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).
This is a preview of subscription content, access via your institution
Access options
Subscribe to this journal
Receive 51 print issues and online access
$199.00 per year
only $3.90 per issue
Buy this article
- Purchase on Springer Link
- Instant access to full article PDF
Prices may be subject to local taxes which are calculated during checkout
Similar content being viewed by others
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).
Author information
Authors and Affiliations
Rights and permissions
About this article
Cite this article
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
Received:
Accepted:
Issue Date:
DOI: https://doi.org/10.1038/258309a0
This article is cited by
-
Thin scattering diffusion and the size of the crab nebula
Astrophysics and Space Science (1977)
Comments
By submitting a comment you agree to abide by our Terms and Community Guidelines. If you find something abusive or that does not comply with our terms or guidelines please flag it as inappropriate.
