燃气轮机分布式控制系统设计

阐述了燃气轮机分布式控制系统的技术方案,详细介绍了该系统的硬件电路设计、软件设计和控制模块机箱设计,为配合动力控制系统的发展提供了新的思路。     

汽车尾气分析仪中的大气压力补偿技术

控制汽车尾气量的增加,是减少汽车废气污染改善人类生活环境的重要措施。汽车尾气分析仪主要是通过检测汽车尾气中不同气体的含量,以达到合理控制的目的。在对气体浓度的检测中,大气压力的影响不能忽视。本文围绕这个问题,详细讨论了大气压力影响的补偿方法。     

中原城市群经济发展水平及空间布局研究

中原城市群位于我国东西部的经济缓冲带，尚处于发展的初始阶段。采用多元统计分析方法，通过对选取的13项经济指标进行定量研究，分别得到了中原城市群在河南省的经济发展水平排名与城市群经济发展相似程度分组，从而得到河南省经济发展水平的空间分布表。结果表明：（1）中原城市群在河南省的总体经济发展水平中居于核心地位，但单个城市优势尚不明显，且存在较大差异；（2）中原城市群经济发展相似程度的空间分布有很强的聚集特征；（3）群内城市分别与群外城市在经济发展上呈现有规律的阶梯分布，且城市群在河南省的总体梯度较高；（4）城市群经济发展水平空间布局与地理位置、资源状况、经济基础紧密相关。结合上述实际情况，河南省应当依托中原城市群，把工作重点放在以下三个方面：（1）进一步突出首位城市郑州对周围城市的带动作用，建设以郑州为中心的城市圈；（2）缩小群内城市的经济水平差异和不平衡性，加快经济发展一体化进程；（3）在推进产业一体化的同时，注重发挥各自特色，形成合理的产业布局。     

论BOT项目中的风险分担及风险管理

文章从项目公司的角度出发,将BOT项目中的风险根据项目参与方担负风险的大小划分为三类,并讨论了权益投资者的风险分担问题,认为风险分担和风险管理是项目成功的关键,之后在BOT项目的四个阶段中,就项目的风险管理进行了分析和探讨.     

带肋和双排出流孔通道的流动特性

研究了通道进口雷诺数和总出流比对带肋和双排出流孔通道流量系数和压力分布的影响。实验研究的通道入口雷诺数为3×104~1.5×105,通道总出流比为0.09~0.22。结果表明:通道总出流比较小时,流量系数沿流向减小。通道进口雷诺数增加,流量系数先增加,之后基本不变;通道总出流比较大时,流量系数基本不变;各工况下总压系数沿流向依次经历迅速减小、基本不变、继续减小的过程;沿流向各位置上的总压系数在通道进口雷诺数为6×104~9×104时最小;出流比增大,沿流向各位置上的总压系数随之增大。     

航空制件超声检测中的声场特性分析

 针对航空制件超声检测中影响缺陷定量准确性的声场问题进行了深入讨论, 研究了脉冲波声场的计算方法, 设计了相应的计算软件并绘制出实用换能器声轴线上的声压分布曲线, 分析了不同材料和厚度的采样回波对频谱的影响, 比较了连续波声场和脉冲波声场的分布特性及异同点。研究结果为提高超声检测中缺陷定量的准确性和科学性提供了依据。     

一种模拟喷管二维流场的新方法

采用ＳＩＭＰＬＥ方法对固体火箭发动机喷管进行了纯气相流场的数值模拟。推导了建立在同位网格之上利用协变物理速度分量为计算变量的离散方程，采用协变物理速度分量推导压力修正方程，对密度采用一阶迎风格式插值，将ＳＩＭＰＬＥ方法扩大到计算可压流动。计算结果表明：本方法计算精度高，收敛速度快，程序编写简单。     

