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A modified multi-group model of angular and momentum distribution of cosmic ray muons for thickness measurement and material discrimination of slabs 被引量:5
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作者 Sa Xiao Wei-Bo He +2 位作者 Ming-Cong Lan Ying Chen Mao-Bing Shuai 《Nuclear Science and Techniques》 SCIE CAS CSCD 2018年第2期111-117,共7页
Muon tomography is a capable imaging technique to measure the geometry of high-Z objects. However,most existed algorithms used in muon tomography have obscured the effects of angular distribution and momentum spectra ... Muon tomography is a capable imaging technique to measure the geometry of high-Z objects. However,most existed algorithms used in muon tomography have obscured the effects of angular distribution and momentum spectra of cosmic ray muons and reduced the spatial resolution. We present a modified multi-group model that takes into account these effects and calibrates the model by the material of lead. Performance tests establish that the model is capable of measuring the thickness of a Pb slab and identifying the material of an unknown slab on a reasonable exposure timescale, in both cases of complete and incomplete angular data. Results show that the modified multi-group model is helpful for improvements in image resolution in real applications. 展开更多
关键词 MUON tomography MODIFIED MULTI-GROUP model ANGULAR distribution momentum spectra
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Wind Structure in an Intermediate Boundary Layer Model Based on Ekman Momentum Approximation
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作者 谈哲敏 王元 《Advances in Atmospheric Sciences》 SCIE CAS CSCD 2002年第2期266-278,共13页
A quasi three–dimensional, intermediate planetary boundary layer (PBL) model is developed by including inertial acceleration with the Ekman momentum approximation, but a nonlinear eddy viscosity based on Blackadar’s... A quasi three–dimensional, intermediate planetary boundary layer (PBL) model is developed by including inertial acceleration with the Ekman momentum approximation, but a nonlinear eddy viscosity based on Blackadar’s scheme was included to improve the theoretical model proposed by Tan and Wu (1993). The model could keep the same complexity as the classical Ekman model in numerical, but extends the conventional Ekman model to include the horizontal accelerated flow with the Ekman momentum approximation. A comparison between this modified Ekman model and other simplified accelerating PBL models is made. Results show that the Ekman model overestimates (underestimates) the wind speed and pumping velocity in the cyclonic (anticyclonic) shear flow due to the neglect of the acceleration flow, however, the semi–geostrophic Ekman model overestimates the acceleration effects resulting from the underestimating (overestimating) of the wind speed and pumping velocity in the cyclonic (anticyclonic) shear flow. The Ekman momentum approximation boundary layer model could be applied to the baroclinic atmosphere. The baroclinic Ekman momentum approximation boundary layer solution has both features of classical baroclinic Ekman layer and the Ekman momentum approximate boundary lager. 展开更多
关键词 Wind structure Ekman momentum approximation Boundary layer model
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Angular Momentum Dependent Exciton Model
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作者 Zhang, Jingshang Wen, Yuanqi 《Chinese journal of nuclear physics》 EI 1994年第2期153-159,共7页
To consider the angular momentum and parity conservation the angular mo-mentum (J) and parity (π) should be addressed in the master equation of the excitonmodel.Therefore the internal transition rates and the emissio... To consider the angular momentum and parity conservation the angular mo-mentum (J) and parity (π) should be addressed in the master equation of the excitonmodel.Therefore the internal transition rates and the emission rates must be Jπ depen-dent.The angular momentum factor of the internal transition rates is given and the an-gular momentum conservation effect is discussed. 展开更多
关键词 ANGULAR momentum PARITY CONSERVATION EXCITON model
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Dynamic Modeling and Motion Simulation for A Winged Hybrid-Driven Underwater Glider 被引量:33
