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The Theory of Magnetic Storms and Auroras

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Abstract

No one will disagree with Prof. Alfvén when he stresses the desirability of attempting scale-model experiments of geophysical phenomena in the laboratory. Unfortunately, experience shows that unambiguous experiments of this type are hard to make : a recent study of such an experiment devised by Chapman1 to test theories of magnetic storms reveals some of the difficulties. It would seem that in the field of low-pressure physics, Nature still provides the laboratory best suited for illustrating fundamental principles in action. Certainly, to date, all scale-model attempts to illustrate theories of magnetic storms have yielded ambiguous results : in Alfvén's own recent words2, “we ought to be careful in applying a result from a scale-model experiment to Nature”.

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References

  1. Chapman, S., J. Atmos. and Terr. Phys., 1, 189 (1951).

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  2. Alfvén, H., “Cosmical Electrodynamics”, 203 (Oxford Univ. Press, 1950).

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  3. Chapman, S., and Ferraro, V. C. A., Terr. Mag., 36, 77 (1931).

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  4. Vestine, E. H., and Chapman, S., Terr. Mag., 43, 351 (1938).

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  5. Kirkpatrick, C. B. (to be published shortly).

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MARTYN, D. The Theory of Magnetic Storms and Auroras. Nature 167, 984–985 (1951). https://doi.org/10.1038/167984b0

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  • DOI: https://doi.org/10.1038/167984b0

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