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About Exact Solution Of The Kinetic Equation For Current Sheath

2011/01/31 by V.V. Lyahov, Lyahov, V. V., V.M. Neshchadim +1
Earth and Planetary Sciences · Physics and Astronomy · #Earth and Planetary Astrophysics (astro-ph.EP) #Earthquake Detection and Analysis #FOS: Physical sciences #Ionosphere and magnetosphere dynamics #Lightning and Electromagnetic Phenomena #Plasma Physics (physics.plasm-ph)

paper · pdf · doi:10.48550/arxiv.1101.5988

openalex publication_date 2011/01/31 · openalex created_date 2025/10/10 · openalex updated_date 2026/07/28

Abstract

In the offered paper the kinetic theory of equilibrium and stability of the nonelectroneutral current sheaths formed at arbitrary values of medium parameters was developed. Equilibrium distribution function of a current sheath (Harris's function) considering anisotropy of temperature of plasma along and across the layers is summarized. The procedure of examination of a current sheath stability with due regard to plasma polarization effect is offered. Tensor of dielectric permeability is calculated and dispersion equation for investigation of possible instability modes of non-electroneutral current sheath is derived. Non-electroneutral equilibrium solution for a current sheath in the magnetospheric tail is derived and its instability is explored. A possible mechanism of magnetic field annihilation in the magnetospheric tail and acceleration of charged particles in the process of magnetospheric substorm development is considered.

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