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S.A. Bowhill 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》1981,1(11):13-16
During the Middle Atmosphere Program, 1982–1985, balloons will play a central role in gathering stratospheric, chemical, and dynamical data. This paper discusses some of the unique aspects of balloons as tools for probing the middle atmosphere, and suggests some directions for future projects and enhanced capabilities that would improve their utility in future investigations. 相似文献
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R.B. Stoltzfus S.A. Bowhill L.G. Smith 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》1984,4(6):143-146
The Langmuir-probe technique for measurement of electron concentration in the mesosphere is capable of excellent altitude resolution, of order 1 m. Measurements from nine rocket flights frequently show small-scale ionization structures in the altitude region 60–90 km. These are believed to be identical with regions of strong coherent backscatter seem by VHF radars at Jicamarca, Peru and Urbana, Illinois. They are believed to represent intermittent turbulence attributable to nonlinear interaction of waves in the mesosphere. Parameters of the turbulent regions are estimated. 相似文献
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瑞士威力铭-马科黛尔公司 《航空制造技术》2008,(13)
瑞士加工中心制造商威力铭-马科黛尔公司着重于质量和生产效率,主要活跃于航空/航天、精密机械、钟表和医疗行业,并以其为用户提供的高性能交钥匙解决方案而著称. 相似文献
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J.W. Parker S.A. Bowhill 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》1984,4(4):171-174
Observations of solar-flare ionization in the mesosphere can be made using coherent-scatter radar systems. The scattered power profiles they measure in the 60–90 km altitude region is a function of the ion concentration gradient and the intensity of turbulent mixing at each atltitude. By comparing the power profiles before, during and after a solar flare, it is possible to estimate the ion production rate during the flare as a function of altitude and time. This analysis is used to compare the ion production rates with generally accepted ion-chemical models. Comparisons are made with ion production rates estimated from the solar X-ray flux for the same flare made by geostationary satellites. 相似文献
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采用基于密度泛函理论(DFT)的第一性原理计算方法,研究了M2CoA型Heusler合金Mn2CoAl、Mn2CoSi、Ti2CoAl和Ti2CoSi的电子结构和磁学性质。发现Heusler合金Mn2CoAl是亚铁磁性自旋无带隙半导体,Mn2CoSi与Ti2CoAl是亚铁磁性自旋半金属,而Ti2CoSi是铁磁性自旋半金属。它们的总自旋磁矩均为整数,符合Slater-Pauling规则。然后,在分析电子能带结构和态密度的基础上,探讨了自旋无带隙半导体与半金属性的根源。最后,声子谱和弹性常数计算结果表明所有M2CoA型Heusler合金在晶格动力学和力学上均是稳定的。 相似文献
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