MHD mode decomposition in the inner-heliosphere from the Parker Solar Probe

Christopher Carew Chaston1, John W Bonnell2, Stuart Bale3, Justin Christophe Kasper4, John R Wygant5, Marc Pulupa2, Phyllis L Whittlesey6, Davin E Larson7, Robert J. MacDowall8, Roberto Livi6, Chadi S Salem9, Daniel Vech10, Anthony W Case11, Keith Goetz5, Kelly E Korreck12, Peter Harvey2, David Malaspina13, Michael Louis Stevens14 and Thierry Dudok de Wit15, (1)University of California Berkeley, Space Sciences Laboratory, Berkeley, CA, United States, (2)University of California, Berkeley, Space Sciences Laboratory, Berkeley, CA, United States, (3)University of California, Berkeley, Berkeley, CA, United States, (4)University of Michigan, Ann Arbor, MI, United States, (5)University of Minnesota, Minneapolis, MN, United States, (6)University of California Berkeley, Berkeley, CA, United States, (7)Space Sciences Laboratory, Berkeley, CA, United States, (8)NASA Goddard SFC, Greenbelt, MD, United States, (9)University of California, Berkeley, CA, United States, (10)Lawrence, KS, United States, (11)Smithsonian Astrophysical Observatory, Cambridge, MA, United States, (12)Smithsonian Observatory, Cambridge, MA, United States, (13)University of Colorado, Boulder, Laboratory for Atmospheric and Space Physics, Boulder, CO, United States, (14)Smithsonian Astrophysics Observatory, Cambridge, MA, United States, (15)LPC2E, CNRS and University of Orléans, Orléans, France