Seismic behavior of steel buildings with out‐of‐plumb          下载免费PDF全文

Ali A. Rad  Gregory A. MacRae  Trevor Z. Yeow  Desmond K. Bull 《地震工程与结构动力学》2015,44(14):2575-2588

A structure that has a permanent offset from a true vertical line is commonly referred to as being ‘out‐of‐plumb’. Out‐of‐plumb may result from construction tolerances or post‐earthquake permanent deformations in steel buildings. This paper quantifies the displacements of buildings with out‐of‐plumb in subsequent seismic events by means of inelastic dynamic time history analysis. Structures considered have different structural heights, force design reduction factors (R), and target inter‐story drifts. It is shown that buildings with greater out of plumb and force design reduction factor have larger normalized peak inter‐story drift ratio and ratio of residual‐to‐peak drift. Also, the ratio of residual‐to‐peak drift was not strongly dependent on structural height or design drift. A design procedure and example provided, based on the results obtained, show how peak and residual inter‐story drift ratio can be estimated. Copyright © 2015 John Wiley & Sons, Ltd.  相似文献   

Mid-Mountain Clouds at Whistler During the Vancouver 2010 Winter Olympics and Paralympics     

Ruping Mo  Paul Joe  George A. Isaac  Ismail Gultepe  Roy Rasmussen  Jason Milbrandt  Ron McTaggart-Cowan  Jocelyn Mailhot  Melinda Brugman  Trevor Smith  Bill Scott 《Pure and Applied Geophysics》2014,171(1-2):157-183

A comprehensive study of mid-mountain clouds and their impacts on the Vancouver 2010 Winter Olympics and Paralympics is presented. Mid-mountain clouds were frequently present on the Whistler alpine venue, as identified in an extensive archive of webcam images over a 45-day period from February 5 to March 21, 2010. These clouds posed serious forecast challenges and had significant impacts on some Olympic and Paralympic alpine skiing competitions. Under fair weather conditions, a diurnal upslope (anabatic) flow can work in concert with a diurnal temperature inversion aloft to produce a localized phenomenon known as “Harvey’s Cloud” at Whistler. Two detailed case studies in this paper suggest that mid-mountain clouds can also develop in the area as a result of a moist valley flow interacting with a downslope flow descending from the mountaintop. A southerly inflow through the Sea-to-Sky corridor can be channeled by the local topography into a westerly upslope flow toward Whistler Mountain, resulting in orographic clouds on the alpine venue. Under favorable circumstances, these clouds are trapped to the mid-mountain zone by the leeward subsidence of an elevated southerly flow. The presence of the downslope subsidence was manifested by a distinguished dry layer observed on the top of the mid-mountain clouds in both cases. It is the subsidence-induced adiabatic warming that imposes a strong buoyant suppression to trap the mid-mountain cloud. On the other hand, the subsidence-induced dry layer has the potential to trigger evaporative instability to periodically breakup the mid-mountain cloud.  相似文献   

A statistically selected Chandra sample of 20 galaxy clusters – II. Gas properties and cool core/non-cool core bimodality     

Alastair J. R. Sanderson  Ewan O'Sullivan  Trevor J. Ponman 《Monthly notices of the Royal Astronomical Society》2009,395(2):764-776

We investigate the thermodynamic and chemical structure of the intracluster medium (ICM) across a statistical sample of 20 galaxy clusters analysed with the Chandra X-ray satellite. In particular, we focus on the scaling properties of the gas density, metallicity and entropy and the comparison between clusters with and without cool cores (CCs). We find marked differences between the two categories except for the gas metallicity, which declines strongly with radius for all clusters  ( Z ∝ r ^−0.31)  , outside  ∼0.02 r ₅₀₀  . The scaling of gas entropy is non-self-similar and we find clear evidence of bimodality in the distribution of logarithmic slopes of the entropy profiles. With only one exception, the steeper sloped entropy profiles are found in CC clusters whereas the flatter slope population are all non-CC clusters. We explore the role of thermal conduction in stabilizing the ICM and conclude that this mechanism alone is sufficient to balance cooling in non-CC clusters. However, CC clusters appear to form a distinct population in which heating from feedback is required in addition to conduction. Under the assumption that non-CC clusters are thermally stabilized by conduction alone, we find the distribution of Spitzer conduction suppression factors, f _c, to be lognormal, with a log (base 10) mean of  −1.50 ± 0.03  (i.e.   f _c= 0.032  ) and log standard deviation  0.39 ± 0.02  .  相似文献   

The anatomy of the NGC 5044 group – II. Stellar populations and star formation histories     

J. Trevor Mendel  Robert N. Proctor  Jesper Rasmussen  Sarah Brough  Duncan A. Forbes 《Monthly notices of the Royal Astronomical Society》2009,396(4):2103-2123

The distribution of galaxy properties in groups and clusters holds important information on galaxy evolution and growth of structure in the Universe. While clusters have received appreciable attention in this regard, the role of groups as fundamental to formation of the present-day galaxy population has remained relatively unaddressed. Here, we present stellar ages, metallicities and α-element abundances derived using Lick indices for 67 spectroscopically confirmed members of the NGC 5044 galaxy group with the aim of shedding light on galaxy evolution in the context of the group environment.
We find that galaxies in the NGC 5044 group show evidence for a strong relationship between stellar mass and metallicity, consistent with their counterparts in both higher and lower mass groups and clusters. Galaxies show no clear trend of age or α-element abundance with mass, but these data form a tight sequence when fitted simultaneously in age, metallicity and stellar mass. In the context of the group environment, our data support the tidal disruption of low-mass galaxies at small group-centric radii, as evident from an apparent lack of galaxies below  ∼10⁹ M_⊙  within ∼100 kpc of the brightest group galaxy. Using a joint analysis of absorption- and emission-line metallicities, we are able to show that the star-forming galaxy population in the NGC 5044 group appears to require gas removal to explain the ∼1.5 dex offset between absorption- and emission-line metallicities observed in some cases. A comparison with other stellar population properties suggests that this gas removal is dominated by galaxy interactions with the hot intragroup medium.  相似文献   

