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1.
Steven D. Howe 《Space Policy》2001,17(4):275-283
The potential benefits to humankind of space exploration are tremendous. Space is not only the final frontier but is also the next marketplace. The orbital space above Earth offers tremendous opportunities for both strategic assets and commercial development. The critical obstacle retarding the use of the space around the Earth is the lack of low cost access to orbit. Further out, the next giant leap for mankind will be the human exploration of Mars. Almost certainly within the next 30 years, a human crew will brave the isolation, the radiation, and the lack of gravity to walk on and explore the Red planet. Both of these missions will change the outlook and perspective of every human being on the planet. However, these missions are expensive and extremely difficult. Chemical propulsion has demonstrated an inability to achieve orbit cheaply and is a very high-risk option to accomplish the Mars mission. An alternative solution is to develop a high performance propulsion system. Nuclear propulsion has the potential to be such a system. The question will be whether humanity is willing to take on the challenge. 相似文献
2.
介绍自行研制的VKM—5型立式捏合机的构造及工作原理,详述了该机采用液压传动和气动元件进行位置检测以及气、电、液安全联锁的特点,并说明与卧式捏合机对比试验情况。 相似文献
3.
通过分析对比,详细介绍了南飞公司应用工业工程重新规划和改进钣金车间生产现场的作法,以及所取得的技术经济效果。 相似文献
4.
人体头部受撞击脑损伤界限的研究 总被引:2,自引:0,他引:2
脑损伤的研究,是生物力学研究的重要问题之一,其研究涉及到医学、力学的很多方面。本文将承受撞击的颅脑看成一个整体,同时又考虑其结构和力学性质。采用粘弹性的Kelvin体进行计算分析,比较分析三种不同的判据对实际人脑的损伤的判断的影响。 相似文献
5.
本文介绍了一种非常规的高速轴振动抑制方法,主要是用振源分析技术,通过确诊设备故障原因来分析影响轴振动的主要因素,调节机器的系统刚度,再通过理论计算修订安装参数,制定设备故障处理对策,在涟源钢铁集团有限公司一万氧压机组上的实践取得了相当满意的效果,很有推广价值。 相似文献
6.
F. Capitanio A. Bazzano P. Ubertini G. De Cesare M. Del Santo A. Tarana A. Joinet 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2006,38(12):2816-2819
On March 2003, IBIS, the γ-ray imager on board the INTEGRAL satellite, detected an outburst from a new source, IGR J17464-3213, that turned out to be an HEAO-1 transient, namely H1743-322. The spectral and temporal evolutions of the source were observed by INTEGRAL in different periods. Also RXTE observed the source for the first time on 2003 March 29 during a PCA Galactic bulge scan. The source flux decayed below the RXTE PCA sensitivity limit in November 2003, then in April 2004 it was again detected by INTEGRAL. On July 3, 2004 the source was again detected by RXTE/PCA at a 2–10 keV intensity of 16 mCrab and on July 7, reached 69 mCrab. Recently, a new outburst was observed on August 2005. We briefly summarise here the behaviour of the source observed by INTEGRAL from March 2003 to August 2005. The new outbursts of the source and the analysis of all the data collected (now public) give a global view of the spectral and time behaviour of this X-ray transient. 相似文献
7.
变轨发动机不等量截尾试验可靠度评估 总被引:1,自引:1,他引:0
对于可靠度要求极高和任务时间以小时计的变轨发动机来说,目前广泛采用以铌合金为材料并喷涂以抗高温氧化涂层方案的推力室,这一类发动机在方案试验阶段结束后的研制试验中往往只出现截尾试验的结果。给出了不等量截尾试验结果的可靠度评估方案。 相似文献
8.
9.
Rudy Wijnands 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2006,38(12):2684-2688
I present a short overview of the behavior and properties of the two simultaneous kilohertz quasi-periodic oscillations (kHz QPOs) seen in the accreting millisecond X-ray pulsar SAX J1808.4–3658. I will focus on the behavior of the upper frequency QPO as a function of time and count rate as seen during the 2002 outburst of this source. I will also discuss briefly the correlated behavior of this QPO with QPOs at lower frequencies (several tens of hertz). 相似文献
10.
Mauro Orlandini 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2006,38(12):2742-2746
Broad-band spectra of accreting X-ray binary pulsars can be fitted by a phenomenological model composed of a power law with a high energy rollover above 10 keV, plus a blackbody component with a temperature of few hundred eV. While, at least qualitatively, the hard tail can be explained in terms of (inverse) Compton scattering, the origin of the soft component cannot find a unique explanation. Recently, a qualitative picture able to explain the overall broad-band spectrum of luminous X-ray pulsars was carried out by taking into account the effect of bulk Comptonization in the accretion column. After a review of these recent theoretical developments, I will present a case study of how different modeling of the continuum affect broad features, in particular the cyclotron resonance features in Vela X-1. 相似文献