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单人Bounce荷载下楼盖结构加速度反应谱设计 被引量:8
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作者 陈隽 王磊 +2 位作者 楼佳悦 徐若天 李果 《振动与冲击》 EI CSCD 北大核心 2015年第5期14-19,38,共7页
Bounce指双脚不离地的人体上下往复运动,是一种常见的有节奏人致激励。采用先进的无线测力鞋垫技术收集了175条bounce荷载曲线,计算每条荷载曲线的单自由系统加速度反应谱,在此基础上提出了设计反应谱分段表达式,主要分为三段:对应bou... Bounce指双脚不离地的人体上下往复运动,是一种常见的有节奏人致激励。采用先进的无线测力鞋垫技术收集了175条bounce荷载曲线,计算每条荷载曲线的单自由系统加速度反应谱,在此基础上提出了设计反应谱分段表达式,主要分为三段:对应bounce一阶主频范围2~3.5 Hz的第一平台段、对应二阶主频范围4~7 Hz的第二平台段以及对应高阶频率的下降段,由试验数据分析给出了两个平台段的不同保证率下的代表值以及下降段参数。文中给出了设计反应谱的详细使用步骤,并通过大跨楼盖试验模型验证了方法的准确性。 展开更多
关键词 大跨楼盖 振动舒适度 加速度反应谱 bounce荷载
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单人Bounce荷载的实验建模研究 被引量:6
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作者 王磊 陈隽 +1 位作者 楼佳悦 李果 《振动与冲击》 EI CSCD 北大核心 2016年第17期52-57,共6页
Bounce指音乐会或体育比赛中常见的观众双脚不离地的身体有节奏的上下往复运动。利用测力板以及无线测力鞋垫,开展了单人在不同频率下的Bounce荷载的测试试验,共得到了109人次822条有效单人Bounce荷载记录。在此基础上,建立了Bounce荷... Bounce指音乐会或体育比赛中常见的观众双脚不离地的身体有节奏的上下往复运动。利用测力板以及无线测力鞋垫,开展了单人在不同频率下的Bounce荷载的测试试验,共得到了109人次822条有效单人Bounce荷载记录。在此基础上,建立了Bounce荷载的傅里叶级数模型,给出了四阶动载因子和相位角的建议值,并与国外已有模型进行了对比分析。本文模型所模拟的Bounce荷载与实测荷载的时域特性相同,所引起的结构响应幅值一致,可供工程设计参考使用。 展开更多
关键词 bounce荷载 大跨楼盖 傅里叶级数模型 动载因子
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多人Bounce荷载下结构动力响应折减系数研究 被引量:3
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作者 陈隽 任静雅 王磊 《振动与冲击》 EI CSCD 北大核心 2019年第11期48-53,共6页
体育比赛、演唱会中观众原地身体上下往复式的欢庆动作会引起Bounce荷载,是典型的有节奏人致动力荷载。该研究将考虑和不考虑人群协同性所计算出的结构响应的比值,定义为Bounce荷载下的结构动力响应折减系数,利用小组人群同步Bounce荷... 体育比赛、演唱会中观众原地身体上下往复式的欢庆动作会引起Bounce荷载,是典型的有节奏人致动力荷载。该研究将考虑和不考虑人群协同性所计算出的结构响应的比值,定义为Bounce荷载下的结构动力响应折减系数,利用小组人群同步Bounce荷载的实测数据,研究了折减系数随人数、结构频率和阻尼比的变化规律,并提出了对应的设计曲线及表达式。应用于实际结构响应计算时,首先由反应谱法计算单人Bounce荷载下结构的动力响应,将其乘以总体重并考虑振型值影响后,再乘以对应的折减系数,即可实现考虑协同性的人群Bounce荷载下结构动力响应的快速计算,算例分析表明了上述步骤及所建议的折减系数的合理性。 展开更多
关键词 bounce荷载 响应折减系数 振动舒适度 大跨工程结构
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Matter Bounce宇宙模型研究
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作者 王晓明 《山西大同大学学报(自然科学版)》 2013年第3期23-24,27,共3页
通过描述宇宙学的发展历史和现状,指出大爆炸理论和暴涨理论虽然有许多优点,可以解释许多现象,但它们并不是完美无缺,无懈可击,仍然有一些无法解释的问题。而matter bounce宇宙模型是一个可以取代前两种理论的模型,可以得到与宇宙观测... 通过描述宇宙学的发展历史和现状,指出大爆炸理论和暴涨理论虽然有许多优点,可以解释许多现象,但它们并不是完美无缺,无懈可击,仍然有一些无法解释的问题。而matter bounce宇宙模型是一个可以取代前两种理论的模型,可以得到与宇宙观测相吻合的结论,因此研究这个模型是非常有意义的。 展开更多
关键词 宇宙学 宇宙 暴涨 MATTER bounce
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Multi-Bounce ATR-FTIR结合Gram-Schmidt正交化法计算烟用香精相似度 被引量:3
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作者 张翼鹏 段焰青 +3 位作者 者为 刘秀明 李源栋 王家俊 《湖北农业科学》 2015年第8期1903-1905,1944,共4页
采集2种不同风格特征烟用香精的Multi-Bounce Attenuated Total Reflectance-Fourier Transform Infrared Spectroscopy(Multi-Bounce ATR-FTIR)指纹图谱,运用主成分分析法各筛选出30条光谱,结合Gram-Schmidt正交化方法,分别建立了2类... 采集2种不同风格特征烟用香精的Multi-Bounce Attenuated Total Reflectance-Fourier Transform Infrared Spectroscopy(Multi-Bounce ATR-FTIR)指纹图谱,运用主成分分析法各筛选出30条光谱,结合Gram-Schmidt正交化方法,分别建立了2类不同风格特征烟用香精的相似度鉴别模型。使用鉴别模型对未知样品进行相似度计算,并评价使用效果。结果显示,当相似度高于90%时,可以判定属于同一类香精,且相似度越高,风格特征越接近;当相似度低于90%时,可以判定不属于同一类香精,且相似度越低,风格特征的差异越显著。 展开更多
关键词 烟用香精 Multi—bounce ATR—FTIR指纹图谱 Gram—Schmidt正交化法 相似度
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Corotating drift-bounce resonance of plasmaspheric electron with poloidal ULF waves 被引量:2
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作者 Qiu-Gang Zong YongFu Wang +4 位作者 Jie Ren XuZhi Zhou SuiYan Fu Robert Rankin Hui Zhang 《Earth and Planetary Physics》 2017年第1期2-12,共11页
