Plasma waves near the electron cyclotron frequency in the near-Sun solar wind: implications for inner heliospheric turbulence and the structure of the solar wind
Plasma waves near the electron cyclotron frequency in the near-Sun solar wind: implications for inner heliospheric turbulence and the structure of the solar wind
David Malaspina1, Stuart Bale2, John W Bonnell3, Thierry Dudok de Wit4, James Webster5, Keith Goetz6, Peter Harvey7, Robert J MacDowall8, Marc Pulupa3, Anthony W Case9, Jasper S Halekas10, Justin Christophe Kasper11, Kelly E Korreck12, Davin E Larson13, Roberto Livi14, Michael Louis Stevens15, Phyllis L Whittlesey14 and Katherine Goodrich16, (1)University of Colorado, Boulder, Laboratory for Atmospheric and Space Physics, Boulder, CO, United States, (2)University of California, Berkeley, Berkeley, CA, United States, (3)University of California, Berkeley, Space Sciences Laboratory, Berkeley, CA, United States, (4)LPC2E, CNRS and University of Orléans, Orléans, France, (5)University of Colorado, Boulder, CO, United States, (6)University of Minnesota, Minneapolis, MN, United States, (7)Space Sciences Laboratory, Berkeley, United States, (8)NASA/Goddard Space Flight Center, Greenbelt, United States, (9)Smithsonian Astrophysical Observatory, Cambridge, MA, United States, (10)University of Iowa, Department of Physics and Astronomy, Iowa City, IA, United States, (11)University of Michigan, Ann Arbor, MI, United States, (12)Smithsonian Observatory, Cambridge, MA, United States, (13)Space Sciences Laboratory, Berkeley, CA, United States, (14)University of California Berkeley, Berkeley, CA, United States, (15)Smithsonian Astrophysics Observatory, Cambridge, MA, United States, (16)University of Colorado Boulder, Boulder, CO, United States
