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介绍了一种采用FPGA技术实现MPEG-4 ASP级视频DCT量化模块的设计方案。该模块包括二维DCT/IDCT、量化/反量化和帧内直流/交流(DC/AC)预测。用VHDL进行描述并通过模拟试验表明,该模块可在880个时钟周期内处理完一个宏块的数据,工作频率达到40MHZ。文章采用全硬件实现方法,提出了各模块的硬件电路结构设计,减少了电路规模。 相似文献
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采用萃取平衡实验法,研究了用有机溶剂萃取水相中2-氯-4,6-二硝基-1,3-苯二酚的萃取热力学性质。考察了选用乙酸乙酯作萃取剂,苯、甲苯、环己烷和正庚烷作稀释剂时对萃取水相中2-氯-4,6-二硝基-1,3-苯二酚的影响。结果表明,萃合物的结构与稀释剂的种类有关,并且2-氯-4,6-二硝基-1,3-苯二酚在有机相中的分配系数随稀释剂介电常数的增大而增大。通过研究温度对萃取过程的影响,证实了乙酸乙酯从水相中萃取2-氯-4,6-二硝基-1,3-苯二酚的过程是一个放热过程,表观热效应ΔH=-10.088 kJ/mol。 相似文献
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大型复杂航天器结构有限元模型的验证策略研究 总被引:4,自引:0,他引:4
大型复杂航天器结构有限元模型的合理性和准确性在航天器研制过程中具有重要意义, 它是开展星箭耦合分析以及力学环境条件设计等工作的基础。首先综合有限元建模、模 态试验、相关分析和模型修正等技术构造了一套系统的航天器结构有限元模型试验验证策略 ;然后,针对我国新一代大型卫星平台——东方红四号卫星开展了整星有限元模型的试验 验证研究,其中整星模态试验以及模型修正等研究工作属首次在东方红四号卫星平台上成功 实施。修正后有限元模型对整星主模态频率预测误差小于5%,模态置信准则大于0.6,预 示精度达到工程要求。
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The Primordial Helium-4 Abundance from Observations of a Large Sample of Blue Compact Dwarf Galaxies
We use a sample of 45 low-metallicity H II regions in blue compact dwarf (BCD) galaxies to determine the primordial helium abundance YP with a precision better than 5%. We have carefully investigated the physical effects which may make the He I line intensities deviate from their recombination values such as collisional and fluorescent enhancements, underlying He I stellar absorption and absorption by Galactic interstellar Na I. By extrapolating the Y vs. O/H and Y vs. N/H linear regressions to O/H = N/H = 0, we obtain YP = 0.244±0.002 and 0.245±0.001, respectively, higher than previous determinations (YP = 0.230 - 0.234). Part of the difference comes from the fact that previous investigators have not taken into account underlying He I stellar absorption, especially in the NW component of the BCD I Zw 18 which, because of its extremely low metallicity plays a key role in the determination of YP. We derive a slope dY/dZ = 2.3±1.0, considerably smaller than those derived before. With this smaller slope and taking into account the errors, chemical evolution models with an outflow of well-mixed material can be built for star-forming dwarf galaxies which satisfy all the observational constraints. Our YP gives bh
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= 0.058±0.007,f consistent with the lower limit set by dynamical measurements and X-ray observations of clusters of galaxies. It is also consistent, within the framework of standard big bang nucleosynthesis theory, with measurements of primordial 7Li in galactic halo stars and with the D/H abundance measured in absorption systems toward quasars by Burles and Tytler (1997). 相似文献
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The development of a powerful parameter estimation routine and its integration into the simulation environment HOST is described. With this tool approaches are being made towards new strategies of mathematical modeling, aimed at providing highly accurate and nevertheless run-time efficient simulation models. The identification routine is capable of optimizing parameterized models in both dynamic time domain simulation and static (e.g. trim state variation) conditions. Examples of both cases are presented to emphasize the improvement in the system response prediction and to demonstrate the abilities of the identification techniques in combination with the nonlinear simulation platform. This article reviews the activities and achievements accomplished by the DLR Institute of Flight Research and the ONERA Systems Control and Flight Dynamics Department during the last few years in the research on rotorcraft flight dynamics modeling and model identification. Future activities that require extensive high fidelity modeling are in the scope of the current and coming modeling activities that include the use of the presented methods and software technologies. 相似文献