Hostname: page-component-77c89778f8-m42fx Total loading time: 0 Render date: 2024-07-17T18:46:30.673Z Has data issue: false hasContentIssue false

The secular variation of the earth's magnetic field

Published online by Cambridge University Press:  24 October 2008

D. W. Allan
Affiliation:
King's College, London, and Department of Geophysics, Cambridge
E. C. Bullard
Affiliation:
King's College, London, and Department of Geophysics, Cambridge

Abstract

The magnetic field observable outside a body of conducting fluid in which field is imbedded may be considerably altered by convection currents in the fluid. One possible explanation of the geomagnetic secular variation foci is that localized convection cells in the earth's core disturb the main field present. An analytic solution for such a process is readily obtained by assuming the form and dimensions for such a cell, and shows that the magnitude of the secular variation cannot easily be explained on these lines without the presence of a subsurface toroidal magnetic field of some hundreds of gauss which is ‘convected through’ the surface of the core.

Type
Research Article
Copyright
Copyright © Cambridge Philosophical Society 1966

Access options

Get access to the full version of this content by using one of the access options below. (Log in options will check for institutional or personal access. Content may require purchase if you do not have access.)

References

REFERENCES

(1)Allan, D. W.On the behaviour of systems of coupled dynamos. Proc. Cambridge Philos. Soc. 58 (1962), 671693.CrossRefGoogle Scholar
(2)Allan, D. W. and Bullard, E. C.Distortion of a toroidal field by convection. Rev. Mod. Phys. 30 (1958), 10871088.CrossRefGoogle Scholar
(3)Braginskii, S. I.Self-excitation of a magnetic field during the motion of a highly conducting fluid. J. Exptl Theoret. Phys. (USSR) 47 (1964), 10841098. Translation Soviet Physics JEPT 20 (1965), 726–735.Google Scholar
(4)Bullard, E. C.The secular change in the earth's magnetic field. Monthly Not. Boy. Astr. Soc. Geophys, Suppl. 5 (1948), 248257.Google Scholar
(5)Bullard, E. C.The secular variation of the earth's magnetic field (9th Charles Chree Lecture). Year Book of the Physical Society (1958), 4760.Google Scholar
(6)SirEdward, Bullard and Gellman, H.Homogeneous dynamos and terrestrial magnetism. Philos. Trans. Roy. Soc. London, Ser. A 247 (1954), 213278.Google Scholar
(7)Coulomb, J.Variation seculaire par convergence ou divergence à la surface du noyau. Ann. Géophys. 11 (1955), 8082.Google Scholar
(8)Elasasser, Walter M.Induction effects in terrestrial magnetism. Phys. Rev. 69 (1946), 106116.CrossRefGoogle Scholar
(9)Hide, R. Free hydromagnetic oscillations of the earth's core and the theory of the geomagnetic secular variation. NATO Advanced Study Institute Meeting on ‘Planetary and Stellar Magnetism’, Newcastle, 1965. To be published as Magnetism and the Cosmos (Oliver and Boyd, 1966).Google Scholar
(10)Hide, R. and Roberts, R. P. The origin of the main geomagnetic field. Chapter 2 of Physics and Chemistry of the Earth, vol. 4 (ed. Ahrens, , Press, , Rankama, , and Runcorn, ) (Pergamon Press; London, 1961).Google Scholar
(11)Jeffreys, H. and Jeffreys, B. S.Methods of mathematical physics (Cambridge, 1956).Google Scholar
(12)Lighthtll, M. J.Introduction to Fourier analysis and generalized functions (Cambridge, 1958).CrossRefGoogle Scholar
(13)Lowes, F. J. and Runcorn, S. K.The analysis of the geomagnetic secular variation. Philos. Trans. Roy. Soc. London, Ser. A 243 (1951), 525546.Google Scholar
(14)Roberts, P. H. Inferences concerning motions of the core. NATO Advanced Study Institute Meeting on ‘Planetary and Stellar Magnetism’, Newcastle, 1965. To be published as Magnetism and the Cosmos (Oliver and Boyd, 1966).Google Scholar
(15)Whittaker, E. T. and Watson, G. N.A course of modern analysis, 4th ed. (Cambridge, 1927).Google Scholar