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The Role of Proton Cyclotron Resonance as a Dissipation Mechanism in Solar Wind Turbulence: A Statistical Study at Ion-kinetic Scales (2018)

First Author: Woodham L

Attributed to: Ion Heating by Turbulence in the Solar Wind funded by STFC

Abstract

No abstract provided

Bibliographic Information

Digital Object Identifier: http://dx.doi.org/10.3847/1538-4357/aab03d

Publication URI: http://dx.doi.org/10.3847/1538-4357/aab03d

Type: Journal Article/Review

Parent Publication: The Astrophysical Journal

Issue: 1