QN control method for building vibration caused by periodic excitation acting on intermediate story     

Liping Xing  Eizaburo Tachibana  Yutaka Inoue 《地震工程与结构动力学》2000,29(8):1079-1091

It has been proved in the authors' latest paper that the effective location of active control devices for building vibration caused by periodic excitation acting on intermediate story is the adjacent three floors to the vibration source. However, in terms of the Discrete‐Optimizing control method, the control forces are on‐line calculated step‐by‐step and time‐delay must exist. The degradation of control effect caused by time‐delay can not be avoided. In this paper, QN control method is proposed in order to resolve this practical problem. Since the external excitations which the building structure would experience are supposed to be periodic to some degree, Quasi‐Newton method is applied into the close‐loop Linear–Quadratic optimal control method and the new control method is called the ‘QN control method’. In this new control method, instead of solving the Riccati equation, the feedback gain matrix is determined by optimizing the quadratic performance index of the structure with the Quasi‐Newton method, one of the most commonly used minimization of functions. The new control law can easily be implemented for time‐delay problems, the degradation can be greatly improved with compensated feedback gain matrix. As a result, the QN control method is proved to be an efficient method to determine the feedback gain matrix. Copyright © 2000 John Wiley & Sons, Ltd.  相似文献   

Astro-E Mission and the X-ray survey     

T. Takahashi  H. Inoue  Y. Ogawara 《Astronomische Nachrichten》1998,319(3):159-162

The fifth Japaniese X-ray astronomy satellite, Astro-E, following Hakucho, Tenma, Ginga, and ASCA is scheduled for launch in the year 2000 by the Institute of Space and Astronautical Science (ISAS) with an M-V rocket. The satellite will be put into an approximately circular orbit with an altitude of ∽550 km and an inclination of ∽31°. There will be three experiments on board Astro-E: an X-ray micro-calorimeter array, four X-ray CCDs and a hard X-ray detector. All three experiments combined, Astro-E will become a spectrometer facility covering a wide energy band from 0.5 keV to 600 keV.  相似文献   

The X-ray spectrum and light curve of Supernova 1995N     

D. W. Fox  W. H. G. Lewin  A. Fabian  K. Iwasawa  R. Terlevich  H. U. Zimmermann  B. Aschenbach  K. Weiler  S. Van Dyk  R. Chevalier  R. Rutledge  H. Inoue  S. Uno 《Monthly notices of the Royal Astronomical Society》2000,319(4):1154-1158

We report on multi-epoch X-ray observations of the Type IIn (narrow emission line) Supernova (SN) 1995N with the ROSAT and ASCA satellites. The 1998 January ASCA X-ray spectrum is well fitted by a thermal bremsstrahlung         or power-law         model. The X-ray light curve shows evidence for significant flux evolution between 1996 August and 1998 January: the count rate from the source decreased by 30 per cent between our 1996 August and 1997 August ROSAT observations, and the X-ray luminosity most likely increased by a factor of ∼2 between our 1997 August ROSAT and 1998 January ASCA observations, although evolution of the spectral shape over this interval is not ruled out. The high X-ray luminosity,     places SN 1995N in a small group of Type IIn supernovae with strong circumstellar interaction, and the evolving X-ray luminosity suggests that the circumstellar medium is distributed inhomogeneously.  相似文献   

A substructure shaking table test for reproduction of earthquake responses of high‐rise buildings     

Xiaodong Ji  Kouichi Kajiwara  Takuya Nagae  Ryuta Enokida  Masayoshi Nakashima 《地震工程与结构动力学》2009,38(12):1381-1399

When subjected to long‐period ground motions, high‐rise buildings' upper floors undergo large responses. Furniture and nonstructural components are susceptible to significant damage in such events. This paper proposes a full‐scale substructure shaking table test to reproduce large floor responses of high‐rise buildings. The response at the top floor of a virtual 30‐story building model subjected to a synthesized long‐period ground motion is taken as a target wave for reproduction. Since a shaking table has difficulties in directly reproducing such large responses due to various capacity limitations, a rubber‐and‐mass system is proposed to amplify the table motion. To achieve an accurate reproduction of the floor responses, a control algorithm called the open‐loop inverse dynamics compensation via simulation (IDCS) algorithm is used to generate a special input wave for the shaking table. To implement the IDCS algorithm, the model matching method and the H_∞ method are adopted to construct the controller. A numerical example is presented to illustrate the open‐loop IDCS algorithm and compare the performance of different methods of controller design. A series of full‐scale substructure shaking table tests are conducted in E‐Defense to verify the effectiveness of the proposed method and examine the seismic behavior of furniture. The test results demonstrate that the rubber‐and‐mass system is capable of amplifying the table motion by a factor of about 3.5 for the maximum velocity and displacement, and the substructure shaking table test can reproduce the large floor responses for a few minutes. Copyright © 2009 John Wiley & Sons, Ltd.  相似文献   

Mid-infrared imaging and spectroscopy of the southern HII region RCW 38     

Craig H. Smith  Tyler L. Bourke  Christopher M. Wright  Henrik W. W. Spoon Spoon  David K. Aitken  Garry Robinson  John W. V. Storey  Takuya Fujiyoshi  Patrick F. Roche  Thomas Lehmann 《Monthly notices of the Royal Astronomical Society》1999,303(2):367-379

