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:  Kinetic plasma turbulence in space and astrophysical flows 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