Differential kinetic dynamics and heating of ions in the turbulent solar wind

Article

Abstract: The solar wind plasma is a fully ionized and turbulent gas ejected by the outer layers of the solar

Palabras claves:

plasma heating, solar wind, space missions, Turbulence

Autores:

Brienza D., Bruno R., Consolini G., de Keyser J., De Marco R., Lavraud B., Luca Sorriso-Valvo, Marcucci M.F., Perrone D., Pezzi O., Retinò A., Salatti M., Servidio S., Stabile S., Vaivads A., Valentini F., Veltri P.

Fuentes:

scopus