Flocculation, switchbacks, and loss of Alfvenicity: Indicators of shear-driven turbulence in the young solar wind?
David J Ruffolo1, William H Matthaeus2, Craig DeForest3, Tulasi Parashar2, Melvyn L Goldstein4,5, D Aaron Roberts6, Rohit Chhiber2, Arcadi V. Usmanov2,4, Thierry Dudok de Wit7, Riddhi Bandyopadhyay8, Alexandros Chasapis9, Bennett Maruca10, Marco C M Velli11 and Justin Christophe Kasper12, (1)Mahidol University, Department of Physics, Faculty of Science, Bangkok, Thailand, (2)University of Delaware, Newark, DE, United States, (3)Southwest Research Institute, Boulder, CO, United States, (4)NASA Goddard SFC, Greenbelt, MD, United States, (5)University of Maryland Baltimore County, Baltimore, MD, United States, (6)NASA Goddard SFC, Code 672, Greenbelt, MD, United States, (7)LPC2E, CNRS and University of Orléans, Orléans, France, (8)University of Delaware, Department of Physics and Astronomy, Newark, DE, United States, (9)Laboratory for Atmospheric and Space Physics, Boulder, United States, (10)Center for Astrophysics, Berkeley, CA, United States, (11)University of California Los Angeles, Earth Planetary and Space Sciences, Los Angeles, CA, United States, (12)University of Michigan, Ann Arbor, MI, United States