The purpose of this paper is to understand how low energy plasmaspheric electrons respond to ULF waves excited by interplanetary shocks impinging on magnetosphere. It is found that both energy and pitch angle disperse... The purpose of this paper is to understand how low energy plasmaspheric electrons respond to ULF waves excited by interplanetary shocks impinging on magnetosphere. It is found that both energy and pitch angle dispersed plasmaspheric electrons with energy of a few eV to tens of eV can be generated simultaneously by the interplanetary shock. The subsequent period of successive dispersion signatures is around 40 s and is consistent with the ULF wave period(third harmonic). By tracing back the energy and pitch angle dispersion signatures, the position of the electron injection region is found to be off-equator at around -32° in the southern hemisphere. This can be explained as the result of injected electrons being accelerated by higher harmonic ULF waves(e.g. third harmonic) which carry a larger amplitude electric field off-equator. The dispersion signatures are due to the flux modulations(or accelerations) of " local" plasmaspheric electrons rather than electrons from the ionosphere. With the observed wave-borne large electric field excited by the interplanetary shock impact, the kinetic energy can increase to a maximum of 23 percent in one bouncing cycle for plasmaspheric electrons satisfying the drift-bounce resonance condition by taking account of both the corotating drift and bounce motion of the local plasmaspheric electron. 展开更多
关键词 drift-bounce resonance plasmaspheric electron poloidal mode ULF wave
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Constraints on Deceleration Parameter of a 5D Bounce Cosmological Model from Recent Cosmic Observations
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作者 李杰超 徐立昕 +2 位作者 吕剑波 常葆荣 刘宏亚 《Chinese Physics Letters》 SCIE CAS CSCD 2008年第2期802-804,共3页
We study the constraint on deceleration parameter q from the recent SNela Gold dataset and observational Hubble data by using a model-independent deceleration parameter q(z) = 1/2 - a/(1 + z)^b under the flve-dim... We study the constraint on deceleration parameter q from the recent SNela Gold dataset and observational Hubble data by using a model-independent deceleration parameter q(z) = 1/2 - a/(1 + z)^b under the flve-dimensional bounce cosmological model. For the cases of SNeIa Gold dataset, Hubble data, and their combination, the present results show that the constraints on transition redshift ZT are 0.35-0.07^+0.14,0.68-0.58^+1.47,and 0.55-0.09^+0.18 with 1σ errors,respectively. 展开更多
关键词 PROBE WMAP OBSERVATIONS HUBBLE-SPACE-TELESCOPE DARK ENERGY BIG bounce CONSTANT QUINTESSENCE ANISOTROPY SUPERNOVA EVOLUTION REDSHIFT
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Observational constraints on the accelerating universe in the framework of a 5D bounce cosmological model
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作者 吕剑波 徐立昕 +1 位作者 刘墨林 桂元星 《Chinese Physics B》 SCIE EI CAS CSCD 2009年第4期1711-1720,共10页
In the framework of a five-dimensional (5D) bounce cosmological model, a useful function f(z) is obtained by giving a concrete expression of deceleration parameter q(z) = q1 +q2/1+1n(1+z) Then using the obt... In the framework of a five-dimensional (5D) bounce cosmological model, a useful function f(z) is obtained by giving a concrete expression of deceleration parameter q(z) = q1 +q2/1+1n(1+z) Then using the obtained Hubble parameter H(z) according to the function f(z), we constrain the accelerating universe from recent cosmic observations: the 192 ESSENCE SNe Ia and the 9 observational H(z) data. The best fitting values of transition redshift zT and current deceleration parameter q0 are given as zT =0.65-0.12^+0.25 and q0=-0.76-0.15^+0.15(1σ). Furthermore, in the 5D bounce model it can be seen that the evolution of equation of state (EOS) for dark energy Wde can cross over -1 at about z = 0.23 and the current value W0de : =-1.15 〈 -1. On the other hand, by giving a concrete expression of model-independent EOS of dark energy Wde, in the 5D bounce model we obtain the best fitting values zT = 0 .66-0.08^+0.11 and q0=-0.69-0.10^+0.10(1σ) from the recently observed data: the 192 ESSENCE SNe Ia, the observational H(z) data, the 3-year Wilkinson Microwave Anisotropy Probe (WMAP), the Sloan Digital Sky Survey (SDSS) baryon acoustic peak and the x-ray gas mass fraction in clusters. 展开更多
