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151.
闫吉 《西安航空技术高等专科学校学报》2009,27(4)
"流行书风"的形成与当时书法艺术家主体的完全独立、书法理论界的思想解放、创作主体对创作的个性化与原创性追求,以及以国家级的展览为代表的展厅文化的推波助澜息惠相关.只要其"根植传统、张扬个性"的宗旨不变,在当前乃至今后一个较长的时期,它将一如既往地继续"流行". 相似文献
152.
Thin silver films are deposited by radio frequency magnetron sputtering on glass ceramic at room temperature.Variations of sputtering power,bios voltage and power density are carried out for each deposition,then parts of as-deposited samples are subjected to annealing at 600 ℃ within a vacuum chamber.Structural properties are studied by X-ray diffraction(XRD),scanning electron microscope(SEM)and laser scanning confocal microscope(LSCM).It is shown that structural properties have a strong dependency on sputtering power and annealing temperature.Electrical contact resistance measured by a four point probe instrument is directly affected by the thickness of films.It is also found that the film conductivity,especially in thinner films,is improved by the increasing grain size.Finally,the film adhesion is observed by scratch tests.And the adhesive ability deposited by radio frequency magnetron sputtering shows a better performance than that produced by traditional methods. 相似文献
153.
针对飞行器进入火星大气时气体辐射加热对防热设计带来不确定性,在简述火星探测和气体辐射研究的发展历程的基础上,对火星进入气体辐射加热研究的进展进行综述。首先,针对火星大气环境描述了气体辐射加热的概念和问题由来。其次,重点综述了近年来火星进入气体辐射加热基础模型的数值和试验研究进展,其中包括:热化学非平衡气体动力学、气体辐射特性和辐射传输的计算模型与方法等数值研究;地面测试设备、试验技术和模拟火星大气环境的气体辐射测量与验证等试验研究。再次,综述了流动辐射耦合和后体气体辐射加热等火星进入器设计方面开展的研究。最后,对未来火星进入气体辐射加热研究进行了展望,提出了研究建议。 相似文献
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156.
V. V. Zharkova K. Arzner A. O. Benz P. Browning C. Dauphin A. G. Emslie L. Fletcher E. P. Kontar G. Mann M. Onofri V. Petrosian R. Turkmani N. Vilmer L. Vlahos 《Space Science Reviews》2011,159(1-4):357-420
We review basic theoretical concepts in particle acceleration, with particular emphasis on processes likely to occur in regions of magnetic reconnection. Several new developments are discussed, including detailed studies of reconnection in three-dimensional magnetic field configurations (e.g., current sheets, collapsing traps, separatrix regions) and stochastic acceleration in a turbulent environment. Fluid, test-particle, and particle-in-cell approaches are used and results compared. While these studies show considerable promise in accounting for the various observational manifestations of solar flares, they are limited by a number of factors, mostly relating to available computational power. Not the least of these issues is the need to explicitly incorporate the electrodynamic feedback of the accelerated particles themselves on the environment in which they are accelerated. A brief prognosis for future advancement is offered. 相似文献
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Meteor Phenomena and Bodies 总被引:12,自引:0,他引:12
Zdeněk Ceplecha JiřÍ Borovička W. Graham Elford Douglas O. ReVelle Robert L. Hawkes VladimÍr Porubčan Miloš Šimek 《Space Science Reviews》1998,84(3-4):327-471
Meteoroids can be observed at collision with the Earth's atmosphere as meteors. Different methods of observing meteors are
presented: besides the traditional counts of individual events, exact methods yield also data on the geometry of the atmospheric
trajectory; on the dynamics and ablation of the body in the atmosphere; on radiation; on the spectral distribution of radiation;
on ionization; on accompanying sounds; and also data on orbits. Theoretical models of meteoroid interaction with the atmosphere
are given and applied to observational data. Attention is paid to radar observations; to spectroscopic observations; to experiments
with artificial meteors and to different types of meteor sounds. The proposed composition and structure of meteoroids as well
as their orbits link them to meteorites, asteroids and comets. Meteor streams can be observed as meteor showers and storms.
The rate of influx of meteoroids of different sizes onto Earth is presented and potential hazards discussed.
This revised version was published online in August 2006 with corrections to the Cover Date. 相似文献
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