Abstract: Can 30 ms Resolution MMS-FPI Electron Distributions Explain Interspersed Parallel and Oblique Whistlers Measured During Magnetopause Reconnection? (2016 AGU Fall Meeting)

Can 30 ms Resolution MMS-FPI Electron Distributions Explain Interspersed Parallel and Oblique Whistlers Measured During Magnetopause Reconnection?

David L Newman¹, Martin V Goldman², Victoria D Wilder³, James Webster¹, Steven J Schwartz⁴, Jonathan P Eastwood⁵ and Giovanni Lapenta⁶, (1)University of Colorado at Boulder, Boulder, CO, United States, (2)University of Colorado at Boulder, Boulder, United States, (3)University of Texas at Arlington, Arlington, TX, United States, (4)Imperial College London, London, United Kingdom, (5)Imperial College London, Physics, London, United Kingdom, (6)KU Leuven, Mathematics, Leuven, Belgium

Back to: Multiscale Structure and Dynamics of Earth's Dayside Magnetopause: Results from the First MMS Dayside Season IV