Towards a model for the solar dynamo
Open Access
- 1 July 2000
- journal article
- research article
- Published by Oxford University Press (OUP) in Monthly Notices of the Royal Astronomical Society
- Vol. 315 (3) , 521-533
- https://doi.org/10.1046/j.1365-8711.2000.03452.x
Abstract
No abstract availableKeywords
This publication has 21 references indexed in Scilit:
- Modulation and symmetry changes in stellar dynamosMonthly Notices of the Royal Astronomical Society, 1998
- An Active Sun Throughout the Maunder MinimumSolar Physics, 1998
- Solar Interface Dynamos. II. Linear, Kinematic Models in Spherical GeometryThe Astrophysical Journal, 1997
- Breaking of equatorial symmetry in a rotating system: A spiralling intermittency mechanismEurophysics Letters, 1997
- STRUCTURE AND ROTATION OF THE SOLAR INTERIOR: INITIAL RESULTS FROM THE MDI MEDIUM-L PROGRAMSolar Physics, 1997
- On the Generation of Equipartition-Strength Magnetic Fields by Turbulent Hydromagnetic DynamosThe Astrophysical Journal, 1996
- Nonlinear saturation of the turbulenteffectPhysical Review E, 1996
- A new model of the solar cycleMonthly Notices of the Royal Astronomical Society, 1996
- Turbulent viscosity, magnetic diffusivity, and heat conductivity under the influence of rotation and magnetic fieldAstronomische Nachrichten, 1994
- Evidence for long-term brightness changes of solar-type starsNature, 1990