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31.
实验研究采用波长为10.6μm的CO2脉冲激光器,N2,He,CO2等三种纯净气体及上述气体的相互混合气作为推进工质时,通过实验舱内的冲击摆装置对抛物形光船获得的冲量耦合系数Cm进行了测量。实验发现气体工质的获得的冲量耦合系数Cm随气压增高而增大,通常气体工质的分子量越大,冲量耦合系数Cm越大;在低气压条件下,分子量较大的气体所占的比例越高,混合气获得的冲量耦合系数Cm越高;在高气压条件下,混合气体工质获得的冲量耦合系数与混合气体的种类及比例密切相关。 相似文献
32.
33.
以涡轮叶片超级冷却技术为研究背景,用数值计算的方法,模拟了离心力场下装有多孔介质的封闭腔体中的热驱动换热现象。计算结果表明,在封闭腔体中加入大孔隙率多孔介质后确实能起到强化换热的效果,采用的固体介质的导热性越好,封闭腔体中流体的热驱动能力越强,换热效果越好。而且采用导热性比较好的固体介质时,在大孔隙率范围内,随着孔隙率的减少,封闭腔体中流体的热驱动能力和换热均得到增强。 相似文献
34.
绿色夹具--基于气动肌腱与机械增力机构的夹具系统 总被引:2,自引:0,他引:2
目前人们对夹具技术绿色化的研究,明显滞后于对绿色切削以及绿色机床等方面的研究。本文以流体传动夹具工作介质的绿色化为出发点,结合采用新型的气动执行元件进行整合创新。提出将气动肌腱与机械增力机构进行组合,以代替容易产生污染的液压传动夹具。并通过具体创新案例,对基于气动肌腱和机械增力机构的绿色化夹具系统进行了分析。 相似文献
35.
In this paper we review the possible mechanisms for production of non-thermal electrons which are responsible for the observed
non-thermal radiation in clusters of galaxies. Our primary focus is on non-thermal Bremsstrahlung and inverse Compton scattering,
that produce hard X-ray emission. We first give a brief review of acceleration mechanisms and point out that in most astrophysical
situations, and in particular for the intracluster medium, shocks, turbulence and plasma waves play a crucial role. We also
outline how the effects of the turbulence can be accounted for. Using a generic model for turbulence and acceleration, we
then consider two scenarios for production of non-thermal radiation. The first is motivated by the possibility that hard X-ray
emission is due to non-thermal Bremsstrahlung by nonrelativistic particles and attempts to produce non-thermal tails by accelerating
the electrons from the background plasma with an initial Maxwellian distribution. For acceleration rates smaller than the
Coulomb energy loss rate, the effect of energising the plasma is to primarily heat the plasma with little sign of a distinct
non-thermal tail. Such tails are discernible only for acceleration rates comparable or larger than the Coulomb loss rate.
However, these tails are accompanied by significant heating and they are present for a short time of <106 years, which is also the time that the tail will be thermalised. A longer period of acceleration at such rates will result
in a runaway situation with most particles being accelerated to very high energies. These more exact treatments confirm the
difficulty with this model, first pointed out by Petrosian (Astrophys. J. 557:560, 2001). Such non-thermal tails, even if possible, can only explain the hard X-ray but not the radio emission which needs GeV or
higher energy electrons. For these and for production of hard X-rays by the inverse Compton model, we need the second scenario
where there is injection and subsequent acceleration of relativistic electrons. It is shown that a steady state situation,
for example arising from secondary electrons produced from cosmic ray proton scattering by background protons, will most likely
lead to flatter than required electron spectra or it requires a short escape time of the electrons from the cluster. An episodic
injection of relativistic electrons, presumably from galaxies or AGN, and/or episodic generation of turbulence and shocks
by mergers can result in an electron spectrum consistent with observations but for only a short period of less than one billion
years. 相似文献
36.
M. Ishiguro Y. Sarugaku S. Nishihara Y. Nakada S. Nishiura T. Soyano K. Tarusawa T. Mukai S.M. Kwon S. Hasegawa F. Usui M. Ueno 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2009
Cometary dust trails were first observed by IRAS; they are widely known to be the origins of meteoric showers. A new window has been opened for the study of dust trails, using ground-based observations. We succeeded in obtaining direct images of the 22P/Kopff dust trail with the Kiso 1.05-m Schmidt telescope. Following this initial success, we have continued to perform a dust trail survey at Kiso. As a result of this survey, we have detected dust trails along the orbit of six periodic comets, between February 2002 and March 2004. The optical depth of these dust trails are 10−9 to 10−8, which is consistent with IRAS measurements. In this paper, we describe the observations and data reduction procedures, and report the brief result obtained between February 2002 and March 2004. 相似文献
37.
基于航空发动机叶片的全报废数据,建立了发动机叶片报废率威布尔分布模型,并运用中位秩的方法对威布尔模型的参数进行了求解。为验证所建立模型的有效性,运用某航空公司CFM56-7B航空发动机报废率数据对模型进行了验证,取得了较好的效果。所建立的报废率模型能够为航空发动机的送修目标确定、维修工作范围制定等提供理论的支持。 相似文献
38.
阐述了硬质合金材料的电火花线切割加工特点.通过采用限位棒、恒张力装置提高电极丝的空间稳定性,并在前两次切割采用复合工作液最后精修采用煤油作为工作介质对硬质合金YG8进行了多次切割.试验结果表明,多次切割的加工表面粗糙度达到1μm以下;与采用复合工作液精修后的加工表面相比,煤油精修后的加工表面微裂纹和微孔洞均明显减少,获得较好的加工表面质量. 相似文献
39.
基于介质圆柱电磁散射理论和等效介质理论,导出了金属柱微粒-电介质复合材料的等效相对介电常数的表达式。数值结果表明:入射波频率低于某一频率或金属柱掺料的体积分数增大到一定数值时,复合材料的等效相对介电常数实部会变为负数。 相似文献
40.
发动机内的燃气等高温介质随着组分和浓度的变化,会引起折射率在空间上的非均匀分布,从而导致辐射能束沿着曲线传播,其相应的辐射传热过程也更为复杂。为了避免射线追踪方法的复杂计算、提高计算效率,本文提出了配置点谱方法求解二维非均匀介质内辐射传热问题。在求解过程中,角向采用离散坐标法处理,空间采用配置点谱方法处理。通过将三种非均匀介质内辐射传热问题的配置点谱方法结果与文献结果进行对比分析,发现配置点谱方法可以在较少的节点数下,获得准确、有效地计算结果。并且,采用配置点谱方法求解三种算例的计算时间均消耗较少,均在20分钟以内。这将为进一步开展发动机复杂结构内高温燃气辐射快速仿真提供基础。 相似文献