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561.
稠密气固两相流颗粒质量流量测量方法研究 总被引:1,自引:0,他引:1
为解决粉末火箭发动机和粉末冲压发动机供粉系统冷流标定过程中颗粒质量流量的测量问题,提出了一种稠密气固两相流中颗粒质量流量的测量方法,并基于旋风分离器和电子天平运用该方法设计了一套气固两相流中固体质量流量的测量装置,同时运用粉末火箭发动机的供粉系统对该测量方法和装置的测试性能进行了实验验证研究。结果表明:测量装置的粉末收集效率可高达98.5%以上,为固体颗粒的质量流量测量提供了保障;测量方法具有较好的可靠性和测量精度,其测量结果相对误差低于3%;测量方法具有较好的测量稳定性,重复性实验中测量结果相对误差低于2%;通过改变旋风分离器结构设计等参数,可拓宽测量方法的适用范围。 相似文献
562.
Alisson Dal Lago Walter D. Gonzalez Aline De Lucas Carlos Roberto Braga Lucas Ramos Vieira Tardelli Ronan Coelho Stekel Marlos Rockenbach 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2013
In this work, we present a study of the coronal mass ejection (CME) dynamics using LASCO coronagraph observations combined with in-situ ACE plasma and magnetic field data, covering a continuous period of time from January 1997 to April 2001, complemented by few extreme events observed in 2001 and 2003. We show, for the first time, that the CME expansion speed correlates very well with the travel time to 1 AU of the interplanetary ejecta (or ICMEs) associated with the CMEs, as well as with their preceding shocks. The events analyzed in this work are a subset of the events studied in Schwenn et al. (2005), from which only the CMEs associated with interplanetary ejecta (ICMEs) were selected. Three models to predict CME travel time to Earth, two proposed by Gopalswamy et al. (2001) and one by Schwenn et al. (2005), were used to characterize the dynamical behavior of this set of events. Extreme events occurred in 2001 and 2003 were used to test the prediction capability of the models regarding CMEs with very high LASCO C3 speeds. 相似文献
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J.-C. Vial F. Auchère J. Chang C. Fang W.Q. Gan K.-L. Klein J.-Y. Prado F. Rouesnel A. Sémery G. Trottet C. Wang 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2008,41(1):183-189
The SMESE (SMall Explorer for Solar Eruptions) mission is a microsatellite proposed by France and China. The payload of SMESE consists of three packages: LYOT (a Lyman α imager and a Lyman α coronagraph), DESIR (an Infra-red Telescope working at 35–80 and 100–250 μm), and HEBS (a High Energy Burst Spectrometer working in X- and gamma-rays). 相似文献
564.
L. Jian C.T. Russell J.G. Luhmann R.M. Skoug 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2008,41(2):259-266
Understanding the evolution of solar wind structures in the inner heliosphere as they approach the Earth is important to space weather prediction. From the in situ solar wind plasma and magnetic field measurements of Pioneer Venus Orbiter (PVO) at 0.72 AU (1979–1988), and of Wind/Advanced Composition Explorer (ACE) missions at 1 AU (1995–2004), we identify and characterize two major solar wind structures, stream interaction regions (SIRs) and interplanetary coronal mass ejections (ICMEs). The average percentage of SIRs occurring with shocks increases significantly from 3% to 24% as they evolve from 0.72 to 1 AU. The average occurrence rate, radial extent, and bulk velocity variation of SIRs do not change from 0.72 to 1 AU, while peak pressure and magnetic field strength both decrease with the radial evolution of SIRs. Within the 0.28 AU distance from the orbit of Venus to that of Earth, the average fraction of ICMEs with shocks increases from 49% to 66%, and the typical radial extent of ICMEs expands by about a fraction of 1.4, with peak pressure and magnetic field strength decreasing significantly. The mean occurrence rate and expansion velocity of ICMEs do not change from 0.72 to 1 AU. 相似文献
565.
In a paper submitted to A&A we present the first line blanketed hydrodynamic models of spherically expanding atmospheres of hot stars. This paper is complementary to the submitted paper. Here, we emphasize the advantages and the weak points of our approach and we present additional technical aspects.The models are characterised by a simultaneous solution of the equation of motion, the non-LTE populations of H and He, and radiation transfer in a line blanketed atmosphere. The entire domain from the optically thick photosphere out to the terminal velocity of the wind is treated. The radiative forces are evaluated consistently with the depth-dependent radiation field, taking into account multiple scattering by metal lines and line overlap. 相似文献
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一种双功能谐振传感器──谐振式质量流量/密度传感器 总被引:1,自引:1,他引:1
详细地讨论了一种双功能谐振式质量流量/密度传感器的测量原理,为我国迅速研制成这种新型的谐振传感器提供了一定的理论依据。 相似文献