The Carbon Content in Comet 67P/Churyumov-Gerasimenko from Rosetta/ROSINA

Martin Rubin1, Kathrin Altwegg2, Hans Balsiger3, Jean-Jacques Berthelier4, Michael R Combi5, Johan De Keyser6, Maria N. Drozdovskaya7, Bjorn Fiethe8, Stephen A Fuselier9, Sébastien Gasc2, Tamas I Gombosi10, Nora P. Hänni2, Kenneth C Hansen10, Urs Mall11, Henri Reme12, Isaac R. H. G. Schroeder2, Markus Schuhmann2, Thierry Semon2, Jack H Waite Jr13, Susanne F. Wampfler7 and Peter Wurz1, (1)University of Bern, Physics Institute, Space Research and Planetary Sciences, Bern, Switzerland, (2)University of Bern, Physikalisches Institut, Bern, Switzerland, (3)University of Bern, Bern, Switzerland, (4)LATMOS Laboratoire Atmosphères, Milieux, Observations Spatiales, Paris Cedex 05, France, (5)Univ Michigan, Ann Arbor, MI, United States, (6)Belgian Institute for Space Aeronomy, Brussels, Belgium, (7)University of Bern, Center for Space and Habitability, Bern, Switzerland, (8)Technical University of Braunschweig, Braunschweig, Germany, (9)Southwest Research Institute, San Antonio, TX, United States, (10)University of Michigan, Ann Arbor, MI, United States, (11)Max Planck Institute for Solar System Research, Planets and Comets, Goettingen, Germany, (12)CNRS, Paris Cedex 16, France, (13)Southwest Research Institute, Space Sciences and Engineering, San Antonio, TX, United States