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31.
32.
In this review we present the current status of line-profile-variation studies of β Cep stars. Such studies have been performed
for 26 bright members of this class of pulsating stars in the past 25 years. We describe all these currently available data
and summarize the interpretations based on them in terms of the excited pulsation modes.
We emphasize that line-profile variations offer a much more detailed picture of the pulsational behaviour of pulsating stars
compared to ground-based photometric data. The latter, however, remain necessary to unravel the often complex frequency pattern
and to achieve unambiguous mode identification for multiperiodic β Cep stars and also to derive the pulsational properties
of the faint members of the class.
We highlight the statistical properties of the sample of 26 stars for which accurate spectroscopic studies are available and
point out some future prospects.
This revised version was published online in June 2006 with corrections to the Cover Date. 相似文献
33.
利用分布粘帖在矩形机翼上下两面的压电驱动器,探索使用该类结构提高飞行器横滚能力的可能性。通过风洞模型设计、材料性能测试、模型固有特性测试、压电柔度矩阵测试等试验项目,保证了有限元模型的计算精度,最终通过模型的风洞试验验证了利用气动弹性效应,获得了附加升力与横滚力矩的方案。该原理性试验说明利用分布式压电驱动器改善横滚性能是可行的。 相似文献
34.
S. Hayakawa J. Kuijpers J. Kleczek Boris Valnicek L. Kresak H. R. De Ruiter 《Space Science Reviews》1991,57(1-2):189-192
35.
36.
空间站大型伸展机构的运动稳定性分析 总被引:4,自引:0,他引:4
从空间站大型伸展机构的运动特点和系统动力学方程出发,着重分析了该系统的稳定性判据。这一问题又可分为五个方面:姿态-伸展-振动耦合系统的分析方法,复杂大系统的分解集结方法,时滞系统和滞后系统的稳定性问题,Stick-Ship运动对系统对系统稳定性的影响,非线性非定常系数稳定性的一般解。其中还对接触、摩擦、碰撞问题,变拓扑系统,非光滑动力学系统等进行了专门的研究,分析了Lyapunov指数方法在这些特殊系统中的适应性。本文对空间站大型伸展机构的稳定性问题进行了较全面的分析,指出了目前在处理这类复杂大系统时存在的一些难点问题,为其设计和研制工作提出了理论基础。 相似文献
37.
C. De Jager 《Space Science Reviews》1993,66(1-4):7-19
The paper gives a summary of the situation mid-1993 of theory and observations regarding massive stars. I describe: stellar mass loss and its implications, pre-main-sequence evolution, the main sequence, problems of atmospheric instability, Luminous Blue Supergiants, Yellow Hypergiants, Wolf-Rayet stars and supernovae. 相似文献
38.
Th. De Graauw 《Space Science Reviews》1975,17(5):709-719
Conclusion For wavelengths < 50m fast and sensitive detectors are available. For wavelengths > 50m the available detectors are far from ideal. Research and development of far infrared detectors for the mixing purpose are highly recommended. 相似文献
39.
Avdeev S Bidoli V Casolino M De Grandis E Furano G Morselli A Narici L De Pascale MP Picozza P Reali E Sparvoli R Boezio M Carlson P Bonvicini W Vacchi A Zampa N Castellini G Fuglesang C Galper A Khodarovich A Ozerov Y Popov A Vavilov N Mazzenga G Ricci M Sannita WG Spillantini P 《Acta Astronautica》2002,50(8):511-525
The phenomenon of light flashes (LF) in eyes for people in space has been investigated onboard Mir. Data on particles hitting the eye have been collected with the SilEye detectors, and correlated with human observations. It is found that a nucleus in the radiation environment of Mir has roughly a 1% probability to cause an LF, whereas the proton probability is almost three orders of magnitude less. As a function of LET, the LF probability increases above 10 keV/micrometer, reaching about 5% at around 50 keV/micrometer. 相似文献
40.
V Bidoli M Casolino M P De Pascale G Furano A Morselli L Narici P Picozza E Reali R Sparvoli A M Galper A V Ozerov YuVPopov N R Vavilov A P Alexandrov S V Avdeev Y u Baturin Y u Budarin G Padalko V G Shabelnikov G Barbellini W Bonvicini A Vacchi N Zampa S Bartalucci G Mazzenga M Ricci O Adriani P Spillantini M Boezio P Carlson C Fuglesang G Castellini W G Sannita 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2000,25(10):2075-2079
The SilEye experiment aims to study the cause and processes related to the anomalous Light Flashes (LF) perceived by astronauts in orbit and their relation with Cosmic Rays. These observations will be also useful in the study of the long duration manned space flight environment. Two PC-driven silicon detector telescopes have been built and placed aboard Space Station MIR. SilEye-1 was launched in 1995 and provided particles track and LF information; the data gathered indicate a linear dependence of FLF(Hz) ( 4 2) 10(3) 5.3 1.7 10(4) Fpart(Hz) if South Atlantic Anomaly fluxes are not included. Even though higher statistic is required, this is an indication that heavy ion interactions with the eye are the main LF cause. To improve quality and quantity of measurements, a second apparatus, SilEye-2, was placed on MIR in 1997, and started work from August 1998. This instrument provides energetic information, which allows nuclear identification in selected energy ranges; we present preliminary measurements of the radiation field inside MIR performed with SilEye-2 detector in June 1998. 相似文献