Current results on the asymptotics of dynamo models

被引：6
|
作者：
Popova, H. P. [1 ,2 ]
机构：
[1] Lomonosov Moscow State Univ, Fac Phys, Leninskie Gory 1,Str 2, Moscow 119991, Russia
[2] Skobeltsyn Inst Nucl Phys, Leninskie Gory 1,Str 2, Moscow 119991, Russia
来源：
PHYSICS-USPEKHI | 2016年 / 59卷 / 06期
基金：
俄罗斯科学基金会;
关键词：
dynamo theory; Sun; stars; galaxies; ALPHA-OMEGA-DYNAMO; SCALE MAGNETIC-FIELDS; MERIDIONAL CIRCULATION; SOLAR DYNAMO; DIFFERENTIAL ROTATION; ALPHA(2)OMEGA-DYNAMO WAVES; POLARIZATION MEASUREMENTS; GALACTIC DYNAMOS; SPIRAL GALAXIES; MAUNDER MINIMUM;
D O I：
10.3367/UFNe.2016.02.037727
中图分类号：
O4 [物理学];
学科分类号：
0702 ;
摘要：
Magnetic field generation and evolution models that are capable of describing a large body of observational material are currently available for different celestial bodies. Despite recent decades of great success in numerical magnetic hydrodynamics and in detailed research into some specific problems, asymptotic methods still have 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.
引用
收藏
页码：513 / 530
页数：18
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