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作者 王树新 孙秀军 +2 位作者 王延辉 武建国 王晓鸣 《China Ocean Engineering》 SCIE EI 2011年第1期97-112,共16页
PETREL, a winged hybrid-driven underwater glider is a novel and practical marine survey platform which combines the features of legacy underwater glider and conventional AUV (autonomous underwater vehicle). It can b... PETREL, a winged hybrid-driven underwater glider is a novel and practical marine survey platform which combines the features of legacy underwater glider and conventional AUV (autonomous underwater vehicle). It can be treated as a multi-rigid-body system with a floating base and a particular hydrodynamic profile. In this paper, theorems on linear and angular momentum are used to establish the dynamic equations of motion of each rigid body and the effect of translational and rotational motion of internal masses on the attitude control are taken into consideration. In addition, due to the unique external shape with fixed wings and deflectable rudders and the dual-drive operation in thrust and glide modes, the approaches of building dynamic model of conventional AUV and hydrodynamic model of submarine are introduced, and the tailored dynamic equations of the hybrid glider are formulated. Moreover, the behaviors of motion in glide and thrust operation are analyzed based on the simulation and the feasibility of the dynamic model is validated by data from lake field trials. 展开更多
关键词 hybrid-driven underwater glider autonomous underwater vehicle dynamic modeling momentum theorem
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Double Multiple Streamtube Model and Numerical Analysis of Vertical Axis Wind Turbine 被引量:2
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作者 Habtamu Beri Yingxue Yao 《Energy and Power Engineering》 2011年第3期262-270,共9页
The present paper contributes to the modeling of unsteady flow analysis of vertical axis wind turbine (VAWT). Double multiple streamtube (DSMT) model was applied for the performance prediction of straight bladed fixed... The present paper contributes to the modeling of unsteady flow analysis of vertical axis wind turbine (VAWT). Double multiple streamtube (DSMT) model was applied for the performance prediction of straight bladed fixed pitch VAWT using NACA0018 airfoil at low wind speed. A moving mesh technique was used to investigate two-dimensional unsteady flow around the same VAWT model with NACA0018 airfoil modified to be flexible at 150 from the main blade axis of the turbine at the trailing edge located about 70 % of the blade chord length using fluent solving Reynolds average Navier-strokes equation. The results obtained from DMST model and the simulation results were then compared. The result shows that the CFD simulation with airfoil modified has shown better performance at low tip speed ratios for the modeled turbine. 展开更多
关键词 Wind TURBINE ACTUATOR DISK momentum model STREAM Tube VAWT CFD
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Coupling model for waves propagating over a porous seabed 被引量:1
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作者 C.C.Liao Z.Lin +1 位作者 Y.Guo D.-S.Jeng 《Theoretical & Applied Mechanics Letters》 CAS CSCD 2015年第2期85-88,共4页
The wave-seabed interaction issue is of great importance for the design of foundation around marine infrastructures. Most previous investigations for such a problem have been limited to uncoupled or one- way coupled m... The wave-seabed interaction issue is of great importance for the design of foundation around marine infrastructures. Most previous investigations for such a problem have been limited to uncoupled or one- way coupled methods connecting two separated wave and seabed sub models with the continuity of pressures at the seabed surface. In this study, a strongly coupled model was proposed to realize both wave and seabed processes in a same program and to calculate the wave fields and seabed response simultaneously. The information between wave fields and seabed fields were strongly shared and thus results in a more profound investigation of the mechanism of the wave-seabed interaction. In this letter, the wave and seabed models were validated with previous experimental tests. Then, a set of application of present model were discussed in prediction of the wave-induced seabed response. Numerical results show the wave-induced liquefaction area of coupled model is smaller than that of uncoupled model. 展开更多
