Abstract: What Solar Wind Conditions Lead to the Generation of the Different Types of Poleward-Moving Auroral Forms? (2017 AGU Fall Meeting)

What Solar Wind Conditions Lead to the Generation of the Different Types of Poleward-Moving Auroral Forms?

Gerard J Fasel¹, Alex Booth², Ashley Golla³, David Cook², Juliet Elise Mills², Simone Raeth², Jennifer Lau⁴, Kaseba Chibwe², Fred Sigernes⁵ and Dag A Lorentzen⁶, (1)Pepperdine University, Natural Science, Malibu, CA, United States, (2)Pepperdine University, Malibu, CA, United States, (3)State College, PA, United States, (4)Pepperdine University, natural science department, Malibu, CA, United States, (5)University Centre in Svalbard, Longyearbyen, Norway, (6)UNIS, Longyearbyen, Norway

Back to: Imaging the Global Dynamics of the Solar Wind-Magnetosphere Interaction II Posters