Phase space of a two-dimensional model of a Parker dynamo


Cite item

Full Text

Open Access Open Access
Restricted Access Access granted
Restricted Access Subscription Access

Abstract

The dependences of the magnetic-field strength, variations of the magnetic field, and the multipole level on the amplitudes of the α and ω effects are considered using a two-dimensional model for a Parker dynamo in a spherical layer. Calculations have been carried out for both traditional spatial distributions of α and ω and geostrophic regimes obtained from three-dimensional modeling of thermal convection. Two-dimensional distributions of the dynamo-wave velocities in the zone where magnetic field is generated are presented. Comparisons with the solar and planetary dynamos are considered.

About the authors

M. Yu. Reshetnyak

Schmidt Intitute of Terrestrial Physics; Pushkov Institute of Terrestrial Magnetism, the Ionosphere and Radio Wave Propagation

Author for correspondence.
Email: m.reshetnyak@gmail.com
Russian Federation, Moscow; Troitsk, Moscow, 142190

Supplementary files

Supplementary Files
Action
1. JATS XML

Copyright (c) 2016 Pleiades Publishing, Ltd.