Magnetosphere Imaging Instrument (MIMI) on the Cassini Mission to Saturn/Titan

The magnetospheric imaging instrument (MIMI) is a neutral and charged particle detection system on the Cassini orbiter spacecraft designed to perform both global imaging and in-situ measurements to study the overall configuration and dynamics of Saturn’s magnetosphere and its interactions with the solar wind, Saturn’s atmosphere, Titan, and the icy satellites. The processes responsible for Saturn’s aurora will be investigated; a search will be performed for substorms at Saturn; and the origins of magnetospheric hot plasmas will be determined. Further, the Jovian magnetosphere and Io torus will be imaged during Jupiter flyby. The investigative approach is twofold. (1) Perform remote sensing of the magnetospheric energetic (E > 7 keV) ion plasmas by detecting and imaging charge-exchange neutrals, created when magnetospheric ions capture electrons from ambient neutral gas. Such escaping neutrals were detected by the Voyager l spacecraft outside Saturn’s magnetosphere and can be used like photons to form images of the emitting regions, as has been demonstrated at Earth. (2) Determine through in-situ measurements the 3-D particle distribution functions including ion composition and charge states (E > 3 keV/e). The combination of in-situ measurements with global images, together with analysis and interpretation techniques that include direct “forward modeling’’ and deconvolution by tomography, is expected to yield a global assessment of magnetospheric structure and dynamics, including (a) magnetospheric ring currents and hot plasma populations, (b) magnetic field distortions, (c) electric field configuration, (d) particle injection boundaries associated with magnetic storms and substorms, and (e) the connection of the magnetosphere to ionospheric altitudes. Titan and its torus will stand out in energetic neutral images throughout the Cassini orbit, and thus serve as a continuous remote probe of ion flux variations near 20R _S (e.g., magnetopause crossings and substorm plasma injections). The Titan exosphere and its cometary interaction with magnetospheric plasmas will be imaged in detail on each flyby. The three principal sensors of MIMI consists of an ion and neutral camera (INCA), a charge–energy–mass-spectrometer (CHEMS) essentially identical to our instrument flown on the ISTP/Geotail spacecraft, and the low energy magnetospheric measurements system (LEMMS), an advanced design of one of our sensors flown on the Galileo spacecraft. The INCA head is a large geometry factor (G ∼ 2.4 cm² sr) foil time-of-flight (TOF) camera that separately registers the incident direction of either energetic neutral atoms (ENA) or ion species (≥5^∘ full width half maximum) over the range 7 keV/nuc < E < 3 MeV/nuc. CHEMS uses electrostatic deflection, TOF, and energy measurement to determine ion energy, charge state, mass, and 3-D anisotropy in the range 3 ≤ E ≤ 220 keV/e with good (∼0.05 cm² sr) sensitivity. LEMMS is a two-ended telescope that measures ions in the range 0.03 ≤ E ≤ 18 MeV and electrons 0.015 ≤ E≤ 0.884 MeV in the forward direction (G ∼ 0.02 cm² sr), while high energy electrons (0.1–5 MeV) and ions (1.6–160 MeV) are measured from the back direction (G ∼ 0.4 cm² sr). The latter are relevant to inner magnetosphere studies of diffusion processes and satellite microsignatures as well as cosmic ray albedo neutron decay (CRAND). Our analyses of Voyager energetic neutral particle and Lyman-α measurements show that INCA will provide statistically significant global magnetospheric images from a distance of ∼60 R _S every 2–3 h (every ∼10 min from ∼20 R _S). Moreover, during Titan flybys, INCA will provide images of the interaction of the Titan exosphere with the Saturn magnetosphere every 1.5 min. Time resolution for charged particle measurements can be < 0.1 s, which is more than adequate for microsignature studies. Data obtained during Venus-2 flyby and Earth swingby in June and August 1999, respectively, and Jupiter flyby in December 2000 to January 2001 show that the instrument is performing well, has made important and heretofore unobtainable measurements in interplanetary space at Jupiter, and will likely obtain high-quality data throughout each orbit of the Cassini mission at Saturn. Sample data from each of the three sensors during the August 18 Earth swingby are shown, including the first ENA image of part of the ring current obtained by an instrument specifically designed for this purpose. Similarily, measurements in cis-Jovian space include the first detailed charge state determination of Iogenic ions and several ENA images of that planet’s magnetosphere.This revised version was published online in July 2005 with a corrected cover date.     

二维过渡区喷流干扰流场的DSMC/EPS仿真

应用DSMC／EPS混合算法，数值模拟过渡区有RCS横向喷流干扰的二维有限平板高超声速流场，分析了流场结构、分离形态及物面气动系数分布等特性。结果表明，不同：Knudsen数下，喷流干扰流场存在差异，过渡区中的稀薄气体效应得以体现，证明了DSMC／EPS混合算法是研究稀薄，连续混合区域高超声速流动的有效方法。     

大型运输机机翼弯曲载荷计算

简要叙述了飞机平飞时影响机翼弯曲载荷的主要因素；重点介绍了机翼升力、机翼油箱燃油重力、机翼结构重力沿翼展分布数学模型的建立和机翼弯曲载荷计算公式的推导过程；所述方法虽然是针对大型运输机提出的，但对其它类型飞机同样适用。