关键词 bounce cosmology deceleration parameter equation of state (EOS) dark energy (DE)
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Optimization design method of contact bounce and breakaway initial velocity for aerospace electromagnetic relay
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作者 叶雪荣 梁慧敏 翟国富 《Journal of Harbin Institute of Technology(New Series)》 EI CAS 2011年第5期130-136,共7页
Aerospace electromagnetic relay is an electric component that has been widely used in aerospace industry.Contact bounce and contact breakaway for initial velocity are the key parameters that have strong influence on r... Aerospace electromagnetic relay is an electric component that has been widely used in aerospace industry.Contact bounce and contact breakaway for initial velocity are the key parameters that have strong influence on reliability and electric life of the relay.Generally,it is difficult to optimize these two parameters simultaneously.In this paper,according to kinetics theory and structural mechanics,a dynamic reaction calculation model of the relay that describes contact bounce and breakaway for initial velocity is proposed.Under the constraints of contact gap and contact force,the optimal combination of debugging parameters is obtained by the application of orthogonal design.It considers the reduction of contact bounce and the augmentation of breakaway for initial velocity as the optimization objectives,and takes the debugging parameters as the optimization variables.All these above ensure the increase of contact breakaway for initial velocity and the decrease of contact bounce simultaneously,and contact arc erosion is also reduced. 展开更多
关键词 aerospace electromagnetic relay debugging parameters contact bounce contact breakaway initial velocity orthogonal design
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Modified Ceiling Bounce Model for Computing Path Loss and Delay Spread in Indoor Optical Wireless Systems
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作者 K. SMITHA A. SIVABALAN J. JOHN 《International Journal of Communications, Network and System Sciences》 2009年第8期754-758,共5页
This paper proposes modifications to the tradional Ceiling Bounce Model and uses it to characterize diffuse indoor optical wireless channel by analyzing the effect of transceiver position on signal propagation propert... This paper proposes modifications to the tradional Ceiling Bounce Model and uses it to characterize diffuse indoor optical wireless channel by analyzing the effect of transceiver position on signal propagation properties. The modified approach uses a combination of the tradional ceiling bounce method and a statistical approach. The effects of different transmitter-receiver separations and height of the ceiling on path loss and delay spread are studied in detail. 展开更多
关键词 INDOOR OPTICAL Channel MODIFIED CEILING bounce MODEL Path Loss Delay Spread
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Could Gravitons from a Prior Universe Survive a (LQG Inspired) “Quantum Bounce” to Re-Appear in Our Present Universe?
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作者 Andrew Walcott Beckwith 《Journal of High Energy Physics, Gravitation and Cosmology》 2017年第4期624-634,共11页
