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31.
Mikhail Sachkov Boris Shustov Ana Ines Gómez de Castro 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2014
During last three decades, astronomers have enjoyed continuous access to the 100–300 nm ultraviolet (UV) spectral range where the resonance transitions of the most abundant atoms and ions (at temperatures between 3000 and 300 000 K) reside. This UV range is not accessible from ground-based facilities. The successful International Ultraviolet Explorer (IUE) observatory, the Russian ASTRON mission and successor instruments such as the Galaxy Evolution Explorer (GALEX) mission or the COS and STIS spectrographs on-board the Hubble Space Telescope (HST) prove the major impact of observations in the UV wavelength range in modern astronomy. Future access to space-based observatories is expected to be very limited. For the next decade, the post-HST era, the World Space Observatory – Ultraviolet (WSO–UV) will be the only 2-m class UV telescope with capabilities similar to the HST. WSO–UV will be equipped with instruments for imaging and spectroscopy and it will be a facility dedicated, full-time, to UV astronomy. In this article, we briefly outline the current status of the WSO–UV mission and the science management plan. 相似文献
32.
The relation between the lithium abundance observed in Population II stars and the primordial abundance, is still an open question (see Cayrel and Duncan, this meeting). A few recent results are discussed. HIPPARCOS data show that the standard model of stellar evolution can explain the 6Li detection in HD 84937, suggesting a negligible depletion of 7Li. A slope in the Li/Teff relation for Pop II dwarfs and a spread of their Li abundance have been advocated, and both used as arguments in favor of Li depletion. The slope is not confirmed when two other independent temperature scales are used. The Li scatter around the plateau is hardly larger than the scatter predicted from determination errors. Hints from a scatter of Li in subgiants of the globular cluster M92 are not completely conclusive. The determination of more accurate Li abundances in the Pop II stars is an urgent but difficult task, requiring better model atmosphere (better convection treatment) and the help of observational data about Pop II stars (such as long base interferometry). 相似文献
33.
王飞 《中国民航学院学报》1996,(6):51-58
介绍了用于对微机测控系统输入接口板、输出接口板测试硬件系统的构成,设计了接口卡电路.针对两块电路板,提出了对数字电路板的测试和故障诊断分四个层次,即整板级、功能模块级、单片级和功能输出点级的思想,采取了对功能输出点进行编码的方法建立数字电路板测试的标准知识库,提出了使用功能标志矩阵的方法对各个层次的测试结果进行存储的方法,并根据各个层次测试的关系及相应功能标志矩阵的关系建立了智能化故障诊断程序. 相似文献
34.
35.
LIN Jin-zhao WANG Jin-liang* ZHOU Bo WU Er-xing Department of Physics Beijing University of Aeronautics Astronautics Beijing China 《中国航空学报》2006,19(Z1)
Studies of nanoindentation were performed on nc-Si:H films to evaluate the effects of the fabrication processes on their mechani-cal properties. It is observed that with the decrease of the SiH4 contents, the grain size of the films increases gradually, and as does the crystalline volume fraction. The smaller the grains become, the more homogeneous the films, and the more even the hardness as well as the modulus will be. The hardness and the modulus will increase with the substrate’s temperature rising. The hardness and the modulus of the nc-Si:H films on the Si substrate prove to be higher than those on the glass substrate given the same technology parameters. How-ever, the films on the glass substrate appear to be more homogeneous. 相似文献
36.
T. Van Doorsselaere I. Arregui J. Andries M. Goossens S. Poedts 《Space Science Reviews》2005,121(1-4):79-89
We will discuss the observed, heavily damped transversal oscillations of coronal loops. These oscillations are often modeled
as transversal kink oscillations in a cylinder. Several features are added to the classical cylindrical model. In our models
we include loop curvature, longitudinal density stratification, and highly inhomogeneous radial density profiles.
In this paper, we will first give an overview of recently obtained results, both analytically and numerically. After that,
we shed a light on the computational aspects of the modeling process. In particular, we will focus on the parallellization
of the numerical codes. 相似文献
37.
This paper presents an application of the recent relativistic HLLC approximate Riemann solver by Mignone & Bodo to magnetized
flows with vanishing normal component of the magnetic field. The numerical scheme is validated in two dimensions by investigating
the propagation of axisymmetric jets with toroidal magnetic fields. The selected jet models show that the HLLC solver yields
sharper resolution of contact and shear waves and better convergence properties over the traditional HLL approach. 相似文献
39.
Examination of the spatial distribution of CO intensity of Comet Halley indicates that a large fraction of CO originates from
the refractory organic component in the coma, rather than directly from the volatiles in the nucleus. Based on the fluffy
aggregate interstellar dust comet model, we have estimated the upper limits of the total amount of CO provided by coma dust.
The implications from the comparison of the predicted results with the observed value have been discussed.
This revised version was published online in June 2006 with corrections to the Cover Date. 相似文献
40.
张乐慧 《西安航空技术高等专科学校学报》2002,20(2):60-61,63
本文介绍了图式理论在阅读理解中的作用。实践表明,图式或背景知识在阅读理解中起着极大的作用。因此,在英语阅读中,教师应该把扩展学生的背景知识放在首位,从而可调动学生的阅读积极性,最终提高学生的阅读理解能力。 相似文献