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11.
12.
为探究超高墩三塔斜拉桥在弹性拉索装置下的减震效果,首先利用SAP2000建立了考虑支座非线性和拉索几何非线性的三维有限元模型;其次基于弹性拉索装置,研究了弹性拉索刚度对三塔斜拉桥地震响应的影响;最后基于数值分析结果并结合某三塔斜拉桥实际工程提出3种减震方案。研究表明:在两边塔塔梁结合处设置弹性拉索可显著减小桥梁在地震作用下的内力和位移响应;提出的方案1(两边塔单根弹性索均为50股,单股刚度均为12000kN/m)、方案2(两边塔单根弹性索均为100股,单股刚度均为10000kN/m)和方案3(15#主塔单根弹性拉索100股,单股刚度10000kN/m;17#主塔单根弹性拉索100股,单股刚度为16000kN/m)相较于无弹性索状态,均可有效降低主塔塔底弯矩、塔底剪力、塔顶位移及主梁纵向位移;相较于方案1,方案2和方案3是更优方案。 相似文献
13.
James?G.?WilliamsEmail authorView authors OrcID profile Dale?H.?Boggs 《Celestial Mechanics and Dynamical Astronomy》2016,126(1-3):89-129
Small tidal forces in the Earth–Moon system cause detectable changes in the orbit. Tidal energy dissipation causes secular rates in the lunar mean motion n, semimajor axis a, and eccentricity e. Terrestrial dissipation causes most of the tidal change in n and a, but lunar dissipation decreases eccentricity rate. Terrestrial tidal dissipation also slows the rotation of the Earth and increases obliquity. A tidal acceleration model is used for integration of the lunar orbit. Analysis of lunar laser ranging (LLR) data provides two or three terrestrial and two lunar dissipation parameters. Additional parameters come from geophysical knowledge of terrestrial tides. When those parameters are converted to secular rates for orbit elements, one obtains dn/dt = \(-25.97\pm 0.05 ''/\)cent\(^{2}\), da/dt = 38.30 ± 0.08 mm/year, and di/dt = ?0.5 ± 0.1 \(\upmu \)as/year. Solving for two terrestrial time delays and an extra de/dt from unspecified causes gives \(\sim \) \(3\times 10^{-12}\)/year for the latter; solving for three LLR tidal time delays without the extra de/dt gives a larger phase lag of the N2 tide so that total de/dt = \((1.50 \pm 0.10)\times 10^{-11}\)/year. For total dn/dt, there is \(\le \)1 % difference between geophysical models of average tidal dissipation in oceans and solid Earth and LLR results, and most of that difference comes from diurnal tides. The geophysical model predicts that tidal deceleration of Earth rotation is \(-1316 ''\)/cent\(^{2}\) or 87.5 s/cent\(^{2}\) for UT1-AT, a 2.395 ms/cent increase in the length of day, and an obliquity rate of 9 \(\upmu \)as/year. For evolution during past times of slow recession, the eccentricity rate can be negative. 相似文献
14.
Suman?MajumdarEmail authorView authors OrcID profile Kanan?K.?Datta Raghunath?Ghara Rajesh?Mondal T.?Roy?Choudhury Somnath?Bharadwaj Sk.?Saiyad?Ali Abhirup?Datta 《Journal of Astrophysics and Astronomy》2016,37(4):32
The line-of-sight direction in the redshifted 21-cm signal coming from the cosmic dawn and the epoch of reionization is quite unique in many ways compared to any other cosmological signal. Different unique effects, such as the evolution history of the signal, non-linear peculiar velocities of the matter etc. will imprint their signature along the line-of-sight axis of the observed signal. One of the major goals of the future SKA-LOW radio interferometer is to observe the cosmic dawn and the epoch of reionization through this 21-cm signal. It is thus important to understand how these various effects affect the signal for its actual detection and proper interpretation. For more than one and half decades, various groups in India have been actively trying to understand and quantify the different line-of-sight effects that are present in this signal through analytical models and simulations. In many ways the importance of this sub-field under 21-cm cosmology have been identified, highlighted and pushed forward by the Indian community. In this article, we briefly describe their contribution and implication of these effects in the context of the future surveys of the cosmic dawn and the epoch of reionization that will be conducted by the SKA-LOW. 相似文献
15.