关键词 Coupled model momentum source Internal wave-maker Seabed response Pore pressure Liquefaction
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基于约束跟随理论的动量轮倒立摆控制研究
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作者 管震涛 刘康 +2 位作者 张远辉 卜洋 付铎 《现代电子技术》 北大核心 2026年第1期108-116,共9页
在处理欠驱动系统的控制问题时,传统控制方法常常面临跟踪精度低、能效差和控制律复杂等挑战。针对动量轮倒立摆这一典型的欠驱动非线性系统,文中提出一种新颖的基于约束跟随理论的控制策略。与传统方法相比,该策略无需线性化处理,能够... 在处理欠驱动系统的控制问题时,传统控制方法常常面临跟踪精度低、能效差和控制律复杂等挑战。针对动量轮倒立摆这一典型的欠驱动非线性系统,文中提出一种新颖的基于约束跟随理论的控制策略。与传统方法相比,该策略无需线性化处理,能够充分利用系统的非线性特性,从而提升控制性能。首先建立了动量轮倒立摆的机械结构模型,并基于拉格朗日方程构建其动力学模型。通过将倒立摆的期望平衡角度设定为伺服约束,基于约束跟随理论推导出满足约束的力矩解析表达式,避免引入拉格朗日乘子等辅助变量。在Matlab/Simulink/Simscape环境中进行的仿真实验验证,以及基于ESP32控制核心的实验平台搭建,均证实了所提控制方法的有效性和优越性。与传统的线性二次调节器(LQR)控制方法相比,所提方法在控制效果上表现出显著优势。 展开更多
关键词 动量轮倒立摆 欠驱动系统 非线性系统 拉格朗日方程 动力学模型 约束跟随
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RELAXATION TIME LIMITS PROBLEM FOR HYDRODYNAMIC MODELS IN SEMICONDUCTOR SCIENCE 被引量:3
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作者 黎勇 《Acta Mathematica Scientia》 SCIE CSCD 2007年第2期437-448,共12页
In this article, two relaxation time limits, namely, the momentum relaxation time limit and the energy relaxation time limit are considered. By the compactness argument, it is obtained that the smooth solutions of the... In this article, two relaxation time limits, namely, the momentum relaxation time limit and the energy relaxation time limit are considered. By the compactness argument, it is obtained that the smooth solutions of the multidimensional nonisentropic Euler-Poisson problem converge to the solutions of an energy transport model or a drift diffusion model, respectively, with respect to different time scales. 展开更多
关键词 Hydrodynamic models nonisentropic Euler-Poisson momentum relaxation time limit energy relaxation time limit
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Theoretical Model Calculation for d+~8Li Reaction
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作者 HAN Yin-Lu GUO Hai-Rui ZHANG Yue ZHANG Jing-Shang 《Communications in Theoretical Physics》 SCIE CAS CSCD 2008年第8期463-467,共5页
Based on the theoretical models for light nuclei, the calculations of reaction cross sections and the angular distributions for d +^8Li reaction are performed. Since all of the particle emissions are from the compoun... Based on the theoretical models for light nuclei, the calculations of reaction cross sections and the angular distributions for d +^8Li reaction are performed. Since all of the particle emissions are from the compound nucleus to the discrete levels, the angular momentum coupling effect in pre-equilibrium mechanism is taken into account. The three- body break-up process and the recoil effect are involved. The theoretical calculated results are compared to existing experimental data. 展开更多
关键词 deuteron-induced reaction cross sections light nuclei of the 1p shell angular momentum andparity dependence exciton model improved Iwamoto-Harada model
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Transverse momentum and transverse mass distributions of charged hadrons produced in Au-Au collisions at high energies
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作者 刘福虎 《Chinese Physics B》 SCIE EI CAS CSCD 2008年第7期2458-2465,共8页
The transverse momentum distribution and the transverse mass distribution of charged hadrons produced in nucleus nucleus collisions at high energies are described by using a two-cylinder model. The results calculated ... The transverse momentum distribution and the transverse mass distribution of charged hadrons produced in nucleus nucleus collisions at high energies are described by using a two-cylinder model. The results calculated by the model are compared and found to be in agreement with the experimental data of the STAR and E895 Collaborations, measured in A^Au collisions at the relativistic heavy ion collider (RHIC) and alternating-gradient synchrotron (AGS) energies, respectively. In the energy range concerned, the excitation degree of emission source close to the central axis of cylinders increases obviously with the collision centrality and incident energy increasing, but it does not show any obvious change with the increase of the (pseudo)rapidity in central collisions. The excitation degree of emission source close to the side-surface of cylinders does not show any obvious change with the collision centrality, the (pseudo)rapidity, and the incident energy increasing. 展开更多
