Quasiadiabatic dynamics of charged particles in a space plasma

L.M. Zelenyi^a, A.I. Neishtadt^a, b, A.V. Artemyev^a, c, D.L. Vainchtein^a, d, H.V. Malova^a, 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.

PACS: 52.20.Dq, 52.40.Kh, 94.05.−a (all)
DOI: 10.3367/UFNe.0183.201304b.0365
URL: https://ufn.ru/en/articles/2013/4/b/
Web of Science

000321510400002
ADS NASA

2013PhyU...56..347Z
Citation: Zelenyi L M, Neishtadt A I, Artemyev A V, Vainchtein D L, Malova H V "Quasiadiabatic dynamics of charged particles in a space plasma" Phys. Usp. 56 347–394 (2013)

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Received: 5th, May 2012, accepted: 18th, June 2012

Оригинал: Зелёный Л М, Нейштадт А И, Артемьев А В, Вайнштейн Д Л, Малова Х В «Квазиадиабатическое описание динамики заряженных частиц в космической плазме» УФН 183 365–415 (2013); DOI: 10.3367/UFNr.0183.201304b.0365

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