scholarly journals Robust Finite Volume Schemes for Two-Fluid Plasma Equations

2013 ◽  
Vol 60 (3) ◽  
pp. 584-611 ◽  
Author(s):  
Remi Abgrall ◽  
Harish Kumar
2019 ◽  
Vol 239 ◽  
pp. 16-32 ◽  
Author(s):  
Isaac Alonso Asensio ◽  
Alejandro Alvarez Laguna ◽  
Mohamed Hassanine Aissa ◽  
Stefaan Poedts ◽  
Nataly Ozak ◽  
...  

2012 ◽  
Vol 12 (4) ◽  
pp. 1070-1095 ◽  
Author(s):  
Shamsul Qamar ◽  
Munshoor Ahmed ◽  
Ishtiaq Ali

AbstractThe space-time conservation element and solution element (CE/SE) method is proposed for solving a conservative interface-capturing reduced model of compressible two-fluid flows. The flow equations are the bulk equations, combined with mass and energy equations for one of the two fluids. The latter equation contains a source term for accounting the energy exchange. The one and two-dimensional flow models are numerically investigated in this manuscript. The CE/SE method is capable to accurately capture the sharp propagating wavefronts of the fluids without excessive numerical diffusion or spurious oscillations. In contrast to the existing upwind finite volume schemes, the Riemann solver and reconstruction procedure are not the building block of the suggested method. The method differs from the previous techniques because of global and local flux conservation in a space-time domain without resorting to interpolation or extrapolation. In order to reveal the efficiency and performance of the approach, several numerical test cases are presented. For validation, the results of the current method are compared with other finite volume schemes.


2018 ◽  
Vol 231 ◽  
pp. 31-44 ◽  
Author(s):  
A. Alvarez Laguna ◽  
N. Ozak ◽  
A. Lani ◽  
H. Deconinck ◽  
S. Poedts

1982 ◽  
Vol 28 (2) ◽  
pp. 193-214 ◽  
Author(s):  
Qiu Xiaoming ◽  
R. Balescu

In this paper we generalize the formalism developed by Balescu and Paiva-Veretennicoff, valid for any kind of weak turbulence, for the determination of all the transport coefficients of an unmagnetized turbulent plasma, to the case of a magnetized one, and suggest a technique to avoid finding the inverse of the turbulent collision operator. The implicit plasmadynamical equations of a two-fluid plasma are presented by means of plasmadynamical variables. The anomalous transport coefficients appear in their natural places in these equations. It is shown that the necessary number of transport coefficients for describing macroscopically the magnetized turbulent plasma does not exceed the number for the unmagnetized one. The typical turbulent and gyromotion terms, representing dissipative effects peculiar to the magnetized system, which contribute to the frequency-dependent transport coefficients are clearly exhibited.


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