On the Helical Dynamo of Lortz as a Model for the Steady Main Geomagnetic Field

Author:

Benton Edward R.

Publisher

Oxford University Press (OUP)

Reference34 articles.

1. Hydromagnetics of rotating fluids;Acheson;Repts. Prog. Phys.,1973

2. A class of self-sustaining dissipative spherical dynamos;Backus;Ann. Phys. N. Y.,1958

3. Kinematics of geomagnetic secular variation in a perfectly conducting core;Backus;Phil. Trans. R. Soc. Lond.,1968

4. Spin-Up;Benton;Ann. Rev. Fluid Mech.,1974

5. Geomagnetic data and core motions;Booker;Proc. R. Soc.,1969

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1. I. The Magnetic Fields of Planets;Physics of Solar Planetary Environments: Proceedings Of the International Symposium on Solar-Terrestrial Physics, June 7-18,1976 Boulder, Colorado Volume II;2013-03-22

2. A unified approach to a class of slow dynamos;Geophysical & Astrophysical Fluid Dynamics;1990-06

3. Mathematical Problems in Dynamo Theory;Physical Processes in Hot Cosmic Plasmas;1990

4. On steady kinematic helical dynamos;Geophysical & Astrophysical Fluid Dynamics;1988-12

5. An explicit solution for static unbounded helical dynamos;Geophysical & Astrophysical Fluid Dynamics;1984-12

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