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Investigating Alfvénic Turbulence in Fast and Slow Solar Wind Streams

Solar wind turbulence dominated by large-amplitude Alfvénic fluctuations, mainly propagating away from the Sun, is ubiquitous in high-speed solar wind streams. Recent observations performed in the inner heliosphere (from 1 AU down to tens of solar radii) have proved that also slow wind streams show...

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Salvato in:
Dettagli Bibliografici
Autori principali: Raffaella D’Amicis, Denise Perrone, Marco Velli, Luca Sorriso-Valvo, Daniele Telloni, Roberto Bruno, Rossana De Marco
Natura: Artigo
Lingua:Inglês
Pubblicazione: MDPI AG 2022-06-01
Serie:Universe
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Accesso online:https://www.mdpi.com/2218-1997/8/7/352
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