On the Energization of Pickup Ions Downstream of the Heliospheric Termination Shock by Comparing 0.52–55 keV Observed Energetic Neutral Atom Spectra to Ones Inferred from Proton Hybrid Simulations
Matina Gkioulidou1, Merav Opher2, Marc Zachary Kornbleuth3, Kostas Dialynas4, Joe Giacalone5, John D Richardson6, Gary P Zank7, Stephen A Fuselier8, Donald G Mitchell1, Stamatios Mike Krimigis9, Elias Roussos10 and Igor Baliukin11, (1)Johns Hopkins University Applied Physics Laboratory, Laurel, MD, United States, (2)Boston University, Astronomy, Boston, MA, United States, (3)Boston University, Boston, MA, United States, (4)Office for Space Research and Technology, Academy of Athens, Athens, Greece, (5)University of Arizona, Planetary Sciences, Tucson, AZ, United States, (6)MIT, Cambridge, MA, United States, (7)Center for Space Plasma and Aeronomic Research, Department of Space Science, The University of Alabama in Huntsville, Huntsville, United States, (8)Southwest Research Institute, San Antonio, TX, United States, (9)Academy of Athens, Space, Athens, Greece, (10)Max Planck Institute for Solar System Research, Göttingen, Germany, (11)Space Research Institute of Russian Academy of Sciences, Moscow, Russia
