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