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Properties of Magnetohydrodynamic Turbulence in the Solar Wind

Published online by Cambridge University Press:  14 August 2015

M. Dobrowolny ,
A. Mangeney  and
P.L. Veltri
M. Dobrowolny
Affiliation:
(Laboratorio Plasma Spazio, CNR, Frascati, Italy)
A. Mangeney
Affiliation:
(Observatoire de Meudon, Paris, France)
P.L. Veltri
Affiliation:
(Dipartimento di Fisica, Università della Calabria, Italy)

Extract

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The observations of MHD turbulence in the solar wind indicate that this is in a state characterized, to a good degree by the absence of non linear interactions. It is argued that this is a general property of incompressible MHD turbulence in a magnetized plasma.

Type
Part II. Coronal and Interplanetary Responses to Long Time Scale Phenomena
Information
Symposium - International Astronomical Union , Volume 91: Solar and Interplanetary Dynamics , 1980 , pp. 143 - 146
Copyright
Copyright © Reidel 1980 

References

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