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Abstract: Investigating hemispheric asymmetries in coronal hole solar wind structured by magnetolatitude (AGU25)

Investigating hemispheric asymmetries in coronal hole solar wind structured by magnetolatitude

Yeimy Rivera1, Adam Finley2, Samuel Timothy Badman3, Kristopher G Klein4, Michael Louis Stevens5, Kristoff W Paulson6, Tatiana Niembro Hernandez1, Srijan Bharati Das1, Michael Terres1, Federico Fraschetti3, Jasper S Halekas7, Roberto Livi8, Davin E Larson9, Ali Rahmati8, Phyllis Whittlesey8, Marco C M Velli10, Zesen Huang11, Orlando Romeo12, Christopher John Owen13, Timothy Simon Horbury14, Tamar Ervin9,15, Stuart D Bale12 and Nour E. Raouafi16, (1)Harvard-Smithsonian Center for Astrophysics, Cambridge, United States, (2)CEA Saclay DSM / LSCE, Gif sur Yvette, France, (3)Harvard-Smithsonian Center for Astrophysics, Cambridge, MA, United States, (4)University of Arizona, Lunar and Planetary Laboratory, Tucson, United States, (5)Smithsonian Astrophysical Observatory, Cambridge, MA, United States, (6)University of New Hampshire, Chelmsford, United States, (7)University of Iowa, Physics and Astronomy, Iowa City, United States, (8)University of California Berkeley, Space Sciences Laboratory, Berkeley, United States, (9)Space Sciences Laboratory, Berkeley, United States, (10)Earth, Planetary, and Space Sciences, University of California, Los Angeles, United States, (11)Department of Earth, Planetary and Space Sciences, University of California Los Angels, Los Angels, United States, (12)University of California Berkeley, Space Sciences Laboratory, Berkeley, CA, United States, (13)UCL, Mullard Space Science Laboratory, Dorking, United Kingdom, (14)Imperial College London, Department of Physics, London, SW7, United Kingdom, (15)University of California, Berkeley, Space Sciences Laboratory, Berkeley, United States, (16)Applied Physics Laboratory Johns Hopkins, Laurel, MD, United States