恒压式气体微流量计的设计

恒压式气体微流量计是校准气体微流量的一种装置,校准范围为（１７．１－１＊１０＾－５）Ｐａ．Ｌ／ｓ,不确定度于小于２％,可采用直接测量法和比较测量法对标准漏孔进行校准。文章介绍恒压式气体微流量计的设计方法和结构参数的选择。     

漏率与压力关系的研究

在高压密封系统中,漏率与压力的关系,目前仍然处于探索之中。对不同的刚性物理漏孔进行了不同压力状态下的漏率试验,发现了漏率的函数关系。在试验的基础上,经理论分析,验证了其规律的正确性。同时,发现随着漏孔长度的减少而压力指数变大的规律。     

钉载作用下层板多孔过盈配合分析

本文利用各向异性体平面弹性理论中的复势方法,以Faber级数为工具,导出层板多孔/弹性核过盈配合在钉载作用下的级数解。     

Optimisation of X-ray proportional counters for Scanning Sky Monitor (SSM) on ASTROSAT

The Scanning Sky Monitor (SSM) on ASTROSAT is a position-sensitive gas-filled proportional counter with a wide field of view. The scientific objective of SSM is to scan the sky within few hours to detect and locate transient X-ray sources in the outburst phase. Once detected, this information will be provided for studies in all energy bands. The energy range of operation of SSM is 2–10 keV. The optimisation of the parameters of the proportional counter such as the cell size, the gas mixture and the gas pressure for the SSM are discussed here.     

吸收法处理工业生产中的有机废气

通过对空气污染原因和有关处理方法的比较分析 ,提出采用化学吸收法处理高温、低密度的烃类污染物是一项经济有效的方法。     

肼推进系统管路工艺孔的一种自动焊技术

介绍了氩气保护自动堵孔焊技术及其所用设备、换气焊接系统、焊接电源等。同时给出了试样焊接、模拟实样堵焊试样的检测试验数据。介绍了焊接的质量，试验表明，各项数据全部符合设计要求。实践证明，自动堵孔焊技术是完全可行的，其设备稳定可靠，重复性好。     

Black hole accretion and X-ray spectra of QSOS

Changes in Eddington accretion ratios are thought to result in X-ray spectral index changes in Galactic binary black hole systems. Objects with higher Eddington ratios have softer X-ray spectra. Can we apply this result to much more massive black hole systems such as QSOs? If so, X-ray observations will give us valuable insight into the physics of QSOs. Among QSOs, X-ray spectral index is part of a large set of correlated optical and UV observational properties, especially optical Fe II and [O III] strengths in the Hβ region. To investigate whether this set of correlations is related to Eddington ratio, we use as probes, BALQSOs that have been suggested to be youthful super-accretors. We conducted infrared spectroscopy of the Hβ rest wavelength region for a sample of BALQSOs and compared line measurements with those for high and low redshift non-BAL QSOs. Hβ line widths and bolometric luminosity are used to calculate QSO black hole masses and Eddington ratios. Our results support the hypothesis that optical Fe II and [O III] line strengths are Eddington ratio indicators in QSO central engines. A possible explanation is that strong Fe II and weak [O III] indicate abundant cold gas that could fuel near Eddington accretion.     

The case for massive,evolving winds in black hole X-ray binaries

In the last decade, high-resolution X-ray spectroscopy has revolutionized our understanding of the role of accretion disk winds in black hole X-ray binaries. Here I present a brief review of the state of wind studies in black hole X-ray binaries, focusing on recent arguments that disk winds are not only extremely massive, but also highly variable. I show how new and archival observations at high timing and spectral resolution continue to highlight the intricate links between the inner accretion flow, relativistic jets, and accretion disk winds. Finally, I discuss methods to infer the driving mechanisms of observed disk winds and their implications for connections between mass accretion and ejection processes.     

气浮陀螺空气轴承涡流力矩的有限元分析

气浮陀螺K0项漂移精度的控制一直是陀螺研制中的难点,而空气轴承涡流力矩是影响陀螺K0项漂移精度最主要因素。因此,本文根据气浮陀螺研制中的实际问题,结合机加工中空气轴承出现的误差形式,建立了空气轴承制造误差对涡流力矩影响的数学模型,并采用有限元方法分析了空气轴承制造误差对涡流力矩的影响规律,得出了浮子圆度误差和窄缝装配误差是引起涡流力矩最主要因素,并通过空气轴承结构参数与涡流力矩的灵敏度分析,得到了径向平均间隙和窄缝平均间隙结构参数的最优值。针对上述研究结论,提出了控制陀螺涡流力矩的技术方法,并通过试验验证了本文理论计算结果的正确性。     

鲁棒的结构网格自动化重叠方法

网格技术是目前数值模拟中的关键技术之一。重叠网格是一种放宽拓扑要求、减小网格生成难度的网格技术。本文以结构重叠网格为基础,分别针对挖洞、寻点以及洞面优化方法进行了研究和改进,同时完成物面网格重叠,形成了一套鲁棒的、自动化的网格重叠系统。在挖洞方面,结合“最小洞映射”方法,提出“复合式挖洞”方法,节省内存开销;在寻点方面,通过构建格心虚网格,保证搜索空间的连续性,同时结合“有效搜索”思想,排除部分对寻点无贡献的网格点,进而减少ADT叉树节点;在洞面优化上,改变填补判别法则并引入两类受保护洞内点,确保两层插值边界建立,提高鲁棒性;在物面网格重叠上,利用物面投影法完成坐标修正,实现物面附近网格流动变量的准确传递。为验证本文方法,分别对定常翼身组合体DLR-F6绕流和非定常机翼挂载分离过程进行了数值模拟,计算结果与实验结果吻合良好,表明该结构重叠网格系统对多物体间定常、非定常扰流具有较好的数值模拟能力和较高的模拟精度,具有较高的工程应用价值。