Magnetic Reconnection in the Heliotail as a Source for the INCA Belt
Magnetic Reconnection in the Heliotail as a Source for the INCA Belt
Marc Zachary Kornbleuth1, Merav Opher2, James Frederick Drake3, Marc Swisdak4, Zhiyu Yin3, Kostas Dialynas5, Yuxi Chen6, Justyna Sokół7, Matina Gkioulidou8, Igor Baliukin9, Vladislav Izmodenov10 and Gary P Zank11, (1)Boston University, Boston, MA, United States, (2)Boston University, Astronomy, Boston, MA, United States, (3)University of Maryland College Park, College Park, MD, United States, (4)University of Maryland, College Park, United States, (5)Office for Space Research and Technology, Academy of Athens, Athens, Greece, (6)Princeton Plasma Physics Laboratory, Princeton, United States, (7)Southwest Research Institute, San Antonio, United States, (8)Johns Hopkins University Applied Physics Laboratory, Laurel, United States, (9)Space Research Institute of Russian Academy of Sciences, Moscow, Russia, (10)Space Res Institute (IKI) Russian Academy of Sciences, Moscow, Russia, (11)Center for Space Plasma and Aeronomic Research, Department of Space Science, The University of Alabama in Huntsville, Huntsville, United States