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Variation of the broad X-ray iron line in MCG–6-30-15 during a flare     

K. Iwasawa    A. C. Fabian    A. J. Young    H. Inoue  C. Matsumoto 《Monthly notices of the Royal Astronomical Society》1999,306(1):L19-L24

We report results on the broad iron emission line of the Seyfert galaxy MCG–6-30-15, obtained from the second long ASCA observation in 1997. The time-averaged profile of the broad line is very similar to that seen with ASCA in 1994, so confirming the detailed model fit then obtained. A bright flare is seen in the light curve, during which the continuum was soft. At that time the emission line peaks around 5 keV and most of its emission is shifted below 6 keV with no component detected at 6.4 keV  (  This can be interpreted as the result of an extraordinarily large gravitational redshift owing to a dominant flare occurring very close to the black hole at a radius of  ≲5  .  相似文献   

Temperature correlations in a compact hyperbolic universe     

Kaiki Taro Inoue  Kenji Tomita  Naoshi Sugiyama 《Monthly notices of the Royal Astronomical Society》2000,314(4):L21-L25

The effect of a non-trivial topology on the temperature correlations of the cosmic microwave background (CMB) in a small compact hyperbolic universe with volume comparable to the cube of the curvature radius is investigated. Because the bulk of large-angle CMB fluctuations are produced at the late epoch in low-Ω₀ models, the effect of a long-wavelength cut-off owing to the periodic structure does not lead to significant suppression of large-angle power as in compact flat models. The angular power spectra are consistent with COBE data for Ω₀0.1.  相似文献   

Advances in computational morphodynamics using the International River Interface Cooperative (iRIC) software     

Yasuyuki Shimizu  Jonathan Nelson  Kattia Arnez Ferrel  Kazutake Asahi  Sanjay Giri  Takuya Inoue  Toshiki Iwasaki  Chang-Lae Jang  Taeun Kang  Ichiro Kimura  Tomoko Kyuka  Jagriti Mishra  Mohamed Nabi  Supapap Patsinghasanee  Satomi Yamaguchi 《地球表面变化过程与地形》2020,45(1):11-37

Results from computational morphodynamics modeling of coupled flow–bed–sediment systems are described for 10 applications as a review of recent advances in the field. Each of these applications is drawn from solvers included in the public-domain International River Interface Cooperative (iRIC) software package. For mesoscale river features such as bars, predictions of alternate and higher mode river bars are shown for flows with equilibrium sediment supply and for a single case of oversupplied sediment. For microscale bed features such as bedforms, computational results are shown for the development and evolution of two-dimensional bedforms using a simple closure-based two-dimensional model, for two- and three-dimensional ripples and dunes using a three-dimensional large-eddy simulation flow model coupled to a physics-based particle transport model, and for the development of bed streaks using a three-dimensional unsteady Reynolds-averaged Navier–Stokes solver with a simple sediment-transport treatment. Finally, macroscale or channel evolution treatments are used to examine the temporal development of meandering channels, a failure model for cantilevered banks, the effect of bank vegetation on channel width, the development of channel networks in tidal systems, and the evolution of bedrock channels. In all examples, computational morphodynamics results from iRIC solvers compare well to observations of natural bed morphology. For each of the three scales investigated here, brief suggestions for future work and potential research directions are offered. © 2019 The Authors Earth Surface Processes and Landforms Published by John Wiley & Sons Ltd  相似文献   

Temperature profiling measurements by sea turtles improve ocean state estimation in the Kuroshio-Oyashio Confluence region     

Miyazawa  Yasumasa  Kuwano-Yoshida  Akira  Doi  Takeshi  Nishikawa  Hatsumi  Narazaki  Tomoko  Fukuoka  Takuya  Sato  Katsufumi 《Ocean Dynamics》2019,69(2):267-282

Ocean Dynamics - We demonstrate that assimilation of water temperature measurements by sea turtles into an operational ocean nowcast/forecast system improves representation of mesoscale eddies and...  相似文献   

The linear stability of the post-Newtonian triangular equilibrium in the three-body problem     

Kei Yamada  Takuya Tsuchiya 《Celestial Mechanics and Dynamical Astronomy》2017,129(4):487-507

Continuing a work initiated in an earlier publication (Yamada et al. in Phys Rev D 91:124016, 2015), we reexamine the linear stability of the triangular solution in the relativistic three-body problem for general masses by the standard linear algebraic analysis. In this paper, we start with the Einstein–Infeld–Hoffmann form of equations of motion for N-body systems in the uniformly rotating frame. As an extension of the previous work, we consider general perturbations to the equilibrium, i.e., we take account of perturbations orthogonal to the orbital plane, as well as perturbations lying on it. It is found that the orthogonal perturbations depend on each other by the first post-Newtonian (1PN) three-body interactions, though these are independent of the lying ones likewise the Newtonian case. We also show that the orthogonal perturbations do not affect the condition of stability. This is because these do not grow with time, but always precess with two frequency modes, namely, the same with the orbital frequency and the slightly different one due to the 1PN effect. The condition of stability, which is identical to that obtained by the previous work (Yamada et al. 2015) and is valid for the general perturbations, is obtained from the lying perturbations.  相似文献