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Abstract: Identifying large scale structures in the solar wind with a simple derivative analysis (AGU25)

Identifying large scale structures in the solar wind with a simple derivative analysis

Tatiana Niembro Hernandez1, Alejandro Lara2, Nishu Karna3, Sergio Vidal-Luengo4, Denny Oliveira5, Daniel T Welling6, Srijan Bharati Das7, Michael Louis Stevens8, Kristoff W Paulson9, Samuel Timothy Badman10, Yeimy Rivera11, Federico Fraschetti3 and Lidiya Ahmed12, (1)Smithsonian Astrophysical Observatory, Cambridge, United States, (2)Universidad Nacional Autonoma de Mexico, Mexico City, Mexico, (3)Harvard-Smithsonian Center for Astrophysics, Cambridge, MA, United States, (4)Laboratory for Atmospheric and Space Physics, Boulder, CO, United States, (5)GSFC/UMBC, Greenbelt, United States, (6)University of Michigan, Ann Arbor, MI, United States, (7)Princeton University, Princeton, United States, (8)Smithsonian Astrophysical Observatory, Cambridge, MA, United States, (9)University of New Hampshire, Chelmsford, United States, (10)University of Oxford, Oxford, United Kingdom, (11)Harvard-Smithsonian Center for Astrophysics, Cambridge, United States, (12)Center for Astrophysics | Harvard & Smithsonian, Cambridge, United States
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