Implications for Nucleus Heterogeneity from the Comparison of Pre- and Post-Equinox Neutral ROSINA Observations Inbound and Outbound Beyond 3 AU
Adrienn Luspay-Kuti1, Kathrin Altwegg2, Jean-Jacques Berthelier3, Arnaud Beth4, Frederik Dhooghe5, Björn Fiethe6, Stephen A Fuselier1, Tamas I Gombosi7, Kenneth C Hansen8, Myrtha Hässig2, Urs Mall9, Kathleen Mandt10, Olivier Mousis11, Petrinec M Steven12, Martin Rubin13, Karlheinz J Trattner14, Chia-Yu Tzou2 and Peter Wurz15, (1)Southwest Research Institute, San Antonio, TX, United States, (2)University of Bern, Physikalisches Institut, Bern, Switzerland, (3)CNRS, Paris Cedex 16, France, (4)Imperial College London, London, United Kingdom, (5)Belgian Institute for Space Aeronomy, Brussels, Belgium, (6)Technical University of Braunschweig, Braunschweig, Germany, (7)University of Michigan, Climate and Space Sciences and Engineering, Ann Arbor, United States, (8)University of Michigan, Ann Arbor, MI, United States, (9)Max Planck Institute for Solar System Research, Planets and Comets, Goettingen, Germany, (10)Applied Physics Laboratory Johns Hopkins, Laurel, MD, United States, (11)Aix-Marseille Université, CNRS, CNES, Institut Origines, LAM, Marseille, France, (12)Lockheed Martin Advanced Technology Center, Palo Alto, CA, United States, (13)Physikalisches Institut, University of Bern, Bern, Switzerland, (14)Laboratory for Atmospheric and Space Physics, Boulder, CO, United States, (15)University of Bern, Space Research and Planetary Sciences, Bern, Switzerland
