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Abstract

The influence of gyroviscosity on the fluctuations of an MHD plasma is investigated by the method reported in a previous note. The main result is that gyroviscosity does not help to remove ultraviolet divergences. For a sub- class of observables it does not even show up. The full nonlinear problem may be needed.

Additional information

Authors: CALDAS I L, MAX-PLANCK-INSTITUT FUER PLASMAPHYSIK, GARCHING BEI MUENCHEN (GERMANY);TASSO H MAX-PLANCK-INSTITUT FUER PLASMAPHYSIK, GARCHING BEI MUENCHEN (GERMANY), MAX-PLANCK-INSTITUT FUER PLASMAPHYSIK, GARCHING BEI MUENCHEN (GERMANY)
Bibliographic Reference: PHYSICS LETTERS, VOL. 104 (1984), NO. 8, PP. 423-424
Record Number: 1989123012100 / Last updated on: 1987-01-01
Category: PUBLICATION
Available languages: en