Current results on the asymptotics of dynamo models

E.P. Popova^a, b
^aLomonosov Moscow State University, Faculty of Physics, Leninskie Gory 1 build. 2, Moscow, 119991, Russian Federation
^bLomonosov Moscow State University, Skobeltsyn Institute of Nuclear Physics, Leninskie Gory 1 build. 2, Moscow, 119991, Russian Federation

Magnetic field generation and evolution models are currently available for different celestial bodies that are capable of describing a large body of observational material. Despite recent decades of great successes in numerical magnetic hydrodynamics and in detailed research into some specific problems, asymptotic methods still need to be used to clarify the magnetic field generation mechanism in dynamo theory. In this review, current asymptotic methods are presented together with the results of their application to the simulation of solar, stellar and galactic magnetic activities.

Keywords: dynamo theory, Sun, stars, galaxies
PACS: 52.30.Cv, 96.60.Hv, 96.60.Q− (all)
DOI: 10.3367/UFNe.2016.02.037727
URL: https://ufn.ru/en/articles/2016/6/a/
Web of Science

000386349400001
Scopus

2-s2.0-84987653261
ADS NASA

2016PhyU...59..513P
Citation: Popova E P "Current results on the asymptotics of dynamo models" Phys. Usp. 59 513–530 (2016)

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Received: 15th, May 2015, revised: 8th, February 2016, accepted: 12th, February 2016

Оригинал: Попова Е П «Cовременные результаты асимптотических исследований моделей динамо» УФН 186 577–596 (2016); DOI: 10.3367/UFNr.2016.02.037727

References (194) Cited by (7) Similar articles (20) ↓

A.Z. Dolginov “Origin of the magnetic fields of the earth and celestial bodies” 30 475–493 (1987)
Ya.B. Zeldovich, A.A. Ruzmaikin “The hydromagnetic dynamo as the source of planetary, solar, and galactic magnetism” 30 494–506 (1987)
S.I. Vainshtein, Ya.B. Zel’dovich “Origin of Magnetic Fields in Astrophysics (Turbulent ’Dynamo’ Mechanisms)” 15 159–172 (1972)
B.P. Filippov “Mass ejections from the solar atmosphere” 62 847–864 (2019)
A.G. Zhilkin, D.V. Bisikalo, A.A. Boyarchuk “Flow structure in magnetic close binary stars” 55 115–136 (2012)
A.B. Severnyi “Magnetic fields of the Sun and stars” 9 1–30 (1966)
A.M. Bykov, I.N. Toptygin “Particle kinetics in highly turbulent plasmas (renormalization and self-consistent field methods)” 36 (11) 1020–1052 (1993)
V.I. Krasovskii “Some results of igy and igc research on the aurora and night glow” 4 904–918 (1962)
T.V. Tropin, Ju.W.P. Schmelzer, V.L. Aksenov “Modern aspects of the kinetic theory of glass transition” 59 42–66 (2016)
A.A. Chernyshov, K.V. Karelsky, A.S. Petrosyan “Subgrid-scale modeling for the study of compressible magnetohydrodynamic turbulence in space plasmas” 57 421–452 (2014)
D.V. Bisikalo, V.I. Shematovich et al “Gas envelopes of exoplanets—hot Jupiters” 64 747–800 (2021)
V.N. Lukash, E.V. Mikheeva, A.M. Malinovsky “Formation of the large-scale structure of the Universe” 54 983–1005 (2011)
P.G. Frick, D.D. Sokoloff, R.A. Stepanov “Wavelets for the space-time structure analysis of physical fields” 65 62–89 (2022)
A.Yu. Potekhin “The physics of neutron stars” 53 1235–1256 (2010)
V.V. Uchaikin, A.D. Erlykin, R.T. Sibatov “Nonlocal (fractional-differential) model of cosmic ray transport in the interstellar medium” 66 221–262 (2023)
E.I. Kut’in, V.L. Lorman, S.V. Pavlov “Methods of the theory of singularities in the phenomenology of phase transitions” 34 (6) 497–514 (1991)
S.B. Pikel’ner “Dynamics of the solar atmosphere” 9 236–250 (1966)
V.L. Ginzburg, S.I. Syrovatskii “Present status of the question of the origin of cosmic rays” 3 504–541 (1961)
V.V. Klinshov, V.I. Nekorkin “Synchronization of delay-coupled oscillator networks” 56 1217–1229 (2013)
Yu.A. Shchekinov, E.O. Vasiliev, B.M. Shustov “Initial episodes of the chemical evolution of the intergalactic medium” 66 1071–1094 (2023)

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