Electron inertia effect on small amplitude solitons in a weakly relativistic two-fluid plasma

2005 ◽  
Vol 12 (5) ◽  
pp. 052103 ◽  
Author(s):  
Khushvant Singh ◽  
Vinod Kumar ◽  
Hitendra K. Malik
1978 ◽  
Vol 20 (2) ◽  
pp. 281-287 ◽  
Author(s):  
S. Hyun ◽  
C. F. Kennel

Using the two-fluid approximation, we summarize properties of linear waves in an unbounded magnetized relativistic plasma by a parameter-space diagram of wave phase velocity: a relativistic plasma pond.


2005 ◽  
Vol 12 (7) ◽  
pp. 072302 ◽  
Author(s):  
Khushvant Singh ◽  
Vinod Kumar ◽  
Hitendra K. Malik

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.


2012 ◽  
Author(s):  
Ross H. Burrows ◽  
Xianzhi Ao ◽  
Gary P. Zank

2021 ◽  
Vol 87 (4) ◽  
Author(s):  
Y. Nakajima ◽  
H. Himura ◽  
A. Sanpei

We derive the two-dimensional counter-differential rotation equilibria of two-component plasmas, composed of both ion and electron ( $e^-$ ) clouds with finite temperatures, for the first time. In the equilibrium found in this study, as the density of the $e^{-}$ cloud is always larger than that of the ion cloud, the entire system is a type of non-neutral plasma. Consequently, a bell-shaped negative potential well is formed in the two-component plasma. The self-electric field is also non-uniform along the $r$ -axis. Moreover, the radii of the ion and $e^{-}$ plasmas are different. Nonetheless, the pure ion as well as $e^{-}$ plasmas exhibit corresponding rigid rotations around the plasma axis with different fluid velocities, as in a two-fluid plasma. Furthermore, the $e^{-}$ plasma rotates in the same direction as that of $\boldsymbol {E \times B}$ , whereas the ion plasma counter-rotates overall. This counter-rotation is attributed to the contribution of the diamagnetic drift of the ion plasma because of its finite pressure.


Author(s):  
Y. Li ◽  
R. Samtaney ◽  
W. Cheng ◽  
V. Wheatley ◽  
Daryl Bond

Sign in / Sign up

Export Citation Format

Share Document