Automatic Detection of Magnetic Reconnection: Solar Orbiter Reveals that Reconnection Jets Cluster in the Solar Wind

Naïs Fargette1, Benoit Lavraud2, Alexis P Rouillard3, Tai Phan4, Marit Oieroset5, Jonathan P Eastwood6, Philippe Louarn7, Andrei Fedorov7, Lubomir Prech8, Roberto Bruno9, Jim M Raines10, Stefano A Livi11, Christopher John Owen12 and Timothy Simon Horbury13, (1)IRAP, Toulouse, France, (2)Institut de Recherche en Astrophysique et Planétologie, Toulouse, France, (3)Université Toulouse III - Paul Sabatier, Observatoire Midi–Pyrénées, CNRS, CNES, IRAP, Toulouse, France, (4)University of California Berkeley, Berkeley, United States, (5)Univ California, Berkeley, CA, United States, (6)Imperial College London, Physics, London, SW7, United Kingdom, (7)IRAP, CNRS, Toulouse, France, (8)Charles University Prague, Prague 8, Czech Republic, (9)IAPS-INAF, Rome, Italy, (10)University of Michigan, Ann Arbor, MI, United States, (11)SwRI, San Antonio, TX, United States, (12)University College London, Mullard Space Science Laboratory, Dorking, United Kingdom, (13)Imperial College London, Department of Physics, London, SW7, United Kingdom