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The investigation of the hierarchical structure of the interstellar magnetic fields

Published online by Cambridge University Press:  03 August 2017

A.L. Lazarian
A.L. Lazarian*
Affiliation:
P.N.Lebedev Physical Institute, U S S R

Abstract

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A new method of investigation of the hierarchical structure of the interstellar magnetic fields is discussed. Synchrotron intensity fluctuations are used. Statistical characteristics of the irregular magnetic field are available. The method was successfully tested.

Type
Velocity Field and Magnetic Field
Information
Symposium - International Astronomical Union , Volume 147: Fragmentation of Molecular Clouds and Star Formation , 1991 , pp. 65 - 66
Copyright
Copyright © Kluwer 1991 

References

1. Chibisov, G.V., Lazarian, A.L. Preprint 283, Moscow, FIAN, 1987.Google Scholar
2. Chibisov, G.V., Ptuskin, V.S. Proc. 17–th Int. Cosmic Ray Conf. (Paris) 2, 233 (1981).Google Scholar
3. Chibisov, G.V., Lazarian, A.L. Preprint 191, Moscow, FIAN, 1989.Google Scholar
4. Oagkesamanskii, R.D., Shutenkov, V.R. (1987) “Radio background fluctuations and the structure of the galactic magnetic field”. Sov. Astron. Lett. 13 (2), 73–76.Google Scholar
5. Lazarian, A.L., Shutenkov, V.R., Preprint 180, Moscow, FIAN, 1989.Google Scholar
6. Lazarian, A.L., Preprint 190, Moscow, FIAN, 1989.Google Scholar