关键词 transverse momentum two-cylinder model nucleus-nucleus collisions
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Study on Stack Effect of Stairwell by Numerical Model of Leakage Flow through Gap of Door
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作者 Jung-Yup Kim Ji-Seok Kim 《Open Journal of Fluid Dynamics》 2013年第4期241-247,共7页
Since stack effect that occurs in high-rise buildings has an effect on the indoor environment of the buildings, energy loss and smoke control in case of a fire, there is a need to conduct research on this. For an anal... Since stack effect that occurs in high-rise buildings has an effect on the indoor environment of the buildings, energy loss and smoke control in case of a fire, there is a need to conduct research on this. For an analysis of the stack effect, analysis methods on the leakage flow through gap of interior door shall be formulated. Until now, studies related to the gap leakage flow in buildings have mainly analyzed flow field and pressure in the buildings one-dimensionally using pressure difference-leakage flowrate relations of Orifice Equation and a network numerical analysis algorithm that as- sumes each compartment in the buildings as a single point. In this study, the Momentum Loss Model which enables pressure drop to be proportional to the flow velocity through the gap of door in computational domain of 3-dimensional numerical analysis was proposed to reflect the gap flow phenomenon effectively in 3-dimensional numerical analysis. Using the proposed model, 3-dimensional numerical analysis of the stack effect on the stairs in buildings was performed, and the effects of separation door and lobby between stair and accommodation on the stack effect were investigated. 展开更多
关键词 STACK Effect LEAKAGE Flow GAP of DOOR momentum Loss model Separation DOOR NUMERICAL Analysis
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A Review on the Study of Continental Drift and Numerical Simulation Associated with the Early Earth Core-Magma Angular Momentum Exchange
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作者 Weihong Qian 《Open Journal of Geology》 2023年第9期980-1006,共27页
According to the drive of planetary-scale upper magma fluid motions associated with the core-magma angular momentum exchange in the early Earth’s interior, this paper reviewed the results of continental drift studied... According to the drive of planetary-scale upper magma fluid motions associated with the core-magma angular momentum exchange in the early Earth’s interior, this paper reviewed the results of continental drift studied over the last three decades. The theoretical speculation is in good fit to the traces of geological events left on the Earth’s surface. A northeastward drift directionality of the Australian, African, and South American continents relative to the Antarctica Continent in the Southern Hemisphere is reanalyzed according to the slowing down of the early Earth’s rotation. Six traces of significant back-and-forth drifts of the Australian and Asian continents left respectively on the Southwest and Northwest Pacific seafloors are reidentified according to the gradually decreasing amplitude of core-magma angular momentum exchange during early geological evolution. Finally, the thickening and shortening of different continents during the early drift processes are re-simulated by using a simple magma fluid dynamical model. 展开更多
关键词 Continental Drift Driving Force DIRECTIONALITY Numerical model Angular momentum Exchange
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The Investigation of Atmospheric Angular Momentum as a Contributor to Polar Wobble and Length of Day Change with AMIP II GCM Data 被引量:1
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作者 钟敏 闫昊明 朱耀仲 《Advances in Atmospheric Sciences》 SCIE CAS CSCD 2002年第2期287-296,共10页
