Astrophysical magnetic fields and nonlinear dynamo theory

A Brandenburg, K Subramanian - Physics Reports, 2005 - Elsevier
The current understanding of astrophysical magnetic fields is reviewed, focusing on their
generation and maintenance by turbulence. In the astrophysical context this generation is …

Solar dynamo theory

P Charbonneau - Annual Review of Astronomy and …, 2014 - annualreviews.org
The Sun's magnetic field is the engine and energy source driving all phenomena collectively
defining solar activity, which in turn structures the whole heliosphere and significantly …

The case for a distributed solar dynamo shaped by near-surface shear

A Brandenburg - The Astrophysical Journal, 2005 - iopscience.iop.org
Arguments for and against the widely accepted picture of a solar dynamo being seated in
the tachocline are reviewed, and alternative ideas concerning dynamos operating in the …

The solar magnetic field

SK Solanki, B Inhester… - Reports on progress in …, 2006 - iopscience.iop.org
The magnetic field of the Sun is the underlying cause of the many diverse phenomena
combined under the heading of solar activity. Here we describe the magnetic field as it …

[图书][B] The magnetic universe: geophysical and astrophysical dynamo theory

G Rüdiger, R Hollerbach - 2006 - books.google.com
Magnetism is one of the most pervasive features of the Universe, with planets, stars and
entire galaxies all having associated magnetic fields. All of these fields are generated by the …

Cross helicity and related dynamo

N Yokoi - Geophysical & Astrophysical Fluid Dynamics, 2013 - Taylor & Francis
The turbulent cross helicity is directly related to the coupling coefficients for the mean
vorticity in the electromotive force and for the mean magnetic-field strain in the Reynolds …

A new dynamo pattern revealed by solar helical magnetic fields

H Zhang, T Sakurai, A Pevtsov, Y Gao… - Monthly Notices of …, 2010 - academic.oup.com
A previously unobservable mirror asymmetry of the solar magnetic field–a key ingredient of
the dynamo mechanism which is believed to drive the 11-year activity cycle–has recently …

Magnetic fields of low-mass main sequences stars: non-linear dynamo theory and mean-field numerical simulations

N Kleeorin, I Rogachevskii, N Safiullin… - Monthly Notices of …, 2023 - academic.oup.com
Our theoretical and numerical analysis have suggested that for low-mass main sequences
stars (of the spectral classes from M5 to G0) rotating much faster than the Sun, the generated …

Turbulent magnetic helicity fluxes in solar convective zone

N Kleeorin, I Rogachevskii - Monthly Notices of the Royal …, 2022 - academic.oup.com
Combined action of helical motions of plasma (the kinetic α effect) and non-uniform
(differential) rotation is a key dynamo mechanism of solar and galactic large-scale magnetic …

Magnetic fluctuations and formation of large-scale inhomogeneous magnetic structures in a turbulent convection

I Rogachevskii, N Kleeorin - Physical Review E—Statistical, Nonlinear, and …, 2007 - APS
Magnetic fluctuations generated by a tangling of the mean magnetic field by velocity
fluctuations are studied in a developed turbulent convection with large magnetic Reynolds …