Magnetism, dynamo action and the solar-stellar connection
AS Brun, MK Browning - Living Reviews in Solar Physics, 2017 - Springer
The Sun and other stars are magnetic: magnetism pervades their interiors and affects their
evolution in a variety of ways. In the Sun, both the fields themselves and their influence on …
evolution in a variety of ways. In the Sun, both the fields themselves and their influence on …
Helioseismic studies of differential rotation in the solar envelope by the solar oscillations investigation using the Michelson Doppler Imager
J Schou, HM Antia, S Basu, RS Bogart… - The Astrophysical …, 1998 - iopscience.iop.org
The splitting of the frequencies of the global resonant acoustic modes of the Sun by large-
scale flows and rotation permits study of the variation of angular velocity Ω with both radius …
scale flows and rotation permits study of the variation of angular velocity Ω with both radius …
Powering stellar magnetism: energy transfers in cyclic dynamos of Sun-like stars
We use the anelastic spherical harmonic code to model the convective dynamo of solar-type
stars. Based on a series of 15 3D MHD simulations spanning four bins in rotation and mass …
stars. Based on a series of 15 3D MHD simulations spanning four bins in rotation and mass …
Global-scale turbulent convection and magnetic dynamo action in the solar envelope
The operation of the solar global dynamo appears to involve many dynamical elements,
including the generation of fields by the intense turbulence of the deep convection zone, the …
including the generation of fields by the intense turbulence of the deep convection zone, the …
An active Sun throughout the Maunder minimum
J Beer, S Tobias, N Weiss - Solar Physics, 1998 - Springer
Measurements of 10 Be concentration in the Dye 3 ice core show that magnetic cycles
persisted throughout the Maunder Minimum, although the Sun's overall activity was …
persisted throughout the Maunder Minimum, although the Sun's overall activity was …
[LIBRO][B] The solar corona
L Golub, JM Pasachoff - 2010 - books.google.com
Intended for graduate students and astronomers seeking an introduction to coronal physics,
this textbook strikes a balance between the observational and theoretical aspects of the …
this textbook strikes a balance between the observational and theoretical aspects of the …
Structure and rotation of the solar interior: initial results from the MDI medium-l program
The medium-l program of the Michelson Doppler Imager instrument on board SOHO
provides continuous observations of oscillation modes of angular degree, l, from 0 to∼ 300 …
provides continuous observations of oscillation modes of angular degree, l, from 0 to∼ 300 …
Penetration and overshooting in turbulent compressible convection
We present the results of a series of high-resolution, three-dimensional numerical
experiments that investigate the nature of turbulent compressible convective motions …
experiments that investigate the nature of turbulent compressible convective motions …
Deeply penetrating banded zonal flows in the solar convection zone
R Howe, J Christensen-Dalsgaard, F Hill… - The Astrophysical …, 2000 - iopscience.iop.org
Helioseismic observations have detected small temporal variations of the rotation rate below
the solar surface that correspond to the so-called" torsional oscillations" known from Doppler …
the solar surface that correspond to the so-called" torsional oscillations" known from Doppler …
Transport and storage of magnetic field by overshooting turbulent compressible convection
We present the results of a series of numerical experiments that investigate the transport of
magnetic fields by turbulent penetrative compressible convection. We find that magnetic flux …
magnetic fields by turbulent penetrative compressible convection. We find that magnetic flux …