Hostname: page-component-848d4c4894-tn8tq Total loading time: 0 Render date: 2024-06-23T15:25:15.711Z Has data issue: false hasContentIssue false

Fluctuations in the Galactic Magnetic Field

Published online by Cambridge University Press:  19 July 2016

James M. Cordes
Affiliation:
Astronomy Department and NAIC Cornell University Ithaca, NY 14853 USA
Andrew Clegg
Affiliation:
Astronomy Department and NAIC Cornell University Ithaca, NY 14853 USA
John Simonetti
Affiliation:
Virginia Polytechnic Institute and State University Department of Physics Blacksburg, VA 24061 USA

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

We discuss small scale structure in the Galactic magnetic field as inferred from Faraday rotation measurements of extragalactic radio sources. The rotation measure data suggest a continuum of length scales extending from parsec scales down to at least 0.01 pc and perhaps to as small as 109 cm. Such turbulence in the magnetic field comprises a reservoir of energy that is comparable to the energy in the large scale field.

Type
2. The Magnetic Field Structure of the Milky Way: The Meeting of Observation and Theory
Copyright
Copyright © Kluwer 1990 

References

1. Simonetti, J. H., Cordes, J. M., and Spangler, S. R. 1984, Ap. J. , 284, 126.Google Scholar
2. Leahy, J. P. 1984, Ph. D. Thesis.Google Scholar
3. Simonetti, J. H., and Cordes, J. M. 1986, Ap. J. , 310, 160.CrossRefGoogle Scholar
4. Lee, L. C. and Jokipii, J. R. 1976, Ap. J. , 206, 735.Google Scholar
5. Armstrong, J. W., Cordes, J. M., and Rickett, B. J. 1981, Nature , 291, 561.CrossRefGoogle Scholar
6. Montgomery, D., Brown, M. R., and Matthaeus, W. H., 1987, J. Geophys. Res. , 92, 282.Google Scholar
7. Jokipii, J. R. 1988, in Radio Wave Scattering in the Interstellar Medium , AIP Conference Proc. 174, 4859.CrossRefGoogle Scholar