We ask the question if a formula for entropy, as given by with a usual value ascribed of initial entropy of the onset of inflation can allow an order of magnitude resolution of the question of if there could be a surv... We ask the question if a formula for entropy, as given by with a usual value ascribed of initial entropy of the onset of inflation can allow an order of magnitude resolution of the question of if there could be a survival of a graviton from a prior to the present universe, using typical Planckian peak temperature values of . We obtain values consistent with up to 1038 gravitons contributing to an energy value of if we assume a relic energy contribution based upon each graviton initially exhibiting a frequency spike of 1010 Hz. The value of is picked from looking at the aftermath of what happens if there exists a quantum bounce with a peak density value of [1] in a regime of LQG bounce regime radii of the order of magnitude of meters. The author, in making estimates specifically avoids using ,?by setting the chemical potential for ultra high temperatures for reasons which will be brought up in the conclusion. 展开更多
关键词 GRAVITONS Prior UNIVERSE QUANTUM bounce
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Cosmology with Bounce by Flat Space-Time Theory of Gravitation and a New Interpretation
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作者 Walter Petry 《Journal of Modern Physics》 2013年第7期20-25,共6页
General relativity predicts a singularity in the beginning of the universe being called big bang. Recent developments in loop quantum cosmology avoid the singularity and the big bang is replaced by a big bounce. A cla... General relativity predicts a singularity in the beginning of the universe being called big bang. Recent developments in loop quantum cosmology avoid the singularity and the big bang is replaced by a big bounce. A classical theory of gravitation in flat space-time also avoids the singularity under natural conditions on the density parameters. The universe contracts to a positive minimum and then it expands during all times. It is not symmetric with regard to its minimum implying a finite age measured with proper time of the universe. The space of the universe is flat and the total energy is conserved. Under the assumption that the sum of the density parameters is a little bit bigger than one the universe is very hot in early times. Later on, the cosmological model agrees with the one of general relativity. A new interpretation of a non-expanding universe may be given by virtue of flat space-time theory of gravitation. 展开更多
关键词 GRAVITATION COSMOLOGY BIG bounce FLAT Space NO BIG Bang Non-Expanding Universe
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Complete Coalescence, Partial Bounce and Rebound: Different Regimes Resulting from the Interaction of a Free Falling Drop with a Target Fluid
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作者 Yuli D.Chashechkin Andrey Y.Ilinykh 《Fluid Dynamics & Materials Processing》 EI 2020年第4期801-811,共11页
The interaction of a falling drop(diluted aqueous solution of ink in various concentrations)with a target fluid(partially degassed tap water)has been tracked by means of high-resolution video recording and photography... The interaction of a falling drop(diluted aqueous solution of ink in various concentrations)with a target fluid(partially degassed tap water)has been tracked by means of high-resolution video recording and photography.The experimental setup has carefully been prepared in order to preserve the axial symmetry of initial conditions.Three regimes of interaction have been identified accordingly(depending on the drop velocity as controlled by the distance of fall):rapid droplet coalescence,rebound with the conservation of the drop volume and shape,and partial coalescence.Previous findings are recovered and confirmed,and enriched with heretofore unseen observations of complex partial coalescence.An extensive set of data is reported to support understanding of the observed dynamics and their repeatability and reproducibility.The overall study has been carried out with the express intent to spur the future development of detailed mathematical models and numerical methods suited for this kind of problems. 展开更多
