摩擦阻尼器的研究进展          下载免费PDF全文

石文龙  张浩波 《地震工程学报》2022,44(1):1-16

摩擦阻尼器是一种运用摩擦阻尼原理耗散由振动输入到结构中能量的减震装置.相比传统的减震(振)阻尼器,摩擦阻尼器具有以下几点优势:工程结构安装的便利性、构造加工组装的简易性、较大的初始刚度及性能方面的稳定性等.整理并总结国内外学者在摩擦阻尼器方面取得的大量研究成果,包括摩擦阻尼器的类型、性能影响因素、试验研究以及国内外摩擦...  相似文献   

Observations of dawn–dusk aligned polar cap aurora during the substorms of January 21, 2005     

A.M. Du  W. Sun  B.T. Tsurutani  R.N. Boroyev  A.V. Moiseyev 《Planetary and Space Science》2011,59(13):1551-1558

A new type of polar cap aurora, dawn–dusk aligned polar cap aurora (DDAPCA), was detected during the exceptionally intense January 21, 2005 substorm (AE_max=3504 nT). The DDAPCA was located at very high latitude (>85° MLAT) in the polar cap region. As the interplanetary magnetic field (IMF) GSM By component rotated from a positive to a negative value, the DDAPCA tilt angle relative to the dawn–dusk direction rotated anticlockwise and reached ∼45°. It is speculated that the DDAPCA arises from the formation of an X-line in the distant (>80R_E) tail due to polar cap magnetic field reconnection under unusually high solar wind compression conditions.  相似文献   

Heating of directly transmitted ions at low Mach number oblique collisionless shocks: A statistical physics formulation     

S.W. Ellacott  W.P. Wilkinson 《Planetary and Space Science》2007,55(15):2251-2256

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吉林台水电站坝址人造地震动研究     

姜慧  杨章  唐丽华  马巍 《内陆地震》2000,14(3):228-233

为满足水库抗震设计的震要,合成了５０年超越概率５％和１００年超越概率２％的基岩加速度时程曲线,考虑到吉林吉台电站所处的特殊地震环境和场地条件,分析其地震危险性认为：５０年超越概率５％的地震动为远震影响;１００年超越概率２％的地震动为近震影响,目前使用的基岩加带度反应谱衰关于关系的来源资料多少丢失一些高频成分,可能低估高频成分的地震动对基岩场地的影响,为此根据大震,远震的特征周期Ｔｇ较大这一规律,把两个概率水平的加速度反应谱的特征周期Ｔｇ都定为０．３ｓ,并增加基岩反应谱高频成分控制,从而把基岩地震加速度反应谱处理成相应的规准谱,在此基础上通过拟合规准谱合成的基岩地震动时程曲线,较好地满足坝址的设防要求。  相似文献   

引潮力对显著地震触发作用与大震关系及在雅江地震预报中的应用   总被引：11，自引：2，他引：9  

陈荣华 《地震》2003,23(1):53-56

大地震的孕育和发生是震源区及其附近地壳应变能的积累和快速释放过程。当地震孕育到后期, 震源区及其附近应变能高度积累, 处于极不稳定的临界状态。因此, 地震短临预报方法必须基于临界状态的特点。临界状态的最重要特点是触发因素将起重要作用。固体潮的引潮力是一种重要的触发因素。笔者改进了过去仅用月亮固体潮引潮力的地方平太阴时方法, 而用月亮与太阳整个固体潮引潮力作为触发因素, 显然这样更为科学和合理。研究表明, 大地震前震源区及其附近发生的几次显著地震易受固体潮引潮力某个方位附近触发。并应用这一现象结合其他地震前兆方法成功预报了2001年2月23日四川雅江6. 0级地震。  相似文献   

Heliospheric magnetic fields, energetic particles, and the solar cycle     

Pter Kirly 《Journal of Astrophysics and Astronomy》2000,21(3-4):431-437

The heliosphere is the region filled with magnetized plasma of mainly solar origin. It extends from the solar corona to well beyond the planets, and is separated from the interstellar medium by the heliopause. The latter is embedded in a complex and still unexplored boundary region. The characteristics of heliospheric plasma, fields, and energetic particles depend on highly variable internal boundary conditions, and also on quasi-stationary external ones. Both galactic cosmic rays and energetic particles of solar and heliospheric origin are subject to intensity variations over individual solar cycles and also from cycle to cycle. Particle propagation is controlled by spatially and temporally varying interplanetary magnetic fields, frozen into the solar wind. An overview is presented of the main heliospheric components and processes, and also of the relevant missions and data sets. Particular attention is given to flux variations over the last few solar cycles, and to extrapolated effects on the terrestrial environment.  相似文献   

A possible explanation for the radio afterglow of GRB 980519: the dense medium effect     

X. Y. Wang  Z. G. Dai  T. Lu 《Monthly notices of the Royal Astronomical Society》2000,317(1):170-174

GRB 980519 is characterized by its rapidly declining optical and X-ray afterglows. Explanations of this behaviour include models invoking a dense medium environment, which makes the shock wave evolve quickly into the subrelativistic phase, a jet-like outflow, and a wind-shaped circumburst medium environment. Recently, Frail et al. found that the latter two cases are consistent with the radio afterglow of this burst. Here, by considering the transrelativistic shock hydrodynamics, we show that the dense medium model can also account for the radio light curve quite well. The potential virtue of the dense medium model for GRB 980519 is that it implies a smaller angular size of the afterglow, which is essential for interpreting the strong modulation of the radio light curve. Optical extinction arising from the dense medium is not important if the prompt optical–UV flash accompanying the γ -ray emission can destroy dust by sublimation out to an appreciable distance. Comparisons with some other radio afterglows are also discussed.  相似文献   

A self-similar solution for spherically symmetric gravitational collapse     

R. N. Antonova  Ya. M. Kazhdan 《Astronomy Letters》2000,26(6):344-355

A model of gas-dynamical flow during gravitational collapse is analyzed mathematically by assuming its spherical symmetry and self-similarity. A shock wave diverging from the center emerges in this model. The physical requirements imposed on the post-shock flow at the center for the specified parameters at infinity unambiguously determine the shock front and the flow behind it.  相似文献   

Sputtering of grains in C-type shocks     

P. W. May  G. Pineau des Forêts  D. R. Flower  D. Field  N. L. Allan  J. A. Purton 《Monthly notices of the Royal Astronomical Society》2000,318(3):809-816

Sputtering yields are reported for the release of Mg, Fe, Si and O under impact of He, C, O, Si and Fe on grain material composed of Mg- and Fe-bearing silicates. The yields were derived using the trim code, which simulates the results of the transport of ions in matter by means of classical Monte Carlo techniques. The energetics of the sputtering process are a key factor in the sputtering calculations, and so detailed determinations have been made of the energy with which atoms are bound to the lattice, using solid-state simulation programs. The probability of ejection of an atom is computed at a given energy, for a number of angles of incidence, and integrated to obtain the mean yield at that energy. These numerical results are then fitted with a simple function of energy for convenience in subsequent applications.
A grid of C-type shock models has been computed, using our new sputtering yields, for pre-shock densities in the range 10⁴ n _H n (H)+2 n (H₂)10⁶ cm⁻³ and shock speeds 20 v _s45 km s⁻¹. Sputtered fractions can be high, exceeding 50 per cent for shock speeds in excess of approximately 40 km s⁻¹. The column densities of Si and SiO were also computed, for comparison with observations.  相似文献   

Erratum: Momentum transfer between ions and neutrals in molecular gas     

D. R. Flower 《Monthly notices of the Royal Astronomical Society》2000,315(2):431-431

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