Turbulence and Waves in the Sub-Alfvénic Solar Wind Observed by the Parker Solar Probe during Encounter 10
Authors: L.-L. Zhao, G. P. Zank, L. Adhikari, D. Telloni, M. Stevens, J. C. Kasper, S. D. Bale, N. E. Raouafi
L.-L. Zhao et al
2022 The Astrophysical Journal Letters934.
Provider: AAS Journals
Caption: Figure 5.
A magnified view of the super-Alfvénic interval between the two sub-Alfvénic flows. The top three panels show the radial magnetic field BR, radial proton speed VR, density np, and magnetic field magnitude ∣B∣. The other panels have the same format as Figure 4.