factors), which is able to predict the peak vertical drift and growth rate of Rayleigh Taylor instability is proposed. The other major outcome of the study is the successful prediction of the Equatorial Spread F (ESF) onset time and duration using the new integrated parameter at 18.5 IST. ESF irregularities and associated scintillations adversely affect communication and navigation systems. Hence, the present methodology for the prediction of the characteristics of these nocturnal irregularities becomes relevant.     

Parameterized Regional Ionospheric Model and a comparison of its results with experimental data and IRI representations

We describe a Parameterized Regional Ionospheric Model (PARIM) to calculate the spatial and temporal variations of the ionospheric electron density/plasma frequency over the Brazilian sector. The ionospheric plasma frequency values as calculated from an enhanced Sheffield University Plasmasphere–Ionosphere Model (SUPIM) were used to construct the model. PARIM is a time-independent 3D regional model (altitude, longitude/local time, latitude) used to reproduce SUPIM plasma frequencies for geomagnetic quiet condition, for any day of the year and for low to moderately high solar activity. The procedure to obtain the modeled representation uses finite Fourier series so that all plasma frequency dependencies can be represented by Fourier coefficients. PARIM presents very good results, except for the F region peak height (hmF2) near the geomagnetic equator during times of occurrence of the F₃ layer. The plasma frequency calculated by IRI from E region to bottomside of the F region present latitudinal discontinuities during morning and evening times for both solar minimum and solar maximum conditions. Both the results of PARIM and the IRI for the E region peak density show excellent agreement with the observational values obtained during the conjugate point equatorial experiment (COPEX) campaign. The IRI representations significantly underestimate the foF2 and hmF2 compared to the observational results over the COPEX sites, mainly during the evening–nighttime period.