环境温度对板式橡胶支座摩擦滑移性能的影响分析          下载免费PDF全文

李悦  纪梦为  李冲 《地震工程学报》2021,43(3):672-678

采用有限元模拟的方式,对板式橡胶支座摩擦滑移特性进行分析,并与常温试验中获得的支座摩擦滑移滞回曲线、等效黏滞阻尼比等进行了对比.在获得可靠模型的基础上,分析环境温度对板式橡胶支座摩擦滑移特性的影响,研究了温度与支座摩擦滑移耗能、等效黏滞阻尼比和滑动起始距离的关系.结果表明:(1)板式橡胶支座的有限元模型可以较好地实现支...  相似文献   

Characteristics of Radar Echo Parameters and Microphysical Structure Simulation of a Short-Time Heavy Precipitation Supercell     

赵桂香  王一颉  连志鸾 《热带气象学报(英文版)》2022,28(4):388-404

By using the conventional observations, radar data, NCEP/NCAR FNL 1°×1° reanalysis data and numerical simulation data and with the construction and calculation of radar echo parameters, this paper presents the structural characteristics and physical processes of a short-time heavy precipitation supercell that occurred in the squall line process in Shanxi Province on 24 June 2020. The results show that this squall line event occurred in front of a surface cold front,combined with infiltration of ...  相似文献   

ICESat-2植被冠层高度和地表高程数据产品用于森林高度提取的效果评价   总被引：1，自引：0，他引：1  

董佳臣  倪文俭  张志玉  孙国清 《遥感学报》2021,25(6):1294-1307

由美国宇航局(NASA)研制的新一代冰、云和陆地高程卫星(ICESat-2)于2018-09-15发射成功,其搭载的先进地形激光测高系统(ATLAS)采用微脉冲多波束光子计数激光雷达技术,可用于全球高程线采样数据的获取.目前公开发布了9种数据产品,其中包括植被冠层高度和地表高程数据产品(ATL08),为全球森林结构参数...  相似文献   

江西省暖季重大短时强降水敏感性参数分析及概念模型     

付超  谌芸  单九生  朱克云 《气象科学》2021,41(1):39-49

利用江西省2010-2016 年5-9 月1 597 个观测站逐小时降水资料,ERA Interim,Daily逐日4 次0.125°×0.125°再分析资料以及南昌和赣州探空资料,筛选出84 例重大短时强降水过程,并建立了5 种重大短时强降水概念模型:冷锋型、西南急流型、副高边缘型、暖切型和台风型,各型分别占比29％...  相似文献   

基于机器学习的多施工参数盾构施工姿态预测     

夏汉庸  尹和军  徐教煌  王嘉伟  黄毅 《测绘通报》2021,(1):157-160,164

针对盾构施工过程中参数易变、轴线难以预测控制的问题,本文提出了基于机器学习的多施工参数盾构施工姿态预测方法,分析了在复杂环境下影响盾构姿态掘进施工的参数,以及掘进参数和盾构姿态内在的关联关系,建立了盾构姿态预测模型,实现了盾首盾尾中心坐标与设计轴线的偏差计算;最后结合某地铁施工段,验证了该预测模型的可行性.  相似文献   

Analysis of pile subjected to torsion in multi‐layered soil     

A. Misra  Rajni Saggu  D. Basu  T. Chakraborty 《国际地质力学数值与分析法杂志》2014,38(5):475-492

A new method of analysis of piles in multi‐layered elastic soil subjected to a torque at the head is developed. The differential equation governing the angle of twist in the pile is derived using the variational principles of mechanics. The method of initial parameters is used to obtain closed‐form solutions of the angle of twist and torque in the pile as a function of depth. The inputs required for the analysis are shear moduli of pile and soil, pile geometry and thickness of soil layers. Copyright © 2013 John Wiley & Sons, Ltd.  相似文献   

Analyses of Wolf-Rayet ultraviolet spectra     

Krzysztof Rochowicz 《Astrophysics and Space Science》1996,238(1):71-74

Ultraviolet spectra of population I WR stars obtained from IUE archive are used to determine fundamental stellar parameters. Terminal velocities for 85 galactic and LMC Wolf-Rayet stars were obtained by means of the empirical relation between spectral quantities easily measured in low resolution and high-resolution terminal velocity measurements. Temperatures and so-called transformed radii were derived based on available contour plots of spectral characteristics for a grid of NLTE models. The effect of the reddening law on stellar far ultraviolet continua is emphasized and the revised extinction curve towards WR stars is used for dereddening. For the sample of stars attributed to open clusters or associations we construct the stellar distance scale and adopt it for the other WR stars. The remaining fundamental parameters are derived and HR diagram for population I WR stars is presented.  相似文献   

太阳二维光谱观测研究的进展和展望     

方成  黄佑然 《天文学进展》1995,13(1):3-11

论述了太阳二维光谱观测和研究的重大意义，综述了二维光谱观测技术和仪器的进展，特别介绍了应用ＣＣＤ的成像光谱仪的最近发展。文中还介绍了近年来二维光谱观测研究所取得的一些新结果，展望了未来观测技术和课题研究的发展前景。  相似文献   

星载合成孔径雷达成像处理     

陈艳玲   《中国科学院上海天文台年刊》2005,(1):22-30

合成孔经雷达(Synthetic Aperture Radar,SAR)是当今微波遥感领域的研究热点,其全天候、全天时、高分辨率以及穿透地表等特点使其具备其他传感器不可比拟的优势,因此得到了极其广泛的应用。成像处理是SAR技术的核心部分。分析了星载SAR点目标回波信号模型和几种常用的星载SAR数字成像处理算法。以距离-多普勒算法为例,阐述了距离压缩和方位压缩的实质,详细讨论了多普勒参数估计、距离徙动校正和斑点噪声的去除等几个关键的问题。采用ERS-1卫星数据做了成像实验,并对SAR成像技术加以总结。  相似文献   

Population Synthesis for Mira Variables     

Chun-Hua Zhu  Chao-Zheng Zha Department of Physics  Xinjiang University  Urumqi   《中国天文和天体物理学报》2005,5(4):419-425

By means of a population synthesis code, we investigate the Mira variables. Their birth rate (over 0.65 yr-1) and their number (-130000) in the Galaxy are estimated. For all possible Mira variables, ranges of their initial masses, pulsating periods, mass losses and lifetimes are given. We check our model with the observed Mira variables near the Sun and our results prove to be valid.  相似文献