A statistical analysis of the Two-Dimensional XMM–Newton Group Survey: the impact of feedback on group properties     

Ria Johnson  Trevor J. Ponman  Alexis Finoguenov 《Monthly notices of the Royal Astronomical Society》2009,395(3):1287-1308

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Probing the 2D kinematic structure of early-type galaxies out to three effective radii     

Robert N. Proctor  Duncan A. Forbes  Aaron J. Romanowsky  Jean P. Brodie  Jay Strader †  Max Spolaor  J. Trevor Mendel  Lee Spitler 《Monthly notices of the Royal Astronomical Society》2009,398(1):91-108

We detail an innovative new technique for measuring the two-dimensional (2D) velocity moments (rotation velocity, velocity dispersion and Gauss–Hermite coefficients h ₃ and h ₄) of the stellar populations of galaxy haloes using spectra from Keck DEIMOS (Deep Imaging Multi-Object Spectrograph) multi-object spectroscopic observations. The data are used to reconstruct 2D rotation velocity maps.
Here we present data for five nearby early-type galaxies to ∼three effective radii. We provide significant insights into the global kinematic structure of these galaxies, and challenge the accepted morphological classification in several cases. We show that between one and three effective radii the velocity dispersion declines very slowly, if at all, in all five galaxies. For the two galaxies with velocity dispersion profiles available from planetary nebulae data we find very good agreement with our stellar profiles. We find a variety of rotation profiles beyond one effective radius, i.e. rotation speed remaining constant, decreasing and increasing with radius. These results are of particular importance to studies which attempt to classify galaxies by their kinematic structure within one effective radius, such as the recent definition of fast- and slow-rotator classes by the Spectrographic Areal Unit for Research on Optical Nebulae project. Our data suggest that the rotator class may change when larger galactocentric radii are probed. This has important implications for dynamical modelling of early-type galaxies. The data from this study are available on-line.  相似文献   

Effect of Vertical Wind Shear on Concentration Fluctuation Statistics in a Point Source Plume     

Trevor Hilderman  David J. Wilson 《Boundary-Layer Meteorology》2008,129(1):65-97

Measurements of concentration fluctuation intensity, intermittency factor, and integral time scale were made in a water channel for a plume dispersing in a well-developed, rough surface, neutrally stable, boundary layer, and in grid-generated turbulence with no mean velocity shear. The water-channel simulations apply to full-scale atmospheric plumes with very short averaging times, on the order of 1–4 min, because plume meandering was suppressed by the water-channel side walls. High spatial and temporal resolution vertical and crosswind profiles of fluctuations in the plume were obtained using a linescan camera laser-induced dye tracer fluorescence technique. A semi-empirical algebraic mean velocity shear history model was developed to predict these concentration statistics. This shear history concentration fluctuation model requires only a minimal set of parameters to be known: atmospheric stability, surface roughness, vertical velocity profile, and vertical and crosswind plume spreads. The universal shear history parameter used was the mean velocity shear normalized by surface friction velocity, plume travel time, and local mean wind speed. The reference height at which this non-dimensional shear history was calculated was important, because both the source and the receptor positions influence the history of particles passing through the receptor position.  相似文献   

Relocating resource peripheries to the core of economic geography's theorizing: rationale and agenda   总被引：2，自引：0，他引：2  

Roger Hayter  Trevor J Barnes  Michael J Bradshaw† 《Area》2003,35(1):15-23

Theorizing in economic geography has focused on core regions, industrial and non-industrial, old and new. Indeed, contemplation of the idea of globalization has reinforced this quest. This paper disputes this blinkered thinking that peripheralizes resource peripheries, and seeks to re-position and emphasize resource peripheries within economic geography's theoretical agenda, specifically that associated with the new 'institutional' approach. A truly 'global' economic geography cannot afford to ignore resource peripheries. In particular, we argue that characterizing resource peripheries, and making them distinct from cores, is the intersection of four sets of institutional values or dimensions which we summarize in terms of industrialism (economic dimension), environmentalism (environmental dimension), aboriginalism (cultural dimension) and imperialism (geopolitical dimension). This admittedly preliminary framework underlies our hypothesis that resource peripheries around the world have become deeply contested spaces, much more so than those found in cores.  相似文献   

Discarded containers on a kent beach     

Trevor R. Dixon  A.Joy Cooke 《Marine pollution bulletin》1977,8(5):105-109

Winter beach surveys of discarded containers at Sandwich Bay showed a wide range of fabrication materials and contents. These were manufactured world-wide and probably distributed by seaborne disposal from local shipping. Although blow moulded polyethylene bottles containing toilet cleansers were commonly observed, there was no evidence to indicate an accumulation of these items in the marine environment.  相似文献   

Double oil spill disasters hit Caribbean     

Trevor R. Dixon 《Marine pollution bulletin》1979,10(9):246-247

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