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Abstract: Ion Microstate Evolution in Coronal Hole Wind from 0.05 to 1 au (AGU25)

Ion Microstate Evolution in Coronal Hole Wind from 0.05 to 1 au

Michael Louis Stevens1, Davin Larson2, Roberto Livi3, Phyllis Whittlesey3, Kristopher G Klein4, Kristoff W Paulson1, Ali Rahmati3, Tatiana Niembro Hernandez5, Samuel Timothy Badman5, Yeimy Rivera6, Michael Terres6, Srijan Bharati Das7, Jia Huang3, Jaye Verniero8, Orlando Romeo9, Jasper S Halekas10, Mingzhe Liu11, Stuart Bale12, Timothy Simon Horbury13, Joseph Wang14, Philippe Louarn15, Andrei Fedorov15, Bennett Maruca16, Lynn B Wilson III17 and Benjamin L. Alterman18, (1)Smithsonian Astrophysical Observatory, Cambridge, MA, United States, (2)University of California Berkeley, Berkeley, United States, (3)University of California Berkeley, Space Sciences Laboratory, Berkeley, United States, (4)University of Arizona, Lunar and Planetary Laboratory, Tucson, United States, (5)Smithsonian Astrophysical Observatory, Cambridge, United States, (6)Harvard-Smithsonian Center for Astrophysics, Cambridge, United States, (7)Harvard-Smithsonian Center for Astrophysics, Cambridge, MA, United States, (8)NASA Goddard Space Flight Center, Code 672, Greenbelt, United States, (9)University of California Berkeley, Space Sciences Laboratory, Berkeley, CA, United States, (10)University of Iowa, Physics and Astronomy, Iowa City, United States, (11)LESIA, Observatoire de Paris, Université PSL, CNRS, Sorbonne Université, Université de Paris, Meudon, France, (12)University of California, Berkeley, Berkeley, CA, United States, (13)Imperial College London, Department of Physics, London, SW7, United Kingdom, (14)Imperial College London, London, SW7, United Kingdom, (15)CNRS - Institut de Recherche en Astrophysique et Planétologie, Toulouse, France, (16)University of Delaware, Department of Physics and Astronomy, Newark, United States, (17)NASA Goddard Space Flight Center, Greenbelt, MD, United States, (18)NASA Goddard Space Flight Center, Greenbelt, United States