The role of Alfvén wave dynamics in the large scale properties of the solar wind: comparing 3D MHD simulation and PSP data

Victor Réville1,2, Marco Velli3, Olga Panasenco4, Anna Tenerani5, Chen Shi6, Alexis P Rouillard7, Stuart D Bale8, Justin Christophe Kasper9, Samuel Timothy Badman10, Kelly E Korreck11, Marc Pulupa8, John W Bonnell8, Anthony W Case12, Davin E Larson13, Roberto Livi10, Michael Louis Stevens14, Phyllis L Whittlesey10, David Malaspina15, Peter Harvey16, Keith Goetz17, Thierry Dudok de Wit18 and Robert J MacDowall19, (1)University of California Los Angeles, Los Angeles, United States, (2)IRAP, Toulouse, France, (3)University of California Los Angeles, Los Angeles, CA, United States, (4)Advanced Heliophysics, Pasadena, CA, United States, (5)University of Texas at Austin, Austin, TX, United States, (6)University of California Los Angeles, Earth, Planetary and Space Sciences, Los Angeles, CA, United States, (7)IRAP/CNRS, Toulouse, France, (8)University of California, Berkeley, Space Sciences Laboratory, Berkeley, CA, United States, (9)University of Michigan, Ann Arbor, MI, United States, (10)University of California Berkeley, Berkeley, CA, United States, (11)Smithsonian Observatory, Cambridge, MA, United States, (12)Smithsonian Astrophysical Observatory, Cambridge, MA, United States, (13)Space Sciences Laboratory, Berkeley, CA, United States, (14)Smithsonian Astrophysics Observatory, Cambridge, MA, United States, (15)University of Colorado, Boulder, Laboratory for Atmospheric and Space Physics, Boulder, CO, United States, (16)Space Sciences Laboratory, Berkeley, United States, (17)University of Minnesota, Minneapolis, MN, United States, (18)LPC2E, CNRS and University of Orléans, Orléans, France, (19)NASA/Goddard Space Flight Center, Greenbelt, United States