Radial Evolution of MHD-Scale Solar Wind Turbulence from 35 Rs to 1 AU

Christopher H K Chen1, Stuart D Bale2, John W Bonnell2, Trevor A Bowen3, David Burgess4, Anthony W Case5, Benjamin D G Chandran6, Thierry Dudok de Wit7, Keith Goetz8, Peter Harvey9, Justin Christophe Kasper10, Kelly E Korreck11, Davin E Larson12, Roberto Livi3, Robert J. MacDowall13, David Malaspina14, Alfred Mallet6, Michael McManus15, Marc Pulupa2, Michael Louis Stevens16 and Phyllis L Whittlesey3, (1)Queen Mary University of London, London, United Kingdom, (2)University of California, Berkeley, Space Sciences Laboratory, Berkeley, CA, United States, (3)University of California Berkeley, Berkeley, CA, United States, (4)Queen Mary, University of London, London, United Kingdom, (5)Smithsonian Astrophysical Observatory, Cambridge, MA, United States, (6)University of New Hampshire, Durham, NH, United States, (7)LPC2E, CNRS and University of Orléans, Orléans, France, (8)University of Minnesota, Minneapolis, MN, United States, (9)Space Sciences Laboratory, Berkeley, United States, (10)University of Michigan, Ann Arbor, MI, United States, (11)Smithsonian Observatory, Cambridge, MA, United States, (12)Space Sciences Laboratory, Berkeley, CA, United States, (13)NASA Goddard SFC, Greenbelt, MD, United States, (14)University of Colorado, Boulder, Laboratory for Atmospheric and Space Physics, Boulder, CO, United States, (15)U.S. EPA, Cincinnati, United States, (16)Smithsonian Astrophysics Observatory, Cambridge, MA, United States