Characteristics and Evolution of Strahl Electrons in the Inner Heliosphere

Davin E Larson1, Phyllis L Whittlesey2, Roberto Livi2, Justin Christophe Kasper3, Anthony W Case4, Kelly E Korreck5, Michael Louis Stevens6, Jasper S Halekas7, Laura Bercic8, Ali Rahmati9, Michael McManus2, Jennifer L Verniero9, Milan Maksimovic8, Stuart D Bale10, Marc Pulupa10, David Malaspina11, John W Bonnell10, Peter Harvey12, Keith Goetz13, Thierry Dudok de Wit14 and Robert J MacDowall15, (1)Space Sciences Laboratory, Berkeley, CA, United States, (2)University of California Berkeley, Berkeley, CA, United States, (3)University of Michigan, Ann Arbor, MI, United States, (4)Smithsonian Astrophysical Observatory, Cambridge, MA, United States, (5)Smithsonian Observatory, Cambridge, MA, United States, (6)Smithsonian Astrophysics Observatory, Cambridge, MA, United States, (7)University of Iowa, Department of Physics and Astronomy, Iowa City, IA, United States, (8)LESIA, Observatoire de Paris, Université PSL, CNRS, Sorbonne Université, Université Paris Diderot, Sorbonne Paris Cité, Meudon, France, (9)University of California Berkeley, Space Sciences Laboratory, Berkeley, CA, United States, (10)University of California, Berkeley, Space Sciences Laboratory, Berkeley, CA, United States, (11)University of Colorado, Boulder, Laboratory for Atmospheric and Space Physics, Boulder, CO, United States, (12)Space Sciences Laboratory, Berkeley, United States, (13)University of Minnesota, Minneapolis, MN, United States, (14)LPC2E, CNRS and University of Orléans, Orléans, France, (15)NASA/Goddard Space Flight Center, Greenbelt, United States