How collisionless are solar wind electrons? The role of skewed kappa distributions in the solar wind heat-flux transport


Pablo S Moya1, Adolfo F. Vinas2, Rodrigo Lopez3, Mark L Adrian4 and Javier Silva1, (1)University of Chile, Department of Physics, Faculty of Sciences, Santiago, Chile, (2)NASA Goddard Space Flight Center, Greenbelt, MD, United States, (3)University of Maryland, College Park, CA, United States, (4)Auburn University, Physics Department, Auburn, AL, United States
Back to: The Forefront of Kappa Distributions: Understanding Plasma Processes in the Heliosphere and Kolmogorov in Space—Application and Extension of Turbulence Theory in Space Plasmas Posters