Solar Wind protons: Gaussian and Inverse-Gaussian components
Solar Wind protons: Gaussian and Inverse-Gaussian components
Philippe Louarn1, Andrei Fedorov2, Benoit Lavraud1, Alexis P Rouillard3, Vincent N Genot1, Illya Plotnikov1, Victor Réville3, Naïs Fargette1, Rungployphan Om Kieokaew4, Emmanuel Penou5, Alain Barthe2, Lubomir Prech6, Tereza Durovcova7, Roberto Bruno8, Raffaella D'Amicis9, Jim M Raines10, Stefano A Livi11, Matthieu Berthomier12, Christopher John Owen13, Milan Maksimovic14, Timothy Simon Horbury15, Stuart D Bale16, Justin Kasper17 and Pierre Trottier1, (1)IRAP, Toulouse, France, (2)IRAP, CNRS, Toulouse, France, (3)Université Toulouse III - Paul Sabatier, Observatoire Midi–Pyrénées, CNRS, CNES, IRAP, Toulouse, France, (4)Mahidol University, Bangkok, Thailand, (5)Universite Paul Sabatier, TOULOUSE, France, (6)Charles University Prague, Prague 8, Czech Republic, (7)Charles University, Prague, Czech Republic, (8)INAF-IFSI, Rome, Italy, (9)National Institute for Astrophysics, Institute for Space Astrophysics and Planetology, Rome, Italy, (10)University of Michigan, Ann Arbor, MI, United States, (11)SwRI, San Antonio, TX, United States, (12)LPP, Ecole Polytechnique, UPMC, Paris, France, (13)University College London, Mullard Space Science Laboratory, Dorking, United Kingdom, (14)LESIA, Observatoire de Paris, Université PSL, CNRS, Sorbonne Université, Université de Paris, Meudon, France, (15)Imperial College London, Department of Physics, London, SW7, United Kingdom, (16)University of California Berkeley, Space Sciences Laboratory, Berkeley, CA, United States, (17)University of Michigan, Ann Arbor, United States