Quasiadiabatic dynamics of charged particles in a space plasma
L.M. Zelenyia,
A.I. Neishtadta,b,
A.V. Artemyeva,c,
D.L. Vainchteina,d,
H.V. Malovaa,c aSpace Research Institute, Russian Academy of Sciences, Profsoyuznaya str. 84/32, Moscow, 117997, Russian Federation bDepartment of Mathematical Sciences, Loughborough University, Loughborough, United Kingdom cLomonosov Moscow State University, Skobeltsyn Institute of Nuclear Physics, Leninskie Gory 1 build. 2, Moscow, 119991, Russian Federation dTemple University, Department of Mechanical Engineering, 1947 North 12th St, Philadelphia, Pennsylvania, 19122, USA
In many space plasma systems, especially when the magnetic field is weak, characteristic scales of the inhomogeneities of the magnetic field are much smaller than the Larmor radius of the ions. Over the last two decades there has been active development of quasiadiabatic models of the dynamics of charged particle in such systems. In this paper, we systematically review the quasiadiabatic approximation and illustrate how it can be used to describe various phenomena in the Earth magnetosphere and to explain many effects observed by satellites.
PT Journal Article
TI Quasiadiabatic dynamics of charged particles in a space plasma
AU Zelenyi L M
FAU Zelenyi LM
AU Neishtadt A I
FAU Neishtadt AI
AU Artemyev A V
FAU Artemyev AV
AU Vainchtein D L
FAU Vainchtein DL
AU Malova H V
FAU Malova HV
DP 10 Apr, 2013
TA Phys. Usp.
VI 56
IP 4
PG 347-394
RX 10.3367/UFNe.0183.201304b.0365
URL https://ufn.ru/en/articles/2013/4/b/
SO Phys. Usp. 2013 Apr 10;56(4):347-394
Received: 5th, May 2012, accepted: 18th, June 2012