Erratum: “Primal Macro-Projective Integration Method for Multi-Scale Plasma Simulation” [Plasma Fusion Res. 3, 021 (2008)]

2009 ◽  
Vol 4 ◽  
pp. 056-056 ◽  
Author(s):  
Miloš M. ŠKORIĆ ◽  
Aleksandra MALUCKOV ◽  
Seiji ISHIGURO
2008 ◽  
Vol 3 ◽  
pp. 021-021 ◽  
Author(s):  
Miloš M. ŠKORIĆ ◽  
Aleksandra MALUCKOV ◽  
Seiji ISHIGURO

1991 ◽  
Vol 96 (1) ◽  
pp. 54-70 ◽  
Author(s):  
A Friedman ◽  
S.E Parker ◽  
S.L Ray ◽  
C.K Birdsall

2017 ◽  
Vol 22 (5) ◽  
pp. 1175-1223 ◽  
Author(s):  
Chang Liu ◽  
Kun Xu

AbstractAs a continuation of developing multiscale method for the transport phenomena, a unified gas kinetic scheme (UGKS) for multi-scale and multi-component plasma simulation is constructed. The current scheme is a direct modeling method, where the time evolution solutions from the Vlasov-BGK equations of electron and ion and the Maxwell equations are used to construct a scale-dependent plasma simulation model. The modeling scale used in the UGKS is the mesh size scale, which can be comparable to or much larger than the local mean free path. As a result, with the variation of modeling scales in space and time through the so-called cell's Knudsen number and normalized Larmor radius, the discretized governing equations can recover a wide range of plasma evolution from the Vlasov equation in the kinetic scale to different-type of magnetohydrodynamic (MHD) equations in the hydrodynamic scale. The UGKS provides a general evolution model, which goes to the Vlasov equation in the kinetic scale and many types of MHD equations in the hydrodynamic scale, such as the two fluids model, the Hall, the resistive, and the ideal MHD equations. All current existing governing equations become the subsets of the UGKS, and the UGKS bridges these distinguishable governing equations seamlessly. The construction of UGKS is based on the implementation of physical conservation laws and the un-splitting treatment of particle collision, acceleration, and transport in the construction of a scale-dependent numerical flux across a cell interface. At the same time, the discretized plasma evolution equations are coupled with the Maxwell equations for electro-magnetic fields, which also cover a scale-dependent transition between the Ampére's law and the Ohm's law for the calculation of electric field. The time step of UGKS is not limited by the relaxation time, the cyclotron period, and the speed of light in the ideal-MHD regime. Our scheme is able to give a physically accurate solution for plasma simulation with a wide range of Knudsen number and normalized Larmor radius. It can be used to study the phenomena from the Vlasov limit to the scale of plasma skin depth for the capturing of two-fluid effect, and the phenomena in the plasma transition regime with a modest Knudsen number and Larmor radius. The UGKS is validated by numerical test cases, such as the Landau damping and two stream instability in the kinetic regime, and the Brio-Wu shock tube problem, and the Orszag-Tang MHD turbulence problem in the hydrodynamic regime. The scheme is also used to study the geospace environment modeling (GEM), such as the challenging magnetic reconnection problem in the transition regime. At the same time, the magnetic reconnection mechanism of the Sweet-Parker model and the Hall effect model can be connected smoothly through the variation of Larmor radius in the UGKS simulations. Overall, the UGKS is a physically reliable multi-scale plasma simulation method, and it provides a powerful and unified approach for the study of plasma physics.


2021 ◽  
Vol 12 (2) ◽  
pp. 701-714
Author(s):  
Xigui Wang ◽  
Siyuan An ◽  
Yongmei Wang ◽  
Jiafu Ruan ◽  
Baixue Fu

Abstract. This study conducts an analytical investigation of the dynamic response characteristics of a two-stage series composite system (TsSCS) with a planetary transmission consisting of dual-power branches. An improved incremental harmonic balance (IHB) method, which solves the closed solution of incremental parameters passing through the singularity point of the analytical path, based on the arc length extension technique, is proposed. The results are compared with those of the numerical integration method to verify the feasibility and effectiveness of the improved method. Following that, the multi-scale perturbation (MsP) method is applied to the TsSCS proposed in this subject to analyze the parameter excitation and gap nonlinear equations and then to obtain the analytical frequency response functions including the fundamental, subharmonic, and superharmonic resonance responses. The frequency response equations of the primary resonance, subharmonic resonance, and superharmonic resonance are solved to generate the frequency response characteristic curves of the planetary gear system (PGS) in this method. A comparison between the results obtained by the MsP method and the numerical integration method proves that the former is ideal and credible in most regions. Considering the parameters of TsSCS excitation frequency and damping, the nonlinear response characteristics of steady-state motion are mutually converted. The effects of the time-varying parameters and the nonlinear deenthing caused by the gear teeth clearance on the amplitude–frequency characteristics of TsSCS components are studied in this special topic.


2012 ◽  
Vol 203 ◽  
pp. 432-437
Author(s):  
Jun Jie Zhao ◽  
Yan Zhi Yang

The global integration time step of multi-scale model is subject to local detailed model, resulting in lower computational efficiency. Mixed time integration method uses different integration time-step in different scale model, it can effectively avoid the above problem. Rest on a large-scale water tunnel under construction, in order to achieve the synchronization of the global and the local simulation, the paper establishes multi-scale finite element model of the tunnel, and calculate it by mixed time integration method. The final calculation and analysis show that the algorithm can guarantee the computational accuracy of multi-scale numerical simulation, and can effectively improve the computational efficiency, it can also provide references for related tunnel project.


1993 ◽  
Vol 107 (2) ◽  
pp. 388-402 ◽  
Author(s):  
S.E. Parker ◽  
A. Friedman ◽  
S.L. Ray ◽  
C.K. Birdsall

2012 ◽  
Vol 116 (8) ◽  
pp. 882-895 ◽  
Author(s):  
Rafael F.V. Saracchini ◽  
Jorge Stolfi ◽  
Helena C.G. Leitão ◽  
Gary A. Atkinson ◽  
Melvyn L. Smith

1990 ◽  
Vol 91 (1) ◽  
pp. 252
Author(s):  
A Friedman ◽  
S.E Parker ◽  
S.L Ray ◽  
C.K Birdsall

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