On the Generation of Equipartition-Strength Magnetic Fields by Turbulent Hydromagnetic Dynamos
- 10 December 1996
- journal article
- Published by American Astronomical Society in The Astrophysical Journal
- Vol. 473 (1) , L59-L62
- https://doi.org/10.1086/310387
Abstract
No abstract availableThis publication has 12 references indexed in Scilit:
- Diffusivity Quenching as a Mechanism for Parker's Surface DynamoThe Astrophysical Journal, 1996
- Stellar Winds with Non-WKB Alfven Waves. II. Wind Models for Cool, Evolved StarsThe Astrophysical Journal, 1995
- On a Babcock-Leighton dynamo model with a deep-seated generating layer for the toroidal magnetic fieldSolar Physics, 1995
- Measurement of the Rotation Rate in the Deep Solar InteriorThe Astrophysical Journal, 1995
- Self-consistent mean field electrodynamics of turbulent dynamosPhysics of Plasmas, 1995
- Emerging flux tubes in the solar convection zone. 1: Asymmetry, tilt, and emergence latitudeThe Astrophysical Journal, 1995
- A solar dynamo surface wave at the interface between convection and nonuniform rotationThe Astrophysical Journal, 1993
- The origin of morphological asymmetries in bipolar active regionsThe Astrophysical Journal, 1993
- The spectrum of random magnetic fields in the mean field dynamo theory of the Galactic magnetic fieldThe Astrophysical Journal, 1992
- The influence of the Coriolis force on flux tubes rising through the solar convection zoneThe Astrophysical Journal, 1987