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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: MSSL Solar & Planetary Physics Consolidated Grant 2016-2019 funded by STFC

Abstract

No abstract provided

Bibliographic Information

Digital Object Identifier: http://dx.doi.org/10.48550/arxiv.1801.07344

Publication URI: https://arxiv.org/abs/1801.07344

Type: Other