The atmospheric angular momentum (AAM) functions in terms of contribution to polar wobble and length of day change, are calculated from the output data of GSM9603 global circulation model (GCM) of Japan Meteorological... The atmospheric angular momentum (AAM) functions in terms of contribution to polar wobble and length of day change, are calculated from the output data of GSM9603 global circulation model (GCM) of Japan Meteorological Agency (JMA), from the reanalysis data of the National Centers for the Environmental Prediction (NCEP)/National Center for Atmospheric Research (NCAR), and from the operational objective analysis data of JMA, respectively. The comparison shows that during the period from 1985 to 1995, the values of the pressure terms in the equatorial components of AAM functions calculated from three data sets agree with each other better along 90°E longitude than along Greenwich meridian direction. The axial component of relative AAM function estimated from GSM 9603 agrees well with those from the other two data sets in terms of seasonal variations with the moderate amplitudes, but not so well with the composite axial component of relative AAM functions estimated from 23 GCM models anticipating in the first phase of AMIP. In addition, its interannual variation from 1979 to 1996 shows the main characteristics of ENSO evolution, just as does the axial component of relative AAM function estimated from NCEP reanalysis data except for the period of anomalous ENSO from 1991 to 1993. 展开更多
关键词 Atmospheric model Inter–comparison Project (AMIP) Atmospheric Angular momentum (AAM) Earth rotation
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Intrinsic Spin Angular Momentum of Electron Relation to the Discrete Indivisible Quantum of Time Kshana or Moment
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作者 Shesharao M. Wanjerkhede 《Journal of Modern Physics》 2024年第9期1337-1352,共16页
The frequency of any periodic event can be defined in terms of units of Time. Planck constructed a unit of time called the Plank time from other physical constants. Vyasa defined a natural unit of time, kshana, or mom... The frequency of any periodic event can be defined in terms of units of Time. Planck constructed a unit of time called the Plank time from other physical constants. Vyasa defined a natural unit of time, kshana, or moment based on the motion of a fundamental particle. It is the time taken by an elementary particle, to change its direction from east to north. According to Vyasa, kshana is discrete, exceedingly small, indivisible, and is a constant time quantum. When the intrinsic spin angular momentum of an electron was related to the angular momentum of a simple thin circular plate, spherical shell, and solid sphere model of an electron, we found that the value of kshana in seconds was equal to ten to a power of minus twenty-one second. The disc model for the spinning electron provides an accurate value of the number of kshanas per second as determined previously and compared with other spinning models of electrons. These results indicate that the disk-like model of spinning electrons is the correct model for electrons. Vyasa’s definition of kshana opens the possibility of a new foundation for the theory of physical time, and perspectives in theoretical and philosophical research. 展开更多
关键词 Natural Time Unit Quantum Time Kshana Plank Time Intrinsic Angular momentum Thin Disc model Compton Wavelength
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基于改进BP神经网络的钢筋混凝土桥墩等效塑性铰长度预测模型研究
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作者 孙治国 刘云华 +2 位作者 刘瑜丽 张春辉 Uzdin A M 《防灾科技学院学报》 2025年第4期72-81,共10页
为提高钢筋混凝土桥墩等效塑性铰长度的预测精度,收集整理了133组钢筋混凝土桥墩抗震试验数据,构建了包含桥墩高度、截面尺寸、混凝土抗压强度、纵筋直径、纵筋屈服强度、纵筋配筋率、箍筋屈服强度、体积配箍率和轴压比等10个影响因素... 为提高钢筋混凝土桥墩等效塑性铰长度的预测精度,收集整理了133组钢筋混凝土桥墩抗震试验数据,构建了包含桥墩高度、截面尺寸、混凝土抗压强度、纵筋直径、纵筋屈服强度、纵筋配筋率、箍筋屈服强度、体积配箍率和轴压比等10个影响因素的数据集。在传统BP神经网络基础上,引入动量算法与RMSprop自适应学习率算法,建立了改进的BP神经网络预测模型,用以预测钢筋混凝土墩柱的等效塑性铰长度。为验证模型预测精度与样本量合理性,开展5次随机划分实验,结果显示各性能指标变异系数均小于15%, 133组样本量足以支撑稳定预测。将改进的BP神经网络预测模型与传统BP神经网络、动量BP神经网络及6种经验公式模型进行了对比分析,结果表明:改进BP神经网络模型在预测精度与稳定性方面均显著优于其他模型,能够更为准确地预测钢筋混凝土桥墩等效塑性铰长度。 展开更多
关键词 桥梁抗震 等效塑性铰长度 BP模型预测 动量 RMSprop算法
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JWST Discoveries—Confirmation of World-Universe Model Predictions
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作者 Vladimir S. Netchitailo 《Journal of High Energy Physics, Gravitation and Cosmology》 CAS 2022年第4期1134-1154,共21页
