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191.
The problem of vibration suppression in large flexible space structure (LFSS) is investigated. Based on the structure property of LFSS, an active damping strategy is proposed to effectively attenuate the critical vibrations of the structure subject to modeling uncertainty and external disturbance. Control algorithms are derived with the aim of suppressing both the vibrating magnitude and vibrating rate to an acceptable level. It is shown that the strategy exhibits robust and adaptive properties and is truly model-independent. The novelty of the proposed approach lies in the fact that it is fairly easy to set up the strategy and the overall computation involved is much less than any other strategies available to date. A two-bay truss is used to verify the validity of the proposed approach 相似文献
192.
Gaurang B. Yodh 《Space Science Reviews》1996,75(1-2):199-212
This paper discusses the properties of using the water Cherenkov technique to detect air showers in the few hundred GeV to 100 TeV energy range. The responses of a 6 m2 2 m deep water Cherenkov counter and that of a 6 m2 10cm thick scintillator-lead sandwich counter to air shower electrons and photons is described. The advantages of water Cherenkov detector is outlined. Its application to do VHE gamma ray astronomy is discussed with particular reference to the MILAGRO telescope currently under construction. Milagro, a water-Cherenkov detector to do gamma ray astronomy above 100 Gev, uses an existing pool 60m × 80m by 8m, located in the Jemez mountains near Los Alamos, NM. The threshold of the MILAGRO detector is comparable to atmospheric Cherenkov detectors, however it has several advantages over these optical detectors. MILAGRO can operate 24 hours a day in all weather conditions and it has an open aperture which allows it to view the entire northern sky every day. These capabilities allow for a systematic all-sky survey to be done for the first time at these energies. MILAGRO will measure the Crab spectrum with high significance over a wide energy range, it will detect and measure the spectra from AGN's such as MRK 421 and it will search for short duration bursts from GRBs and possibly evaporating PBHs. 相似文献
193.
194.
《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2005,35(11):1957-1963
The heights of horizontal structures in the OH airglow images were observed with two all-sky imagers at Platteville (40.2N, 104.7W) and Yucca Ridge Field Station (40.7N, 104.9W) in Colorado. The sodium temperature-wind lidar of CSU at Fort Collins (40.6N, 105.1W) observed temperature and wind velocities around 80–105-km altitude, providing time-height variations of atmospheric stability. Simultaneous observations with the imagers and the lidar were successful on two nights: November 18 and 19, 2003. The estimated height from OH airglow images were lower (80–86 km) than those observed in Japan, with significant time variation. Comparison with the temperature and wind observed by the lidar showed that the estimated height is likely to coincide with the height of small N2 (close to 0) values. Ripples (<10-km horizontal scale) were simultaneously observed in the image. 相似文献
195.
196.
由于质量矩导弹是一个具有非线性和模型不确定性的多变量系统,为了进一步提高控制系统的鲁棒性,对三滑块质量矩导弹进行了鲁棒控制系统的研究。以所建立的质量矩导弹数学模型为基础,通过对模型合理的简化,得到一个耦合的非线性动力学系统,考虑到质量矩导弹的鲁棒性要求和三个滑块的协调控制问题,在混合灵敏度控制的基础上,采用H∞控制理论对导弹进行姿态控制系统的研究,仿真结果验证了这种方法的有效性。 相似文献
197.
198.
Aprajita Verma Vassilis Charmandaris Ulrich Klaas Dieter Lutz Martin Haas 《Space Science Reviews》2005,119(1-4):355-407
Some of the most ‘active’ galaxies in the Universe are obscured by large quantities of dust and emit a substantial fraction
of their bolometric luminosity in the infrared. Observations of these infrared luminous galaxies with the Infrared Space Observatory
(ISO) have provided a relatively unabsorbed view to the sources fuelling this active emission. The improved sensitivity, spatial
resolution and spectroscopic capability of ISO over its predecessor Infrared Astronomical Satellite (IRAS) of enabled significant
advances in the understanding of the infrared properties of active galaxies. ISO surveyed a wide range of active galaxies
which, in the context of this review, includes those powered by intense bursts of star formation as well as those containing
a dominant active galactic nucleus (AGN). Mid-infrared imaging resolved for the first time the dust enshrouded nuclei in many
nearby galaxies, while a new era in infrared spectroscopy was opened by probing a wealth of atomic, ionic and molecular lines
as well as broad band features in the mid- and far-infrared. This was particularly useful, since it resulted in the understanding
of the power production, excitation and fuelling mechanisms in the nuclei of active galaxies including the intriguing but
so far elusive ultraluminous infrared galaxies. Detailed studies of various classes of AGN and quasars greatly improved our
understanding of the unification scenario. Far-infrared imaging and photometry revealed the presence of a new very cold dust
component in galaxies and furthered our knowledge of the far-infrared properties of faint starbursts, ULIGs and quasars. We
summarise almost nine years of key results based on ISO data spanning the full range of luminosity and type of active galaxies. 相似文献
199.
Joris A. D. L. Blommaert Jan Cami Ryszard Szczerba Michael J. Barlow 《Space Science Reviews》2005,119(1-4):215-243
A large fraction of ISO observing time was used to study the late stages of stellar evolution. Many molecular and solid state
features, including crystalline silicates and the rotational lines of water vapour, were detected for the first time in the
spectra of (post-)Asymptotic Giant Branch (AGB) stars. Their analysis has greatly improved our knowledge of stellar atmospheres
and circumstellar environments. A surprising number of objects, particularly young planetary nebulae with Wolf-Rayet (WR)
central stars, were found to exhibit emission features in their ISO spectra that are characteristic of both oxygen-rich and
carbon-rich dust species, while far-IR observations of the PDR around NGC 7027 led to the first detections of the rotational
line spectra of CH and CH+.
Based on observations with ISO, an ESA project with instruments funded by ESA Member States (especially the PI countries:
France, Germany, The Netherlands, and the United Kingdom), and with the participation of ISAS and NASA. 相似文献
200.