The Role of Proton Cyclotron Resonance as a Dissipation Mechanism in Solar Wind Turbulence: A Statistical Study at Ion-kinetic Scales (2018)
Attributed to:
Thermodynamics of Astrophysical Plasmas: Macroscopic Effects of Collisionless Microphysics
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