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Abstract: Whistler wave mode generation via large amplitude steepened magnetic structures propagating through the Martian ionosphere (AGU25)

Whistler wave mode generation via large amplitude steepened magnetic structures propagating through the Martian ionosphere

Christopher M Fowler1, Kathleen Gwen Hanley2, Jasper S Halekas3, Catherine Regan4, James P McFadden5, David Mitchell6, Laila Andersson7, Yuki Harada8, Duncan Bark2, Yingjuan Ma9, Christopher Carew Chaston5, Beatriz Sanchez-Cano10, Mark Lester11, David A Brain12, Christian Xavier Mazelle13, Jared R Espley14, Mehdi Benna15, Rebecca Jolitz16 and Shannon Curry17, (1)West Virginia University, Department of Physics and Astronomy, Morgantown, United States, (2)Laboratory for Atmospheric and Space Physics, Boulder, United States, (3)University of Iowa, Physics and Astronomy, Iowa City, United States, (4)University College London, Mullard Space Science Laboratory, London, United Kingdom, (5)Univ California Berkeley, Berkeley, United States, (6)Space Sciences Laboratory, University of California Berkeley, Berkeley, United States, (7)Laboratory for Atmospheric and Space Physics, University of Colorado, Boulder, United States, (8)University of Iowa, Iowa City, United States, (9)University of California Los Angeles, Los Angeles, CA, United States, (10)University of Leicester, Leicester, LE1, United Kingdom, (11)University of Leicester, Leicester, United Kingdom, (12)University of Colorado at Boulder, Laboratory for Atmospheric and Space Physics, Boulder, United States, (13)University Paul Sabatier Toulouse III, Toulouse Cedex 09, France, (14)Goddard Space Flight Center, Greenbelt, United States, (15)NASA Goddard Space Flight Center, Greenbelt, MD, United States, (16)University of California Berkeley, Space Sciences Laboratory, Berkeley, United States, (17)University of Colorado Boulder, Laboratory for Atmospheric and Space Physics, Boulder, United States