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Abstract: Quantifying Proton Heat Flux in Solar Wind Switchbacks Using a Gyrotropic Slepian Basis Reconstruction (AGU25)

Quantifying Proton Heat Flux in Solar Wind Switchbacks Using a Gyrotropic Slepian Basis Reconstruction

Michael Terres1, Srijan Bharati Das2, Roberto Livi3, Davin E Larson4, Michael Louis Stevens5, Kristoff W Paulson6, Jaye Verniero7, Samuel Timothy Badman2, Yeimy Rivera6 and Andrea Larosa8, (1)Smithsonian Astrophysical Observatory, Cambridge, United States, (2)Harvard-Smithsonian Center for Astrophysics, Cambridge, MA, United States, (3)University of California Berkeley, Space Sciences Laboratory, Berkeley, United States, (4)Space Sciences Laboratory, Berkeley, United States, (5)Smithsonian Astrophysical Observatory, Cambridge, MA, United States, (6)Harvard-Smithsonian Center for Astrophysics, Cambridge, United States, (7)NASA Goddard Space Flight Center, Code 672, Greenbelt, United States, (8)Laboratoire de Physique et Chimie de l'Environnement et de l'Espace, Orléans Cedex 2, France