Energy partition between the solar wind proton "core" and "tail" distributions in the inner heliosphere
Energy partition between the solar wind proton "core" and "tail" distributions in the inner heliosphere
Michael Louis Stevens1, Anthony W Case1, Kristoff W Paulson2, Tatiana Niembro Hernandez3, Kelly E Korreck1, Justin Kasper4, Davin Larson5, Roberto Livi6, Phyllis L Whittlesey6, Ali Rahmati7, Michael McManus8, Ben Alterman9, Jaye Verniero10 and Dakeyo Jean-Baptiste11, (1)Smithsonian Astrophysical Observatory, Cambridge, MA, United States, (2)University of New Hampshire, Chelmsford, United States, (3)UNAM National Autonomous University of Mexico, Fac. de Ciencias, Mexico City, Mexico, (4)University of Michigan, Ann Arbor, United States, (5)University of California Berkeley, Berkeley, CA, United States, (6)Space Sciences Laboratory, University of California Berkeley, Berkeley, United States, (7)University of California Berkeley, Space Sciences Laboratory, Berkeley, CA, United States, (8)SSL/UC Berkeley, Berkely, United States, (9)Southwest Research Institute, San Antonio, United States, (10)NASA/GSFC, Greenbelt, United States, (11)LESIA, Observatoire de Paris, Meudon, France