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时间副词和否定副词“不”的相对位序 被引量:3
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作者 潘青 乐玥 《贵州教育学院学报》 2008年第11期70-72,共3页
学界认为时间副词一般位于否定副词"不"之前,通过考察各类时间副词和否定副词"不"之间的相对位序的语料基础上发现时间副词并不总是位于否定副词"不"之前,归纳出和否定副词"不"有三种位置关系... 学界认为时间副词一般位于否定副词"不"之前,通过考察各类时间副词和否定副词"不"之间的相对位序的语料基础上发现时间副词并不总是位于否定副词"不"之前,归纳出和否定副词"不"有三种位置关系的时间副词的类。 展开更多
关键词 时间副词 否定副词“不” 相对位序
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Effects of friction variability on isolation performance of rolling-spring systems 被引量:1
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作者 魏标 王鹏 +3 位作者 杨添涵 戴公连 蒋丽忠 文颖 《Journal of Central South University》 SCIE EI CAS CSCD 2016年第1期233-239,共7页
By taking a rolling-spring isolation system as the study object, the effects of the non-uniform distribution of rolling friction coefficient on its isolation performance were analyzed by a compiled computer program. T... By taking a rolling-spring isolation system as the study object, the effects of the non-uniform distribution of rolling friction coefficient on its isolation performance were analyzed by a compiled computer program. The results show that the errors associated with the structural maximum relative displacement, acceleration and residual displacement due to ignoring the friction variability sequentially grow. This rule is weakened by the spring action, however, the unreasonable spring constant will cause sympathetic vibration. Under the condition of large friction variability, in the calculation of the structural maximum relative displacement and acceleration, the friction variability should be considered. When the structural residual displacement is concerned, the variability of rolling friction coefficient should be fully considered regardless of the friction variability. 展开更多
关键词 rolling-spring structure seismic isolation rolling friction seismic performance
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Seismic performance of isolation system of rolling friction with springs
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作者 魏标 戴公连 +1 位作者 文颖 夏烨 《Journal of Central South University》 SCIE EI CAS 2014年第4期1518-1525,共8页
In order to study an isolation system of rolling friction with springs, computer programs were compiled to evaluate the seismic performance based on its movement characteristics. Through the programs, the influences o... In order to study an isolation system of rolling friction with springs, computer programs were compiled to evaluate the seismic performance based on its movement characteristics. Through the programs, the influences of various seismic performance factors, e.g., rolling friction coefficient, spring constant, were systematically investigated. Results show that by increasing the rolling friction coefficient, the structural relative displacement due to seismic load effectively decreases, while the structural response magnitude varies mainly depending on the correlations between the following factors: the spring constant, the earthquake intensity, and the rolling friction coefficient. Furthermore, increasing the spring constant can decrease the structural relative displacement, as well as residual displacement, however, it increases the structural response magnitude. Finally, based on the analyses of various seismic performance factors subjected to the scenario earthquakes, optimized theoretical seismic performance can be achieved by reasonably combining the spring constant and the rolling friction coefficient. 展开更多
关键词 structure seismic isolation rolling friction spring
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Detecting super-Nyquist-frequency gravitational waves using a pulsar timing array
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作者 Shu-Xu Yi Shuang-Nan Zhang 《Science China(Physics,Mechanics & Astronomy)》 SCIE EI CAS CSCD 2016年第8期78-86,共9页
The maximum frequency of gravitational waves(GWs) detectable with traditional pulsar timing methods is set by the Nyquist frequency( fNy) of the observation. Beyond this frequency, GWs leave no temporal-correlated sig... The maximum frequency of gravitational waves(GWs) detectable with traditional pulsar timing methods is set by the Nyquist frequency( fNy) of the observation. Beyond this frequency, GWs leave no temporal-correlated signals; instead, they appear as white noise in the timing residuals. The variance of the GW-induced white noise is a function of the position of the pulsars relative to the GW source. By observing this unique functional form in the timing data, we propose that we can detect GWs of frequency >f_(Ny)(super-Nyquist frequency GWs; SNFGWs). We demonstrate the feasibility of the proposed method with simulated timing data.Using a selected dataset from the Parkes Pulsar Timing Array data release 1 and the North American Nanohertz Observatory for Gravitational Waves publicly available datasets, we try to detect the signals from single SNFGW sources. The result is consistent with no GW detection with 65.5% probability. An all-sky map of the sensitivity of the selected pulsar timing array to single SNFGW sources is generated, and the position of the GW source where the selected pulsar timing array is most sensitive to is λ_s =.0.82,β_s =-1.03(rad); the corresponding minimum GW strain is h = 6.31 × 10^(-11) at f = 1 × 10^(-5) Hz. 展开更多
关键词 gravitational wave pulsar black hole
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