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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
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New Astronomy
Ulysses
Cluster
29