In 1937, P. Dirac proposed the Large Number Hypothesis and Hypothesis of Variable Gravitational Constant [1], and later added notion of Continuous Creation of Matter in the World [2]. Developed Hypersphere World-Unive... In 1937, P. Dirac proposed the Large Number Hypothesis and Hypothesis of Variable Gravitational Constant [1], and later added notion of Continuous Creation of Matter in the World [2]. Developed Hypersphere World-Universe Model (WUM) follows these ideas, albeit introducing different mechanism of Matter creation. Most direct observational evidence of validity of WUM are: 1) Microwave Background Radiation and Intergalactic Plasma speak in favor of existence of Medium;2) Laniakea Supercluster with binding mass ~10<sup>17</sup>M<sub>&odot;</sub> is home to Milky Way (MW) galaxy and ~10<sup>5</sup> other nearby galaxies, which did not start their movement from Initial Singularity (see Figure 1);3) MW is gravitationally bounded with Virgo Supercluster (VSC) and has Orbital Angular Momentum calculated based on distance of 65 Mly from VSC and orbital speed of ~400 km·s<sup>-1</sup>, which far exceeds rotational angular momentum of MW;4) Mass-to-light ratio of VSC is ~300 times larger than that of Solar ratio. Similar ratios are obtained for other superclusters (see Figure 2). These ratios are main arguments in favor of the presence of tremendous amounts of Dark Matter (DM) in the World. JWST discoveries confirm the most important predictions of WUM in 2018: 1) Absolute Age of World is 14.22 Gyr;2) Dark Epoch (spanning for Laniakea Supercluster (LSC) from the Beginning of World for 0.45 Gyr) when only DM Macroobjects (MOs) form and evolve;3) Luminous Epoch (ever since, 13.77 Gyr for LSC) when Luminous MOs (superclusters, galaxies, extrasolar systems, etc.) emerge;4) Transition from Dark Epoch to Luminous Epoch is due to Explosive Rotational Fission of Overspinning (surface speed at equator exceeding escape velocity) DM Supercluster’s Cores and self-annihilation of DM Particles (DMPs);5) MOs of World form from top (Superclusters) down to Galaxies and Extrasolar systems in parallel around different Cores made up of different DMPs;6) 3D Finite Boundless World presents a Patchwork Quilt of different Luminous Superclusters, which emerged in different places of World at different Cosmological times. 展开更多
关键词 James Webb Space Telescope World-Universe model Medium Angular momentum Dark Matter Dark Epoch Luminous Epoch Rotational Fission Patchwork Quilt Early-Galaxies Inter-Connectivity of Primary Cosmological Parameters
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Principal Role of Angular Momentum in Cosmology
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作者 Vladimir S. Netchitailo 《Journal of High Energy Physics, Gravitation and Cosmology》 2023年第4期984-1003,共20页
According to “Evolution Encyclopedia” (The Origin of the Solar System), “There is no possible means by which the angular momentum from the sun could be transferred to the planets”. Yet this is what would have to b... According to “Evolution Encyclopedia” (The Origin of the Solar System), “There is no possible means by which the angular momentum from the sun could be transferred to the planets”. Yet this is what would have to be done if any of the evolutionary theories of solar system origin are to be accepted. Scientists cannot account for this puzzling situation: less than one percent of the mass of the solar system is in the planets, while a staggering 98 percent of its angular momentum is in them. It simply does not fit into any of the cosmologies. Speaking of the mass-angular momentum problem, D. Bergamini says: “A theory of evolution that fails to account for this peculiar fact is ruled out before it starts” [1]. Angular Momentum problem is one of the most critical problems in Standard model that must be solved. To the best of our knowledge, the developed Hypersphere World-Universe Model (WUM) is only cosmological model in existence that is consistent with the Law of Conservation of Angular Momentum [2]. In the present paper, we discuss Angular Momenta of Solar System, Milky Way galaxy, and Superclusters in frames of WUM. 展开更多
关键词 Angular momentum Rotational Fission Multicomponent Dark Matter Macroobject Shell model Macroobjects Formation Solar System Milky Way SUPERCLUSTERS
