The Noble Gas Abundances in the Coma of Comet 67P/Churyumov-Gerasimenko from Rosetta/ROSINA

Martin Rubin1, Kathrin Altwegg1, Hans R Balsiger2, Jean-Jacques Berthelier3, Christelle Briois4, Michael R Combi5, Johan De Keyser6, Björn Fiethe7, Stephen A Fuselier8, Sébastien Gasc1, Tamas I Gombosi9, Kenneth C Hansen10, Annette Jäckel1, Ernest Kopp1, Axel Korth11, Urs Mall12, Bernard Marty13, Olivier Mousis14, Tobias Owen15, Henri Reme6, Markus Schuhmann1, Isaac R. H. G. Schroeder1, Thierry Semon1, Chia-yu Tzou1, Jack H Waite Jr16 and Peter Wurz1, (1)University of Bern, Physikalisches Institut, Bern, Switzerland, (2)Physikalisches Institut, University of Bern, Bern, Switzerland, (3)CNRS, Paris Cedex 16, France, (4)Laboratoire de Physique et Chimie de l'Environnement et de l'Espace, LPC2E, Orléans Cedex 2, France, (5)Univ Michigan, Ann Arbor, MI, United States, (6)Belgian Institute for Space Aeronomy, Brussels, Belgium, (7)Technical University of Braunschweig, Braunschweig, Germany, (8)Southwest Research Institute, San Antonio, TX, United States, (9)Univ of Michigan, Ann Arbor, MI, United States, (10)University of Michigan, Ann Arbor, MI, United States, (11)Max Planck Institute for Solar System Research, Katlenburg-Lindau, Germany, (12)Max-Planck-Institut für Sonnensystemforschung, Göttingen, Germany, (13)CRPG Centre de Recherches Pétrographiques et Géochimiques, Vandoeuvre-Les-Nancy, France, (14)Aix Marseille Université, CNRS, LAM (Laboratoire d'Astrophysique de Marseille), Marseille, France, (15)University of Hawaii, Institute for Astronomy, Honolulu, HI, United States, (16)Department of Space Science, Southwest Research Institute, San Antonio, United States