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The Parker Solar Probe mission has shown the ubiquitous presence of strong magnetic field deflections, namely switchbacks, during its first perihelion where it was embedded in a highly Alfvenic slow stream. Here, we study the turbulent magnetic fluctuations around ion scales in three intervals characterized by a different switchback activity, identified by the behavior of the magnetic field radial component, B-r. Quiet (B-r does not show significant fluctuations), weakly disturbed (B-r has strong fluctuations but no reversal ...
Published by: ASTROPHYSICAL JOURNAL Published on: 12/2020
YEAR: 2020   DOI: 10.3847/1538-4357/abc480
Published by: \apjl Published on: 02/2013
YEAR: 2013   DOI: 10.1088/2041-8205/763/2/L30