关键词 DROP COALESCENCE bounce spray transport of matter miscible fluids
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Prostate specific antigen bounce after intensity-modulated radiation therapy in an Asian population
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作者 Yu Guang Tan Weber Lau Kam On +1 位作者 Hong Hong Huang Terence Tan Wee Kiat 《Asian Journal of Urology》 2016年第2期59-63,共5页
Objective:Serum prostate specific antigen(PSA)is commonly used to evaluate treatment response after definitive radiation therapy(RT).However,PSA levels can temporarily rise without a clear reason,termed“PSA bounce”,... Objective:Serum prostate specific antigen(PSA)is commonly used to evaluate treatment response after definitive radiation therapy(RT).However,PSA levels can temporarily rise without a clear reason,termed“PSA bounce”,and often engender great anxiety for both patients and physicians.The present study aimed to determine the prevalence and factors that predict“PSA bounce”after intensity-modulated radiation therapy(IMRT),and the relevance to biochemical failure and cancer recurrence in an Asian population.Methods:We retrospectively reviewed 206 patients who received IMRT for prostate cancer from 2004 to 2012 in the National Cancer Centre Singapore.These patients were followed up with regular PSA monitoring.We defined“PSA bounce”as a rise of 0.1 ng/mL,followed by two consecutive falls.Patients with biochemical failure(PSA nadir t 2 ng/mL)were further evaluated for cancer recurrence.Results:Sixty-one patients(29.6%)experienced“PSA bounce”,at a median time of 16 months and lasted for 12 months.Age remained the most consistent predictor of the incidence,duration and extent of“PSA bounce”.Other contributory factors included baseline PSA,Gleason score and PSA nadir.Hormonal therapy and prostate volume did not affect this phenomenon.Sixteen patients(7.8%)developed biochemical recurrence,at median time of 32 months,of which 11 were confirmed to have metastatic disease.The median follow-up time was 71 months. 展开更多
关键词 Prostate specific antigen Prostate specific antigen bounce Prostate cancer Intensity modulated radiation therapy
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Predicting the Curvature of the Cosmos, and Point of Volume Contraction in a Big Bounce Scenario
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作者 Christopher Pilot 《International Journal of Astronomy and Astrophysics》 2021年第2期265-278,共14页
Based on the latest Planck surveys, the universe is close to being remarkably flat, and yet, within observational error, there is still room for a slight curvature. If the curvature is positive, then this would lead t... Based on the latest Planck surveys, the universe is close to being remarkably flat, and yet, within observational error, there is still room for a slight curvature. If the curvature is positive, then this would lead to a closed universe, as well as allow for a big bounce scenario. Working within these assumptions, and using a simple model, we predict that the cosmos may have a positive curvature in the amount, <span style="white-space:nowrap;"><span style="white-space:nowrap;">Ω<sub>0</sub>=1.001802</span></span>, a value within current observational bounds. For the scaling laws associated with the density parameters in Friedmann’s equations, we will assume a susceptibility model for space, where, <img src="Edit_18751d6f-dbfa-47ba-be7c-8298073a34fd.png" alt="" style="white-space:normal;" />, equals the smeared cosmic susceptibility. If we allow the <img src="Edit_18751d6f-dbfa-47ba-be7c-8298073a34fd.png" alt="" /> to <em>decrease with increasing</em> cosmic scale parameter, “<em>a</em>”, then we can predict a maximum Hubble volume, with minimum CMB temperature for the voids, before contraction begins, as well as a minimum volume, with maximum CMB temperature, when expansion starts. A specific heat engine model for the cosmos is also entertained for this model of a closed universe. 展开更多
