Skip to main content

Antidynamo and Bounding Theorems

  • Reference work entry

Dynamos are devices that convert mechanical energy into electromagnetic energy. While technical dynamos depend on a suitable arrangement of multiply connected regions (usually wires) of high electrical conductivity within an insulating space, the generation of magnetic fields in planets and stars must occur in simply connected domains of essentially uniform finite conductivity. For a long time after Larmor (1919) (see Larmor, J. ) first proposed this homogeneous dynamo process as the origin of magnetic fields in sunspots it has been doubtful whether it is possible. Mathematicians and geophysicists have proved antidynamo theorems in order to determine the conditions under which homogeneous dynamos are possible. The first and most famous theorem has been formulated and proved by Cowling (1934) (see Cowling, T.G. ). He demonstrated that axisymmetric or two‐dimensional magnetic fields cannot be generated by the homogeneous dynamo process (see Cowling's Theorem ). Since the Earth's magnetic...

This is a preview of subscription content, log in via an institution.

Buying options

Chapter
USD   29.95
Price excludes VAT (USA)
  • Available as PDF
  • Read on any device
  • Instant download
  • Own it forever
eBook
USD   499.00
Price excludes VAT (USA)
  • Available as PDF
  • Read on any device
  • Instant download
  • Own it forever
Hardcover Book
USD   599.99
Price excludes VAT (USA)
  • Durable hardcover edition
  • Dispatched in 3 to 5 business days
  • Free shipping worldwide - see info

Tax calculation will be finalised at checkout

Purchases are for personal use only

Learn about institutional subscriptions

Bibliography

  • Backus, G., 1958. A class of self‐sustaining dissipative spherical dynamos, Annals of Physics, 4: 372–447.

    Google Scholar 

  • Bullard, E., and Gellman, H., 1954. Homogeneous dynamos and terrestrial magnetism. Philosophical Transactions of the Royal Society of London, A247: 213–278.

    Google Scholar 

  • Busse, F.H., 1975. A necessary condition for the geodynamo. Journal of Geophysical Research, 80: 278–280.

    Google Scholar 

  • Childress, S., 1969. Théorie magnétohydrodynamique de l'effet dynamo, Lecture Notes. Département Méchanique de la Faculté des Sciences, Paris.

    Google Scholar 

  • Cowling, T.G., 1934. The magnetic field of sunspots. Monthly Notices of the Royal Astronomical Society, 34: 39–48.

    Google Scholar 

  • Elsasser, W.M., 1946. Induction effects in terrestrial magnetism. Physical Review, 69: 106–116.

    Google Scholar 

  • Gailitis, A., 1970. Magnetic field excitation by a pair of ring vortices. Magnetohydrodynamics (N.Y.), 6: 14–17.

    Google Scholar 

  • Herzenberg, A., 1958. Geomagnetic Dynamos. Philosophical Transactions of the Royal Society of London, A250: 543–585.

    Google Scholar 

  • Ivers, D.J., 1995. On the antidynamo theorem for partly symmetric flows. Geophysical and Astrophysical Fluid Dynamics, 80: 121–128.

    Google Scholar 

  • Kaiser, R., 1995. Towards a poloidal magnetic field theorem. Geophysical and Astrophysical Fluid Dynamics, 80: 129–144.

    Google Scholar 

  • Kaiser, R., Schmitt, B.J., and Busse, F.H., 1994. On the invisible dynamo. Geophysical and Astrophysical Fluid Dynamics, 77: 91–109.

    Google Scholar 

  • Larmor, J., 1919. How could a rotating body such as the sun become a magnet? Reports of the British Association for the Advancement of Science, 159–160.

    Google Scholar 

  • Lortz, D., 1968. Exact solutions of the hydromagnetic dynamo problem. Plasma Physics, 10: 967–972.

    Google Scholar 

  • Namikawa, T., and Matsushita, S., 1970. Kinematic dynamo problem. Geophysical Journal of the Royal Astronomical Society, 19: 319–415.

    Google Scholar 

  • Proctor, M.R.E., 1977. On Backus’ necessary condition for dynamo action in a conducting sphere. Geophysical and Astrophysical Fluid Dynamics, 9: 89–93.

    Google Scholar 

  • Proctor, M.R.E., 1979. Necessary conditions for the magnetohydrodynamic dynamo. Geophysical and Astrophysical Fluid Dynamics, 14: 127–145.

    Google Scholar 

  • Proctor, M.R.E., 2004. An extension of the toroidal theorem. Geophysical and Astrophysical Fluid Dynamics, 98: 235–240.

    Google Scholar 

Download references

Authors

Editor information

Editors and Affiliations

Rights and permissions

Reprints and permissions

Copyright information

© 2007 Springer-Verlag

About this entry

Cite this entry

Busse, F., Proctor, M. (2007). Antidynamo and Bounding Theorems. In: Gubbins, D., Herrero-Bervera, E. (eds) Encyclopedia of Geomagnetism and Paleomagnetism. Springer, Dordrecht. https://doi.org/10.1007/978-1-4020-4423-6_8

Download citation

Publish with us

Policies and ethics