Comparison of Parker Solar Probe Observations during First Perihelion with Global Magnetohydrodynamic Model Results

Pete Riley1, Cooper Downs1, Jon Linker1, Roberto Lionello1, Ronald M. Caplan1, Stuart D Bale2, Justin Christophe Kasper3, Russell Howard4, Marc Pulupa2, David Malaspina5, John W Bonnell2, Peter Harvey2, Keith Goetz6, Thierry Dudok de Wit7, Robert J MacDowall8, Anthony W Case9, Kelly E Korreck10, Davin E Larson11, Roberto Livi12, Michael Louis Stevens13 and Phyllis L Whittlesey12, (1)Predictive Science Inc., San Diego, CA, United States, (2)University of California, Berkeley, Space Sciences Laboratory, Berkeley, CA, United States, (3)University of Michigan, Ann Arbor, MI, United States, (4)Naval Research Laboratory, Washington, DC, United States, (5)University of Colorado, Boulder, Laboratory for Atmospheric and Space Physics, Boulder, CO, United States, (6)University of Minnesota, Minneapolis, MN, United States, (7)LPC2E, CNRS and University of Orléans, Orléans, France, (8)NASA/Goddard Space Flight Center, Greenbelt, United States, (9)Smithsonian Astrophysical Observatory, Cambridge, MA, United States, (10)Smithsonian Observatory, Cambridge, MA, United States, (11)Space Sciences Laboratory, Berkeley, CA, United States, (12)University of California Berkeley, Berkeley, CA, United States, (13)Smithsonian Astrophysics Observatory, Cambridge, MA, United States