Figure 4 from Sub-Alfvénic Solar Wind Observed by the Parker Solar Probe: Characterization of Turbulence, Anisotropy, Intermittency, and Switchback

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Sub-Alfvénic Solar Wind Observed by the Parker Solar Probe: Characterization of Turbulence, Anisotropy, Intermittency, and Switchback

Authors: R. Bandyopadhyay, W. H. Matthaeus, D. J. McComas, R. Chhiber, A. V. Usmanov, J. Huang, R. Livi, D. E. Larson, J. C. Kasper, A. W. Case, M. Stevens, P. Whittlesey, O. M. Romeo, S. D. Bale, J. W. Bonnell, T. Dudok de Wit, K. Goetz, P. R. Harvey, R. J. MacDowall, D. M. Malaspina, and M. Pulupa

2022 The Astrophysical Journal Letters 926 L1.

Provider: AAS Journals

Caption: Figure 4.

Histogram of PVI in the sub-Alfvénic and the neighboring super-Alfvénic periods near perihelia 8 and 9 (see Figure 1 and Section 3). PVI values larger than 2.5 (vertical line) represent intermittent structures.

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