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Abstract: Direct evidence of Synchrotron radiation from near-Sun traveling shock waves (AGU25)

Direct evidence of Synchrotron radiation from near-Sun traveling shock waves

Immanuel Christopher Jeba Raj1, Oleksiy V Agapitov2, Michael Gedalin3, Laura Vuorinen4, Vladimir Krasnoselskikh5, Michael A Balikhin6, Andrii Voshchepynets7, Athanasios Kouloumvakos8, J. Grant Mitchell9, Marc Pulupa10, Nina Dresing4, Rami O Vainio1, Allan Wayne Labrador11, Christina Cohen12, Nicolas Wijsen13, Lucas Colomban5, David J McComas14 and Stuart D Bale10, (1)University of Turku, Turku, Finland, (2)Space Science Laboratory, UCB, Berkeley, United States, (3)Ben-Gurion University of the Negev, Beer Sheva, Israel, (4)University of Turku, Department of Physics and Astronomy, Turku, Finland, (5)Laboratoire de Physique et Chimie de l'Environnement et de l'Espace, Orléans Cedex 2, France, (6)Univ Sheffield, Sheffield, United Kingdom, (7)IRF Swedish Institute of Space Physics Kiruna, Kiruna, Sweden, (8)The Johns Hopkins University. Applied Physics Laboratory, Laurel, United States, (9)NASA Goddard Space Flight Center, Greenbelt, MD, United States, (10)University of California Berkeley, Space Sciences Laboratory, Berkeley, CA, United States, (11)Mail Code 290-17, Pasadena, CA, United States, (12)Caltech, Pasadena, United States, (13)KU Leuven, Leuven, Belgium, (14)Princeton University, Department of Astrophysical Sciences, Princeton, United States