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空间环境自由分子流与壁面动量适应系数研究
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作者 郭占平 商圣飞 +4 位作者 唐振宇 郑慧奇 章潜 李馨洁 贺碧蛟 《空间控制技术与应用》 北大核心 2025年第2期71-80,共10页
超低轨道飞行器已经成为空间技术领域的研究热点.在超低轨环境下,空间分子对飞行器产生的气动阻力会使飞行器速度衰减,从而需要频繁进行速度补偿.超低轨环境下的气体流动属于稀薄流动,气体分子与固体壁面的相互作用对气动阻力的评估至... 超低轨道飞行器已经成为空间技术领域的研究热点.在超低轨环境下,空间分子对飞行器产生的气动阻力会使飞行器速度衰减,从而需要频繁进行速度补偿.超低轨环境下的气体流动属于稀薄流动,气体分子与固体壁面的相互作用对气动阻力的评估至关重要.基于气固相互作用的Maxwell模型,重点开展了适应系数的评估研究.研究结果表明,超低轨空间分子流对卫星表面材料(聚酰亚胺)的正向入射适应系数为0.98,随着入射角度的增加呈下降趋势,变化区间约为0.67~0.98.通过圆柱绕流试验进行了气动力的校验,计算结果与试验结果吻合较好.本项研究可以为超低轨飞行器大气气动力和力矩仿真的适应系数选择提供参考. 展开更多
关键词 超低轨 空间大气 气动力 Maxwell模型 适应系数
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World-Universe Model—Alternative to Big Bang Model 被引量:1
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作者 Vladimir S. Netchitailo 《Journal of High Energy Physics, Gravitation and Cosmology》 2020年第1期133-158,共26页
This manuscript provides a comparison of the Hypersphere World-Universe Model (WUM) with the prevailing Big Bang Model (BBM) of the Standard Cosmology. The performed analysis of BBM shows that the Four Pillars of the ... This manuscript provides a comparison of the Hypersphere World-Universe Model (WUM) with the prevailing Big Bang Model (BBM) of the Standard Cosmology. The performed analysis of BBM shows that the Four Pillars of the Standard Cosmology are model-dependent and not strong enough to support the model. The angular momentum problem is one of the most critical problems in BBM. Standard Cosmology cannot explain how Galaxies and Extra Solar systems obtained their substantial orbital and rotational angular momenta, and why the orbital momentum of Jupiter is considerably larger than the rotational momentum of the Sun. WUM is the only cosmological model in existence that is consistent with the Law of Conservation of Angular Momentum. To be consistent with this Fundamental Law, WUM discusses in detail the Beginning of the World. The Model introduces Dark Epoch (spanning from the Beginning of the World for 0.4 billion years) when only Dark Matter Particles (DMPs) existed, and Luminous Epoch (ever since for 13.8 billion years). Big Bang discussed in Standard Cosmology is, in our view, transition from Dark Epoch to Luminous Epoch due to Rotational Fission of Overspinning Dark Matter (DM) Supercluster’s Cores. WUM envisions Matter carried from the Universe into the World from the fourth spatial dimension by DMPs. Ordinary Matter is a byproduct of DM annihilation. WUM solves a number of physical problems in contemporary Cosmology and Astrophysics through DMPs and their interactions: Angular Momentum problem in birth and subsequent evolution of Galaxies and Extrasolar systems—how do they obtain it;Fermi Bubbles—two large structures in gamma-rays and X-rays above and below Galactic center;Diversity of Gravitationally-Rounded Objects in Solar system;some problems in Solar and Geophysics [1]. WUM reveals Inter-Connectivity of Primary Cosmological Parameters and calculates their values, which are in good agreement with the latest results of their measurements. 展开更多
关键词 Big Bang model Four Pillars of Standard Cosmology ANGULAR momentum Problem Black Holes Hypersphere World-Universe model Multicomponent DARK MATTER Macroobjects Structure Law of Conservation of ANGULAR momentum Medium of the World Inter-Connectivity of Primary Cosmological Parameters The Beginning of the World DARK EPOCH Rotational Fission Luminous EPOCH Macroobject Shell model DARK MATTER Core Gravitational Burst Intergalactic Plasma Microwave Background Radiation Far-Infrared Background Radiation Emergent Phenomena CODATA
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弯扭耦合效应下风力机叶片预弯后掠对其气弹载荷影响的分析
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作者 马新稳 孙敬伟 +1 位作者 陈严 彭响华 《太阳能学报》 北大核心 2025年第9期1-10,共10页
为研究风力机柔性叶片预弯和不同后掠几何外形设计对其气弹载荷的影响,利用转动矩阵精确地表征叶素处的气流速度和叶素的位移、方向、振动速度,并对叶素动量模型进行修正建立气弹仿真模型。基于DTU10MW叶片分别设计3种不同后掠叶片,对3... 为研究风力机柔性叶片预弯和不同后掠几何外形设计对其气弹载荷的影响,利用转动矩阵精确地表征叶素处的气流速度和叶素的位移、方向、振动速度,并对叶素动量模型进行修正建立气弹仿真模型。基于DTU10MW叶片分别设计3种不同后掠叶片,对3种叶片进行静力学、动力学和气弹耦合分析。研究叶片弯扭耦合变形对叶片攻角的影响,叶片预弯、后掠引起的气动力臂增大对叶根扭矩的影响。研究发现叶片的弯扭耦合效应受叶片的几何外形影响较大,后掠叶片对降低叶根的挥舞疲劳载荷效果最好,达到-11.14%,但会大幅增大叶根扭转疲劳载荷,预弯叶片会减小叶根的挥舞和扭转疲劳载荷。 展开更多
关键词 风力机叶片 气动弹性 疲劳载荷 叶素动量模型修正 弯扭耦合
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