Shock erosion caused by cavitons and spontaneous hot flow anomalies in a hybrid-Vlasov global simulation
Xochitl Blanco-Cano1, Markus Batttarbee2, Lucile Turc2, Andrew P Dimmock3, K Emilia J Kilpua2, Sanni Hoilijoki4, Urs Ganse2, David G Sibeck5, Paul Cassak6, Robert C Fear7, Riku Jarvinen8, Liisa Juusola9, Yann Pfau-Kempf2, Rami O Vainio10 and Minna Palmroth2, (1)Instituto de Geofísica Universidad Nacional Autónoma de México, Mexico City, Mexico, (2)University of Helsinki, Department of Physics, Helsinki, Finland, (3)IRF Swedish Institute of Space Physics Uppsala, Uppsala, Sweden, (4)Laboratory for Atmospheric and Space Physics, Boulder, United States, (5)NASA Goddard Space Flight Center, Greenbelt, MD, United States, (6)West Virginia University, Department of Physics and Astronomy, Morgantown, United States, (7)University of Southampton, School of Physics & Astronomy, Southampton, United Kingdom, (8)Finnish Meteorological Inst, Helsinki, Finland, (9)Finnish Meteorological Institute, Helsinki, Finland, (10)University of Turku, Turku, Finland
