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IMPLICATIONS OF A NON-MODAL LINEAR THEORY FOR THE MARGINAL STABILITY STATE AND THE DISSIPATION OF FLUCTUATIONS IN THE SOLAR WIND (2010)

First Author: Camporeale E

Attributed to: Simulation of kinetic effects in turbulence and collisionless shocks funded by STFC

Abstract

No abstract provided

Bibliographic Information

Digital Object Identifier: http://dx.doi.org/10.1088/0004-637x/715/1/260

Publication URI: http://dx.doi.org/10.1088/0004-637x/715/1/260

Type: Journal Article/Review

Parent Publication: The Astrophysical Journal

Issue: 1