Application of subtracted bi-Maxwellian distribution function in propagation of electron cyclotron waves in magnetospheric plasma of an outer planet

Optik ◽  
2020 ◽  
Vol 219 ◽  
pp. 164629
Author(s):  
Suresh Chandra ◽  
Mohit Kumar Sharma
Keyword(s):  
Distribution Function ◽  
Electron Cyclotron ◽  
Magnetospheric Plasma ◽  
Maxwellian Distribution ◽  
Outer Planet ◽  
Maxwellian Distribution Function ◽  
Electron Cyclotron Waves

Weakly relativistic dielectric tensor in the presence of temperature anisotropy

1990 ◽  
Vol 44 (2) ◽  
pp. 319-335 ◽  
Author(s):  
M. Bornatici ◽  
G. Chiozzi ◽  
P. de Chiara
Keyword(s):  
Distribution Function ◽  
Cyclotron Frequency ◽  
Electron Cyclotron ◽  
Maxwellian Distribution ◽  
Larmor Radius ◽  
Dielectric Tensor ◽  
Temperature Anisotropy ◽  
Finite Larmor Radius ◽  
Maxwellian Distribution Function ◽  
Analytical Expressions

Analytical expressions for the weakly relativistic dielectric tensor near the electron-cyclotron frequency and harmonies are obtained to any order in finite-Larmor-radius effects for a bi-Maxwellian distribution function. The dielectric tensor is written in ternis of generalized Shkarofsky dispersion functions, whose properties are well known. Relevant limiting cases are considered and, in particular, the anti-Hermitian part of the (fully relativistic) dielectric tensor is evaluated for two cases of strong temperature anisotropy.

The Drifted Maxwellian Distribution Function in InSb

1967 ◽  
Vol 20 (2) ◽  
pp. K135-K139 ◽  
Author(s):  
G. Jones ◽  
G. Smith ◽  
A. R. Beattle
Keyword(s):  
Distribution Function ◽  
Maxwellian Distribution ◽  
Maxwellian Distribution Function

The Excitation Equilibrium in the Solar Corona and Non-Maxwellian Electron Distributions

1994 ◽  
Vol 144 ◽  
pp. 435-438
Author(s):  
E. Dzifčáková
Keyword(s):  
Distribution Function ◽  
Solar Corona ◽  
Maxwellian Distribution ◽  
Collisional Excitation ◽  
Excitation Coefficient ◽  
Electron Distributions ◽  
Maxwellian Distribution Function ◽  
Excitation Equilibrium

AbstractWe demonstrate the influence of an electron non-Maxwellian distribution function on the collisional excitation coefficient and, as an example, on the excitation equilibrium of Fe XIV in the solar corona. The results can be used for specific applications in the solar corona, especially in the active corona, where deviations from Maxwellian distribution can be significant.

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