Abstract
A UNIFORM, large scale magnetic field is probably an abstraction not found in nature. All sorts of instabilities may arise, and a filamentary or sheet-like structure is most likely to ensue. For example, it is well known that a picture of the optical continuum of the Crab Nebula shows a cotton-like structure, on a scale much smaller than the wisps (∼ 1016 cm).
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References
Tucker, W. H., thesis, Univ. California, San Diego (1966).
Pounds, K., Second European Meeting in Astronomy, Trieste, Italy (1974).
Apparao, K. M. V., Astrophys. Space Sci., 25, 3 (1973).
Fazio, G. G., Helmken, H. F., O'Mongain, E., and Weekes, T. C., Astrophvys. J. Lett., 175, L117 (1972).
Blumenthal, G. R., and Gould, R. J., Rev. Mod. Phys., 42, 237 (1970).
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CAVALLO, G., VENTURA, A. Qualitative features of synchrotron radiation in an inhomogeneous magnetic field. Nature 258, 309–310 (1975). https://doi.org/10.1038/258309a0
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DOI: https://doi.org/10.1038/258309a0
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