关键词 Cosmic Curvature Closed Universe Cyclic Universe Heat Engine Model for Universe Big bounce Susceptibility Model for Universe Carnot Cycle Model for Cosmos Causal Isotropy in CMB Temperature
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Gedanken Experiment for Energy, and Scale Factor, Based upon the Assumption of Quintessence and Idea of Quantum Bounce in Order to Isolate Admissible Frequency for Gravitational Waves in the Beginning of Cosmological Evolution
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作者 Andrew Walcott Beckwith 《Journal of High Energy Physics, Gravitation and Cosmology》 2016年第1期92-97,共6页
We initially look at a non-singular universe representation of time, and of comparing a general formula of a cosmological Potential energy as given by Padmanbhan, with Weinberg’s Quintessence Potential energy. Isolat... We initially look at a non-singular universe representation of time, and of comparing a general formula of a cosmological Potential energy as given by Padmanbhan, with Weinberg’s Quintessence Potential energy. Isolating a given time component which may serve as an introduction. We then compare this to when , and seeing what the time component then allows as far as available initial energy, the scale factor a(t) and &oslash;, then finally admissible frequency, for Pre Planckian process generated Gravitational waves. 展开更多
关键词 Gedanken Experiment Quantum bounce Gravitational Waves Cosmological Evolution
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Some Tools to Model Ground or Supply Bounces Induced in and out of Heterogeneous Integrated Circuits
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作者 Christian Gontrand Olivier Valorge +4 位作者 Rabah Dahmanil Fengyuan Sun Francis Calmon Jacques Verdier Paul Dautriche 《Computer Technology and Application》 2011年第10期788-800,共13页
Electrical ground looks simple on a schematic; unfortunately, the actual performance of a circuit is dictated by its layout (and by its printed-circuit-board). When the ground node moves, system performance suffers ... Electrical ground looks simple on a schematic; unfortunately, the actual performance of a circuit is dictated by its layout (and by its printed-circuit-board). When the ground node moves, system performance suffers and the system radiates electromagnetic interferences. But the understanding of the physics of ground noise can provide an intuitive sense for reducing the problem. Ground bounce can produce transients with amplitudes of volts; most often changing magnetic flux is the cause; in this work, the authors use a Finite-Difference Time-Domain to begin to understand such phenomena. Additionally, predicting substrate cross-talks in mixed-signal circuits has become a critical issue to preserve signal integrity in future integrated systems. Phenomena that involve parasitic signal propagation into the substrate are discussed. A simple methodology to predict the substrate cross-talk and some associated tools are presented. Finally, the authors indicate a stochastic method which could grasp both outer or inner RF (Radio-Frequency) radiations and substrate parasites. 展开更多
关键词 Electromagnetism 3D (three-dimensional) integration noise TSV (through silicon vias) ground or supply bounce mixed analog-digital integrated circuits substrate noise stochastic methodology.
