On the Spatial Homogeneity of the H2O Coma of 67P/C.-G. at 3.9-3.5 AU as Seen from MIRO
Christopher Jarchow1, Ladislav Rezac1, Paul Hartogh2, Samuel Gulkis3, Mark Allen4, Paul A A Von Allmen4, Gerard Beaudin5, Nicolas Biver6, Dominique Bockelée-Morvan7, Mathieu Choukroun8, Jacques Crovisier9, Pierre Encrenaz5, Therese Encrenaz10, Margaret A. Frerking11, Mark D Hofstadter12, Wing-Huen Ip13, Michael A Janssen4, Seungwon Lee14, Emmanuel Lellouch15, Cedric Leyrat16, F. Peter Schloerb17 and Thomas R Spilker18, (1)Max Planck Institute for Solar System Research, Katlenburg-Lindau, Germany, (2)Max Planck Institute for Solar System Research, Göttingen, Germany, (3)California Institute of Technology, Pasadena, CA, United States, (4)NASA Jet Propulsion Laboratory, Pasadena, CA, United States, (5)Observatoire de Paris, LERMA, Paris, France, (6)Observatoire de Paris, Paris, France, (7)Paris Observatory, Paris, France, (8)Jet Propulsion Laboratory, Pasadena, United States, (9)LESIA Observatoire de Paris, Meudon, France, (10)Paris Observatory-PSL, LIRA, Meudon, France, (11)Jet Propulsion Laboratory, Pasadena, CA, United States, (12)Jet Propulsion Laboratory/California Institute of Technology, Pasadena, CA, United States, (13)National Central University, Institute of Astronomy, Taoyuan City, Taiwan, (14)NASA Jet Propulsion Laboratory, Pasadena, United States, (15)LESIA, Observatoire de Paris, Paris, France, (16)Paris Observatory Meudon, Meudon, France, (17)University of Massachusetts Amherst, Amherst, MA, United States, (18)Independent Consultant, Pasadena, CA, United States
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