scholarly journals Multi-temperature generalized Zhdanov closure for scrape-off layer/edge applications

Author(s):  
Madhusudan Raghunathan ◽  
Yannick Marandet ◽  
Hugo Bufferand ◽  
Guido Ciraolo ◽  
Philippe Ghendrih ◽  
...  

Abstract The derivation of the multi-temperature generalized Zhdanov closure is provided starting from the most general form of the left hand side of the moment averaged kinetic equation with the Sonine-Hermite polynomial ansatz for an arbitrary number of moments. The process of arriving at the reduced higher-order moment equations, with its assumptions and approximations, is explicitly outlined. The generalized multi-species, multi-temperature coefficients from the authors' previous article are used to compute values of higher order moments such as heat flux in terms of the lower order moments. Transport coefficients and the friction and thermal forces for magnetic confinement fusion relevant cases with the generalized coefficients are compared to the scheme with the single-temperature coefficients previously provided by Zhdanov et al. It is found that the 21N-moment multi-temperature coefficients are adequate for most cases relevant to fusion. Furthermore, the 21N-moment scheme is also tested against the trace approximation to determine the range of validity of the trace approximation with respect to fusion relevant plasmas. Possible refinements to the closure scheme are illustrated as well, in order to account for quantities which might be significant in certain schemes such as the drift approximation.

1980 ◽  
Vol 91 ◽  
pp. 459-474
Author(s):  
S. Cuperman

Three ways to improve the theory and therefore the understanding of the physical processes in the interplanetary medium (during both quiet and disturbed periods of solar activity) are suggested. They are: (1) the development and consequently the use of higher order moments (fluid) equations as well as of more realistic closure conditions and transport coefficients for the macroscopic description of the solar wind ; (2) the undertaking of computer simulation experiments on the nonlinear collective relaxation process through particle-wave-particle interaction due to the plasma electromagnetic instabilities which may develop under conditions prevailing in the solar wind; and (3) the consideration of collective interactions in the evaluation of the transport coefficients, as deduced from the quasi-linear theory and computer simulation experiments, and their incorporation into the higher order moment equations.


Metaphysics ◽  
2020 ◽  
pp. 102-114
Author(s):  
A. M Panichev

The cycle of experiments with free-rolling gyroscopes at different angular velocity intervals including those on scales with continuous-discrete weight registration was carried out. We concluded that the free-running time of gyroscopes in one interval of angular velocities can vary greatly (within hundreds of percent). Measuring the free running time of a gyroscope during a solar eclipse has shown a connection between registered fluctuations in the gyroscope behavior and the eclipse stroke. The data obtained during the periods of sunrise indicate that the gyroscope can react at the moment of the sunrise while recording the true ascent, as well as the ascent preceding the true one with a difference of 8 minutes. Statistical analysis of the graphs of weight changes of the disk at right and left-hand free rotation in the speed range from 5000 to 250 rpm showed that the abnormal weight changes recorded at certain “critical” frequencies with different directions of rotation reliably differ in amplitude characteristics.


Author(s):  
Mahdi Pourrafiee ◽  
AmirHossein Nafei ◽  
Shokoufe Banihashemi ◽  
S. Pourmohammad Azizi

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