A 1.2 m snow pit was recovered on July 29th, 2009 from the Bogda Glacier, eastern Tianshan (天山). The sample site temperature of -9.6 ℃ indicates that the unique glaciochemical re-cord was well preserved and suitable for the reconstruction of air pollution levels in this previously un-explored region. Samples were analyzed for major ions (Na+, K+, Ca2+, Mg2+, NH4+, Cl-, SO42-, NO3-, HCOO-, and CH3COO-). NO3- and SO42- were characterized by significant high levels of pollution con-centration. Most air masses ... 相似文献
16.
Currently, one of the effective means in monitoring glacier change in regional scale is remote sensing and site-observation method. In this article, we present a study of comparing glacier area in 2005 derived from SPOT5 satellite image with area in 1972 derived from topographic maps. Moreover, Miaoergou (庙儿沟) flat-summit glacier is site observed to verify glacial change in regional scale. During the study period, glaciers located in the southern slope of Kalik (喀尔里克) Mountain re-duced their area by 12.3%. ... 相似文献
17.
Samples were continuously collected from aerosol, fresh snow, and snow pits on Glacier No. 1 at Urumqi River source in eastern Tianshan (天山) Mountains. The deposition processes and the characteristics of mineral dust microparticles from aerosol to fresh snow, and then evolution to the snow pit were determined. Total dust microparticle concentration in the surface snow and aerosol showed a similar temporal variation trend, which was strongly associated with regional and local at-mospheric circulation in the ... 相似文献
18.
为了评价和认识秦南地区有重大勘探突破的陡坡带和该区的勘探潜力,利用该地区天然气组分和碳同位素等分析资料、伴生原油的油源对比以及油气运移模拟,定量刻画与定性评价相结合,对秦南地区天然气成因和油气勘探潜力进行了系统研究.研究表明:凸起带天然气为新近系溶解气且以干气为主,陡坡带天然气为古近系凝析气且为湿气;陡坡带天然气主要为... 相似文献
19.
基于对川北米仓山西部旺苍县鼓城乡唐家河下寒武统仙女洞组露头剖面的观察与镜下分析发现,仙女洞组下段由生物碎屑泥晶灰岩(L)、粉砂质泥岩(M)、似瘤状砾屑灰岩(L')、角砾灰岩(R)、藻凝块灰岩(A)和含生屑钙质砂岩(S)组合而成,其以角砾灰岩、似瘤状砾屑灰岩和藻凝块灰岩为特征,且发育异地岩块和滑塌变形构造。进一步分析认为:L-M岩石组合为正常的斜坡环境低能沉积;L'-R岩石组合中的角砾灰岩为上斜坡生物灰泥丘崩坍滑动至下部而形成的,似瘤状砾屑灰岩可能是由于L-M岩石组合快速沉积导致沉积物失稳滑动变形、上斜坡生物灰泥丘崩落角砾致使的差异压实和滑动、以及后期物质成分差异引起的压溶作用等共同作用的结果,从而使灰质层发生破碎并被泥质包围形成断续的砾屑状,甚至轻微的位移,进而形成条带特征不明显的杂乱变形构造;微生物岩(Mb)组合为上斜坡的灰泥丘沉积;S-M岩石组合为斜坡上部的浊流沉积。根据上述分析结果建立米仓山西部仙女洞组碳酸盐岩台缘斜坡沉积模式,表明仙女洞组沉积早期米仓山西部存在台缘斜坡相沉积。 相似文献
20.
利用有限元软件ABAQUS,结合用户自定义Python程序,开展地震断层作用下深海管道局部变形和压溃过程的数值模拟。分析均质土体和随机分布土体模型的地震断层位移大小对管道局部变形的影响,并分析断层诱发的局部挤压变形对管道压溃压力的影响。研究表明:相比于断层走向与管道轴线方向垂直的走滑断层,断层走向与管道轴线方向夹角为45°的走滑断层作用下管道的压溃压力较小,且当断层走向为管道轴线方向逆时针旋转45°时,左旋走滑断层作用下管道的压溃压力低于右旋走滑断层作用下的管道压溃压力。断层位移相同时,管道径厚比越大,压溃压力越小。考虑土壤随机性时,由于APIX65钢制管道刚性较大,且管道两侧土体内聚力和摩擦角分散于均质土壤土体参数均值两侧,因此断层作用过程中管道受到的土压力在均质土壤模型中的土压力数值处上下波动。 相似文献