Observations of magnetohydrodynamic turbulence in the 3D heliosphere

Conference Object

Abstract: The solar wind is a high Reynolds' number plasma flow of solar origin that permeates the whole helio

Palabras claves:

Interplanetary space, Solar wind fields, Solar wind plasma, Waves and discontinuities

Autores:

Bavassano B., Bruno R., Carbone V., Luca Sorriso-Valvo

Fuentes:

scopus