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Solar wind turbulence: Connections with energetic particles
DOI: 10.1016/j.newast.2020.101507 Bibcode: 2021NewA...8301507O

Oughton, Sean; Engelbrecht, N. Eugene

For the solar wind, a wealth of observational evidence indicates that turbulence is an important dynamical process for velocity (v), magnetic (b), and other related fluctuations at MHD (fluid) scales. Here we review such observations and turbulence features, including discussion of when wave or turbulence descriptions can (or cannot) explain the o…

2021 New Astronomy
Ulysses Cluster 29