Dynamic soil−pile−superstructure interaction is crucial for understanding pile behavior in earthquake-prone ground.Evaluating the safety of piles requires determining the seismic bending moment caused by combined iner...Dynamic soil−pile−superstructure interaction is crucial for understanding pile behavior in earthquake-prone ground.Evaluating the safety of piles requires determining the seismic bending moment caused by combined inertial and kinematic interactions,which is challenging.This paper addresses this problem through numerical simulations of piles in different soil sites,considering soil nonlinearity.Results reveal that the period of the soil site significantly affects the interaction among soil,piles,and structures.Bending moments in soft and hard soil sites exceed those in medium soil sites by more than twice.Deformation modes of piles exhibit distinct characteristics between hard and soft soil sites.Soft soil sites exhibit a singular inflection point,while hard soil sites show two inflection points.In soft soil sites,pile-soil kinematic interaction gradually increases bending moment from tip to head,with minor influence from superstructure’s inertial interaction.In hard soil sites,significant inertial effects from soil,even surpassing pile-soil kinematic effects near the tip,lead to reversed superposition bending moment.Superstructure’s inertial interaction notably impacts pile head in hard soil sites.A simplified coupling method is proposed using correlation coefficient to represent inertial and kinematic interactions.These findings provide insights into complex seismic interactions among soil,piles,and structures.展开更多
The study ofkiloparsec-scale dual active galactic nuclei （AGN） provides important clues for understanding the co-evolution between host galaxies and their central supermassive black holes undergoing a merging proces...The study ofkiloparsec-scale dual active galactic nuclei （AGN） provides important clues for understanding the co-evolution between host galaxies and their central supermassive black holes undergoing a merging process. We present long-slit spectroscopy of J0038 ＋4128, a kiloparsec-scale dual AGN candidate, discovered recently by Huang et al., using the Yunnan Faint Object Spectrograph and Camera （YFOSC） mounted on the Lijiang 2.4-m telescope administered by Yunnan Observatories. From the long-slit spectra, we find that the average relative line-of-sight （LOS） velocity between the two nuclei （J0038＋4128N and J0038＋4128S） is about 150 km s-1. The LOS velocities of the emission lines from the gas ionized by the nuclei activities and of the absorption lines from stars governed by the host galaxies for different regions of J0038＋4128 exhibit the same trend. The same trend in velocities indicates that the gaseous disks are co-rotating with the stellar disks in this ongoing merging system. We also find several knots/giant H II regions scattered around the two nuclei with strong star formation revealed by the observed line ratios from the spectra. Those regions are also clearly detected in images from HST F336W/U-band and HST F555W/V-band.展开更多
基金the National Natural Science Foundation of China(Grant No.42277163)for the financial support to this work.
文摘Dynamic soil−pile−superstructure interaction is crucial for understanding pile behavior in earthquake-prone ground.Evaluating the safety of piles requires determining the seismic bending moment caused by combined inertial and kinematic interactions,which is challenging.This paper addresses this problem through numerical simulations of piles in different soil sites,considering soil nonlinearity.Results reveal that the period of the soil site significantly affects the interaction among soil,piles,and structures.Bending moments in soft and hard soil sites exceed those in medium soil sites by more than twice.Deformation modes of piles exhibit distinct characteristics between hard and soft soil sites.Soft soil sites exhibit a singular inflection point,while hard soil sites show two inflection points.In soft soil sites,pile-soil kinematic interaction gradually increases bending moment from tip to head,with minor influence from superstructure’s inertial interaction.In hard soil sites,significant inertial effects from soil,even surpassing pile-soil kinematic effects near the tip,lead to reversed superposition bending moment.Superstructure’s inertial interaction notably impacts pile head in hard soil sites.A simplified coupling method is proposed using correlation coefficient to represent inertial and kinematic interactions.These findings provide insights into complex seismic interactions among soil,piles,and structures.
基金Funding for the telescope has been provided by CASthe People’s Government of Yunnan Province+2 种基金supported by the National Natural Science Foundation of China(Grant Nos.11133006 and 11361140347)the Strategic Priority Research Program“The Emergence of Cosmological Structures”of the Chinese Academy of Sciences(Grant No.XDB09000000)support by the National Key Basic Research Program of China(2014CB845700)
文摘The study ofkiloparsec-scale dual active galactic nuclei （AGN） provides important clues for understanding the co-evolution between host galaxies and their central supermassive black holes undergoing a merging process. We present long-slit spectroscopy of J0038 ＋4128, a kiloparsec-scale dual AGN candidate, discovered recently by Huang et al., using the Yunnan Faint Object Spectrograph and Camera （YFOSC） mounted on the Lijiang 2.4-m telescope administered by Yunnan Observatories. From the long-slit spectra, we find that the average relative line-of-sight （LOS） velocity between the two nuclei （J0038＋4128N and J0038＋4128S） is about 150 km s-1. The LOS velocities of the emission lines from the gas ionized by the nuclei activities and of the absorption lines from stars governed by the host galaxies for different regions of J0038＋4128 exhibit the same trend. The same trend in velocities indicates that the gaseous disks are co-rotating with the stellar disks in this ongoing merging system. We also find several knots/giant H II regions scattered around the two nuclei with strong star formation revealed by the observed line ratios from the spectra. Those regions are also clearly detected in images from HST F336W/U-band and HST F555W/V-band.
