How Numerical Magnetic Dissipation at the Heliospheric Current Sheet Affects Model Predictions at Voyager 1 and Results from a Kinetic-MHD Model of the Heliosphere within SWMF

Adam Michael, Johns Hopkins University Applied Physics Laboratory, Laurel, MD, United States, Merav Opher, Boston University, Astronomy, Boston, MA, United States, Gabor Toth, University of Michigan Ann Arbor, Department of Climate and Space Sciences and Engineering, Ann Arbor, MI, United States, Dmitry Borovikov, University of Michigan Ann Arbor, Ann Arbor, MI, United States, Valeriy Tenishev, University of Michigan, Climate and Space Sciences and Engineering, Ann Arbor, United States and Elena Provornikova, US Naval Research Laboratory, Washington, DC, United States
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