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41.
详细分析了发动机瞬变过程中热传递对压气机稳定性的影响机理,建立了热传递对压气机稳定裕度影响的数学模型,并以一台增压比为26的涡扇发动机为例进行计算,结果表明了建立模型的正确性。 相似文献
42.
W型发动机双轴摆动故障的排除 总被引:1,自引:0,他引:1
简要介绍了DPF-2型控制系统在W型发动机上的应用,分析了该系统在使用过程中出现的双轴摆动现象,对整个系统的稳定性进行了探讨,采取措施解决了该发动机双轴摆动故障并进行了试验验证。该研究对进一步完善该型发动机的燃油控制系统有一定的参考作用。 相似文献
43.
A lightning swept stroke model: A valuable tool to investigate the lightning strike to aircraft 总被引:1,自引:0,他引:1
Alain Broc Philippe Lalande Emmanuel Montreuil Jean-Patrick Moreau Alain Delannoy Anders Larsson Pierre Laroche 《Aerospace Science and Technology》2006,10(8):700-708
In the context of lightning strike on the Dassault Falcon family of aircraft, the standard zoning of Falcon 50, 900 and 2000, inferred from FAA and EUROCAE WG31 documents [US Department of Transportation, Federal Aviation Administration, Advisory Circular AC 20-53A, 1985; US Department of Transportation, Federal Aviation Administration, Advisory Circular AC 20-53B, Draft, 1991; EUROCAE WG 31, Aircraft Lightning Zoning Standard, ED-91, 1998], has been presented. Zoning proves to be quite similar between the three types of aircraft. Thanks to the feed-back on lightning strikes to Falcon, lightning traces have been observed on the fuselage for different flight conditions and aircraft. Observations are compared with the zoning performed by Dassault. A physical model, developed by ONERA, was used to simulate the sweeping of lightning on the fuselage of a Falcon 900. The results are in good agreement with the lightning traces observed on the fuselages. 相似文献
44.
杨守环 《中国民航学院学报》1990,(2):19-28
本文在分析现代飞机电源系统所使用的几种过电压保护装置工作原理的基础上,着重对其反延时特性和动作电压进行计算,并就决定和影响过电压保护性能指标的电路参数的调整进行了计算和论述。 相似文献
45.
R. J. Murphy 《Space Science Reviews》2007,130(1-4):127-138
Interactions of ions accelerated in solar flares produce gamma-ray lines and continuum and neutrons. These emissions contain
a rich set of observables that provides information about both the accelerated ions and the environment where the ions are
transported and interact. Ion interactions with the various nuclei present in the ambient medium produce gamma-ray lines at
unique energies. How abundance information is extracted from the measurements is discussed and results from analyses of a
number of solar flares are presented. The analyses indicate that the composition of the ambient gas where the ions interact
(typically at chromospheric densities) is different from that of the photosphere and more like the composition of the corona,
exhibiting low-FIP elemental enhancements that may vary from flare to flare. Evidence for increased Ne/O and the photospheric
3He abundance is also discussed. 相似文献
46.
P. C. Frisch 《Space Science Reviews》2007,130(1-4):355-365
The properties of interstellar matter at the Sun are regulated by our location with respect to a void in the local matter
distribution, known as the Local Bubble. The Local Bubble (LB) is bounded by associations of massive stars and fossil supernovae
that have disrupted dense interstellar matter (ISM), driving low density intermediate velocity ISM into the void. The Sun
appears to be located in one of these flows of low density material. This nearby interstellar matter, dubbed the Local Fluff,
has a bulk velocity of ∼19 km s−1 in the local standard of rest. The flow is coming from the direction of the gas and dust ring formed where the Loop I supernova
remnant merges into the LB. Optical polarization data suggest that the local interstellar magnetic field lines are draped
over the heliosphere. A longstanding discrepancy between the high thermal pressure of plasma filling the LB and low thermal
pressures in the embedded Local Fluff cloudlets is partially mitigated when the ram pressure component parallel to the cloudlet
flow direction is included. 相似文献
47.
T. S. Bastian 《Space Science Reviews》1994,68(1-4):261-274
Radio and X-ray observations of stellar flares provide the most direct probes of energy relaase particle acceleration, and energy transport on stars other than the Sun. In this review, the observational basis for our understanding of the flare phenomenon on other stars is briefly described and outstanding interpretive and theoretical issues are discussed. I shall confine my attention to objects which are solar-like, to the extent that they possess deep convective envelopes and display activity which is presumed to be magnetic in origin. These include pre-main sequence objects, classical flare stars, and close binaries. Future directions are briefly discussed. 相似文献
48.
教练机发动机设计载荷谱推导方法 总被引:1,自引:3,他引:1
系统地研究了教练机航空发动机设计载荷谱的推导方法,主要包括:(1)基准机的选取与现役发动机载荷谱的空测、统计;(2)新机发动机飞行剖面的预测;(3)新机发动机设计任务循环的编制等三大步骤。提出的方法具有一定的通用性,可以推广到其它类型的发动机设计载荷谱研究。 相似文献
49.
C. De Jager 《Space Science Reviews》2005,120(3-4):197-241
50.
Rita M. Sambruna 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2004,34(12):2571-2578
Relativistic jets are a common property of radio-loud Active Galactic Nuclei (AGN). Understanding jet physical properties is an essential precursor to understanding the mechanisms of energy transport, and ultimately, how energy is extracted from the central black hole. In this paper, I highlight recent developments from Chandra and HST observations of kpc-scale jets in AGN, with particular emphasis on our survey of 17 radio jets in a sample of FRII radio galaxies. These observations show that (1) X-ray and optical emission is common from kpc-scale jets, (2) a large fraction of the bolometric luminosity is emitted at X-rays, and (3) in most sources, a candidate emission process for the X-rays is inverse Compton scattering of the Cosmic Microwave Background off the relativistic electrons in the jet. If the latter scenario holds, the implication is that jets are still relativistic on kpc scales. 相似文献