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多簧片结构的磁保持继电器多物理场刚柔耦合仿真模型建立和实验分析 被引量:1
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作者 赵靖英 李宁 +1 位作者 张雪辉 赵正元 《电工技术学报》 EI CSCD 北大核心 2024年第10期3192-3205,共14页
多簧片结构的磁保持继电器衔铁转动引起的触点碰撞、弹跳现象使运动过程复杂,静、动态特性理论分析和仿真模型建立困难。以某型号多簧片结构的磁保持继电器为研究对象,理论分析结构拓扑及工作机理,考虑触点间切入深度,引入狄拉克函数和... 多簧片结构的磁保持继电器衔铁转动引起的触点碰撞、弹跳现象使运动过程复杂,静、动态特性理论分析和仿真模型建立困难。以某型号多簧片结构的磁保持继电器为研究对象,理论分析结构拓扑及工作机理,考虑触点间切入深度,引入狄拉克函数和赫维赛德函数,解决簧片受力分散及触点由于碰撞、弹跳引起的作用力不连续问题;将簧片等效为悬臂梁,基于欧拉-伯努利梁理论建立触簧系统三簧片分段耦合动力学模型。利用Ansys Maxwell引入基于误差的自适应网格划分方法求解电磁机构静态特性;考虑触簧系统簧片运动变形效应,通过ADAMS基于模态理论,构建刚柔耦合动力学仿真模型。基于分段动力学思想,搭建电-磁-机械运动多物理场刚柔耦合仿真模型。利用高速摄像机、电流探头等设计磁保持继电器实验方案,搭建实验平台,测试并分析磁保持继电器触点吸合运动时间、触点压力、弹跳时间、线圈电流,并分析人工装配簧片引起触点压力不同使继电器动作过程存在的不一致性问题,验证该文所提多簧片结构的磁保持继电器特性分段耦合分析方法和多物理场刚柔耦合仿真模型的有效性。 展开更多
关键词 磁保持继电器 多簧片结构 碰撞弹跳 分段耦合动力学模型 多物理场刚柔耦合
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基于体弹跳射线法的等离子体目标散射建模技术研究
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作者 杨伟 蔡宇峰 +3 位作者 胡皓全 陈波 赵志钦 肖礼康 《电子科技大学学报》 EI CAS CSCD 北大核心 2024年第1期1-7,共7页
针对非均匀等离子体包裹目标的电磁散射问题,提出了一种基于体射弹射线法的建模技术,重点研究电磁波在介质体中的传播特性及散射分析方法。针对在介质体中透射与反射射线数据量激增的问题,提出了基于迭代追踪加速技术以此提高体介质散... 针对非均匀等离子体包裹目标的电磁散射问题,提出了一种基于体射弹射线法的建模技术,重点研究电磁波在介质体中的传播特性及散射分析方法。针对在介质体中透射与反射射线数据量激增的问题,提出了基于迭代追踪加速技术以此提高体介质散射中透射反射射线的追踪效率。仿真实例表明,与传统弹跳射线法相比,体弹跳射线法能更快速准确地计算出等离子体目标的散射特性。采用所提出的技术研究了等离子体鞘套对阿波罗号返回舱雷达散射截面积的影响,验证了等离子体对目标雷达散射截面积有一定缩减作用。 展开更多
关键词 迭代射线追踪 等离子体鞘套 雷达散射截面积 体弹跳射线法
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动车组合闸过电压故障机理兮析及仿真研究
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作者 张明锐 张宁川 刘正威 《城市轨道交通研究》 北大核心 2024年第6期84-89,94,共7页
[目的]动车组出分相时,断路器合闸产生的过电压会加剧高压设备的绝缘老化,研究合闸过电压的产生机理及影响因素对动车组主电路绝缘匹配和设备选型具有理论意义。[方法]结合动车组主电路结构和过分相过程,分析其正常运行方式下操作过电... [目的]动车组出分相时,断路器合闸产生的过电压会加剧高压设备的绝缘老化,研究合闸过电压的产生机理及影响因素对动车组主电路绝缘匹配和设备选型具有理论意义。[方法]结合动车组主电路结构和过分相过程,分析其正常运行方式下操作过电压的形成原因。考虑真空断路器合闸弹跳特性对过电压的特殊影响,建立动车组主电路仿真模型;对比研究动车组主电路合闸过电压特征,得出主回路状态动作时刻、动车组高压电缆参数、接触网参数及设备特性对过电压的影响规律。[结果及结论]极端状态下过电压峰值为工频电压峰值的2.39倍,接近《高速动车组整车试验规范》规定的2.4倍,在极端工况下产生的过电压会对动车组高压设备的绝缘性能产生影响,甚至导致击穿现象。因此,需采取如采用相控合闸技术控制断路器在目标相位闭合、选择单位分布电容较小的高压电缆、改进真空断路器的机械特性等相关措施进行防范,以有效降低动车组合闸过电压。 展开更多
关键词 动车组 真空断路器 弹跳特性 操作过电压
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