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排序方式: 共有160条查询结果,搜索用时 15 毫秒
21.
不锈钢管板小群孔加工技术 总被引:1,自引:0,他引:1
分析了不锈钢管板加工的难点,介绍了机床和钻头的选择及优化切削参数,获得较好的技术经济效果. 相似文献
22.
跨声速风洞斜孔壁非线性流动试验 总被引:1,自引:0,他引:1
为分析跨声速风洞斜孔壁近壁区域的流动特性,评估气流偏角-压力系数的非线性关联,在0.6 m跨超声速风洞中开展了基于七孔探针的流动特性测量试验。通过气流偏角和压力系数分布分析了斜孔壁流动的差阻特性,以及马赫数、模型升力对斜孔壁流动的影响,最后基于试验结果发展了计算斜孔壁特性参数的微分法,并与经验方法结果进行对比。结果表明,斜孔壁流动呈现出明显的差阻性和非线性,在负压差范围内,近壁流动仍以出流为主;高亚声速时,空风洞模型区孔壁流动特性趋于实壁;安装模型后,随着升力的增大,升力面对应的孔壁区域流动向入流发展,孔壁流动特性趋于开口边界。 相似文献
23.
Beverley J. Wills Zhaohui Shang 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2004,34(12):2584-2587
The evolution of luminous QSOs is linked to the evolution of massive galaxies. We know this because the relic black-holes found locally have masses dependent on the properties of the host galaxy’s bulge. An important way to explore this evolution would be to measure dependences of black-hole masses and Eddington accretion ratios over a range of redshifts, i.e., with cosmological age. For low redshift QSOs (and their lower luminosity Seyfert galaxy counterparts) it has been possible to infer black-hole masses from the luminosities and velocity dispersions of their host-galaxy bulges. These masses agree with those virial black-hole masses calculated from the Doppler widths of the broad Hβ emission lines. The latter method can then be extended to more distant and luminous QSOs, up to redshifts of 0.6 with ground-based optical observations. We discuss ways to extend these explorations to higher redshifts – up to 3 using the widths of QSOs’ broad UV emission lines, and in principle, and to redshifts near 4 from ground-based infrared observations of rest-frame Hβ at 2.5 μm. We discuss the possibility of investigating the accretion history of the higher redshift QSOs using measures of Eddington accretion ratio – the soft X-ray spectral index and the eigenvectors of Principal Components Analyses of QSOs’ UV emission-line spectra. 相似文献
24.
M. van der Klis 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2006,38(12):2675-2679
Some aspects of the rapid X-ray variability of low magnetic-field neutron stars in low-mass X-ray binaries are briefly summarized. 相似文献
25.
26.
阎鲁滨 《中国空间科学技术》1988,8(2)
本文介绍了一种賦形波束天线用的圆极化馈源。讨论了形成賦形波束的多馈源天线的特殊问题,通过理论及其实验以及它们的相互比较,说明了十字膜片馈源对于解决这类问题的适用性。比较了不同种类馈源对天线覆盖区增益的影响,从而进一步证明了十字膜片馈源的优点。 相似文献
27.
地磁Ap指数滞后太阳周循环分析 总被引:3,自引:0,他引:3
把1932-2006年地磁Ap指数12个月流动均值分解成为(Ap)R和(Ap)I.其中(Ap)R为太阳黑子数R的线性函数,与太阳黑子数R相位相同,可能对应于日冕物质抛射(CME)等地磁控制因素. (Ap)I分量与太阳黑子数R相位相差约180°,该分量可能对应于极冕洞变化(从太阳峰年开始,由日面极区逐渐向赤道延伸).以地磁Ap指数与太阳黑子数R滞后非常严重的第20太阳周为例,证实了(Ap)I分量与极冕洞向赤道延伸循环变化相对应.因此极冕洞循环变化可能是导致地磁扰动指数与太阳周循环相位不一致,出现滞后现象的一个十分重要原因. 相似文献
28.
B.J. Carr J. McDowell H. Sato 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》1984,3(10-12)
We examine whether the IR background reported by Matsumoto (1983) could have been generated by stars or black holes in the pregalactic era, z=10100. 相似文献
29.
Shawqi Al Dallal 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2010
Diffuse Galactic gamma-ray flux resulting from the evaporation of primordial black holes has been the subject of intensive research work during the last few decades. Theoretical work addressing this issue started in the 1970s whereas data started pouring in only in the 1990s. We discuss in this paper a model of the potential contribution to the Galactic gamma-ray flux of primordial black holes in binary systems and extend the argument to include stable gravitational bound states called Holeums. The model has a predictive power and can be tested by looking for gamma-ray excess in the vicinity of violent events occurring in the Galaxy such as supernova explosions. 相似文献
30.
We analyzed UVCS/SOHO data and compared the H I Lyα (121.6 nm) and O VI (103.2 nm, 103.7 nm) emission in the polar and equatorial
coronal holes. We found that the emission lines have similar characteristics in these two types of coronal holes. Both types
show evidence for superradially diverging boundaries. The latitudinal distribution of the O VI line ratio may indicate that
the equatorial coronal hole has O+5 outflow velocities lower than in the polar coronal holes.
This revised version was published online in June 2006 with corrections to the Cover Date. 相似文献