Whistler wave propagation and interplay between electron inertia and Larmor radius effects

2019 ◽  
Vol 26 (4) ◽  
pp. 042106 ◽  
Author(s):  
Garima Joshi ◽  
G. Ravi ◽  
S. Mukherjee
2006 ◽  
Vol 74 (4) ◽  
pp. 425-438 ◽  
Author(s):  
A V Kudrin ◽  
V A Es'kin

1984 ◽  
Vol 31 (2) ◽  
pp. 197-208 ◽  
Author(s):  
R. W. Boswell

The dispersion of the radial eigenmodes of a cylindrical m = 1 whistler wave with Ωi; ≪ ω < Ωe ≪ ωpe is investigated for both conducting and insulating boundaries. The effects of electron inertia and resistivity on the modes are discussed.


Author(s):  
Redouane Mecheri ◽  
Eckart Marsch

We study wave propagation in the low-β coronal plasma using a collisionless multi-fluid model. Neglecting the electron inertia, this model allows us to take into account ion-cyclotron wave effects that are absent in the magnetohydrodynamics model. To accomplish this, we perform a Fourier plane-wave perturbation analysis. Solving numerically the dispersion relations obtained from a two- and three-fluid model, dispersion curves for representative parameters of the solar corona are presented. The results reveal the presence of resonance frequencies that might play a role in coronal heating.


1977 ◽  
Vol 20 (11) ◽  
pp. 1960 ◽  
Author(s):  
B. D. McVey ◽  
J. E. Scharer

2018 ◽  
Vol 84 (4) ◽  
Author(s):  
E. Tassi ◽  
D. Grasso ◽  
D. Borgogno ◽  
T. Passot ◽  
P. L. Sulem

An electromagnetic reduced gyrofluid model for collisionless plasmas, accounting for electron inertia, finite ion Larmor radius effects and Landau-fluid closures for the electron fluid is derived by means of an asymptotic expansion from a parent gyrofluid model. In the absence of terms accounting for Landau damping, the model is shown to possess a non-canonical Hamiltonian structure. The corresponding Casimir invariants are derived and use is made thereof, in order to obtain a set of normal field variables, in terms of which the Poisson bracket and the model equations take a remarkably simple form. The inclusion of perpendicular temperature fluctuations generalizes previous Hamiltonian reduced fluid models and, in particular, the presence of ion perpendicular gyrofluid temperature fluctuations reflects into the presence of two new Lagrangian invariants governing the ion dynamics. The model is applied, in the cold-ion limit, to investigate numerically a magnetic reconnection problem. The Landau damping terms are shown to reduce, by decreasing the electron temperature fluctuations, the linear reconnection rate and to delay the nonlinear island growth. The saturated island width, on the other hand, is independent of Landau damping. The fraction of magnetic energy converted into perpendicular kinetic energy also appears to be unaffected by the Landau damping terms, which, on the other hand, dissipate parallel kinetic energy as well as free energy due to density and electron temperature fluctuations.


2005 ◽  
Vol 33 (2) ◽  
pp. 637-646 ◽  
Author(s):  
W.E. Amatucci ◽  
D.D. Blackwell ◽  
D.N. Walker ◽  
G. Gatling ◽  
G. Ganguli

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