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51.
脉冲爆震燃烧室出口燃气能量分布特性 总被引:1,自引:1,他引:0
为了提高脉冲爆震燃烧室出口燃气能量转换效率,采用数值计算方法,研究了带气动阀和爆震增强结构的脉冲爆震燃烧室出口燃气能量分布特性,结果表明:脉冲爆震燃气的膨胀过程先后经历一次膨胀、二次膨胀和过度膨胀3个阶段,单个周期内二次膨胀阶段的时间和能量占比最大;燃烧室出口燃气压力势能、动能、内能和能流密度的分布主要受燃气压力的影响,且变化规律与燃气压力一致;一次膨胀阶段燃气增加的压力势能、动能、内能分别占单个周期的479%、259%、251%;二次膨胀阶段燃气增加的压力势能、动能、内能分别占单个周期的502%、576%、581%。 相似文献
52.
钛合金蜂窝壁板隔热性能试验研究 总被引:2,自引:0,他引:2
针对钛合金蜂窝夹层结构的隔热性能进行试验研究。试验中研究了在300 ℃稳态条件下,蜂窝芯格尺寸、芯格高度和芯格壁厚等参数对隔热性能的影响规律;分析了各几何参数对隔热性能的敏感度;测试了不同温度条件下钛合金蜂窝夹层结构壁板的等效导热系数。试验结果表明:增大蜂窝芯格尺寸和芯格高度,减少芯格壁厚均有利于提高蜂窝壁板的隔热效果;不同几何参量对钛合金蜂窝夹层结构隔热效果的影响敏感程度从大到小依次为:芯体高度、芯格尺寸和芯体壁厚;钛合金蜂窝壁板的等效导热系数随温度的升高而增大,相同温度下钛合金蜂窝壁板的等效导热系数约为钛合金材料的3%~5%。 相似文献
53.
机械振动全息分析及其若干问题 总被引:3,自引:1,他引:2
蔡云良 《南京航空航天大学学报》1988,(3)
本文用球面波多重象全息照相分析物体的机械振动,简要地讨论了球面波多重象全息三维振动分析的基本规律,介绍了用计算机控制的显微光密度计确定由测点振动引起的物光波的相位差技术,用几何光学方法推导了曲面测件图象上测点位置的修正公式,提出了提高全息振动条纹分辨率的方法.本文在15cm长度物体上至少可记录105级能分辨的全息振型条纹. 相似文献
54.
基于改进遗传算法的机器人动态路径规划 总被引:2,自引:1,他引:2
针对基本遗传算法解决移动机器人路径规划的不足,提出了一种改进的遗传算法。首先,采用栅格法对机器人路径规划进行建模。然后,提出一种生成初始种群的方法和精英策略,设计出自适应变异概率,提高了算法的求解质量。同时,在规划过程中,将全局路径规划与局部路径规划相结合,并且根据机器人与动态障碍物碰撞类型的不同,提出了相应的避碰策略。仿真实验表明:该算法优于基本遗传算法,能够有效地指导机器人在动态环境中实现避障,获得无碰最优或次优路径。 相似文献
55.
移相谐振PWM技术的研究 总被引:1,自引:0,他引:1
本文着重讨论在高频应用场合下的移相零电压谐振PWM 技术,分析移相型谐振变换器、谐振腔电路及定频PWM(脉宽调制)技术中的设计规范。 相似文献
56.
Solar sail formation flying on an inclined Earth orbit 总被引:2,自引:0,他引:2
The versatility of solar sail propulsion can be utilized in the exploration of Earth’s magnetotail. An inclined periodic orbit with respect to ecliptic is possible for a solar sail with its orbital plane in synchronous rotation with the sun. Solar sail evolving on such an inclined orbit is free of Earth shadow. Formation flying of a cluster of sails around such an inclined periodic orbit is investigated in this paper. The solution of the first-order approximation to the linear relative motion is used to qualitatively analyze the configurations of relative orbits. Since the relative motion is unstable, active control is necessary to keep a periodic relative motion. A typical LQR method is employed to stabilize the relative motion. The design method is validated by numerical examples. 相似文献
57.
58.
Qile Zhao Jing Guo Zhigang Hu Chuang Shi Jingnan Liu Hua Cai Xianglin Liu 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2011
The GRACE (Gravity Recovery And Climate Experiment) monthly gravity models have been independently produced and published by several research institutions, such as Center for Space Research (CSR), GeoForschungsZentrum (GFZ), Jet Propulsion Laboratory (JPL), Centre National d’Etudes Spatiales (CNES) and Delft Institute of Earth Observation and Space Systems (DEOS). According to their processing standards, above institutions use the traditional variational approach except that the DEOS exploits the acceleration approach. The background force models employed are rather similar. The produced gravity field models generally agree with one another in the spatial pattern. However, there are some discrepancies in the gravity signal amplitude between solutions produced by different institutions. In particular, 10%–30% signal amplitude differences in some river basins can be observed. In this paper, we implemented a variant of the traditional variational approach and computed two sets of monthly gravity field solutions using the data from January 2005 to December 2006. The input data are K-band range-rates (KBRR) and kinematic orbits of GRACE satellites. The main difference in the production of our two types of models is how to deal with nuisance parameters. This type of parameters is necessary to absorb low-frequency errors in the data, which are mainly the aliasing and instrument errors. One way is to remove the nuisance parameters before estimating the geopotential coefficients, called NPARB approach in the paper. The other way is to estimate the nuisance parameters and geopotential coefficients simultaneously, called NPESS approach. These two types of solutions mainly differ in geopotential coefficients from degree 2 to 5. This can be explained by the fact that the nuisance parameters and the gravity field coefficients are highly correlated, particularly at low degrees. We compare these solutions with the official and published ones by means of spectral analysis. It is found that our solutions are, in general, consistent with others in the spatial pattern. The water storage variations of the Amazon, Chari and Ganges river basins have also been computed. The variations computed with the NPARB approach are closer to those produced by JPL and DEOS solutions, while the variations produced with the NPESS approach are in good agreement with those produced by the CSR and GFZ solutions. A simulation study is implemented with considering realistic noise and low-frequency error. The two approaches are used to recover the true model. The NPESS solution appears closer to the true one. Therefore we are inclined to estimate the nuisance parameters simultaneously with the geopential coefficients. 相似文献
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