no code implementations • 26 Jan 2021 • K. G. Klein, J. L. Verniero, B. Alterman, S. Bale, A. Case, J. C. Kasper, K. Korreck, D. Larson, E. Lichko, R. Livi, M. McManus, M. Martinović, A. Rahmati, M. Stevens, P. Whittlesey
The hot and diffuse nature of the Sun's extended atmosphere allows it to persist in non-equilibrium states for long enough that wave-particle instabilities can arise and modify the evolution of the expanding solar wind.
Solar and Stellar Astrophysics Space Physics
