P41C:
Rosetta 2014 IV Posters

Thursday, 18 December 2014: 8:00 AM-12:20 PM
Primary Convener:  Matthew G Taylor, ESA/ESTEC, Noordwijk, Netherlands
Co-Convener:  Claudia J Alexander, JPL, Pasadena, CA, United States

Abstracts Submitted to this Session:

 
Rosetta Mission Status Update
Matthew G Taylor1, Nicolas Altobelli2, Claudia J Alexander3, Gerhard H Schwehm4, Fred Jansen2,4, Michael Küppers5, Laurence O'Rourke2, Maud Barthelemy2, Bernhard Geiger2, Bjorn Grieger2, Richard Moissl2 and Claire Vallat6, (1)ESTEC, Noordwijk, 2201, Netherlands, (2)European Space Agency, Villanueva de la Canada, Spain, (3)Jet Propulsion Laboratory, Pasadena, CA, United States, (4)ESTEC, Noordwijk, Netherlands, (5)European Space Agency, Villanueva De La Can, Spain, (6)ESAC, Villanueva, Spain
 
Philae - Landing on a Comet
Stephan Ulamec1, Jens Biele1, Cedric Delmas2, Cinzia Fantinati1, Philippe Gaudon2, Koen Geurts1, Eric Jurado2, Michael Maibaum1, Reinhard Roll3, Mario Salatti4 and Lars Witte5, (1)German Aerospace Center DLR Cologne, Cologne, Germany, (2)CNES French National Center for Space Studies, Toulouse Cedex 09, France, (3)Max Planck Institute for Solar System Research, Katlenburg-Lindau, Germany, (4)Italian Space Agency, Rome, Italy, (5)German Aerospace Center DLR Bremen, Bremen, Germany
 
Close-up multispectral images of the surface of comet 67P/Churyumov-Gerasimenko by the ROLIS camera onboard the Rosetta Philae lander
Stefan Schroeder1, Stefano Mottola1, Gabriele Arnold1, Hans-Georg Grothues2, Ralf Jaumann1, Harald Michaelis1, Gerhard Neukum3, Ivanka Pelivan1 and Jean-Pierre Bibring4, (1)German Aerospace Center DLR Berlin, Berlin, Germany, (2)DLR, Space Management, Space Science, Bonn, Germany, (3)Free University of Berlin, Berlin, Germany, (4)IAS Institut d'Astrophysique Spatiale, Orsay Cedex, France
 
Full-Waveform Inversion Method for Data Measured by the CONSERT Instrument aboard Rosetta
Christoph Statz1, Dirk Plettemeier1, Alain Herique2 and Wlodek W Kofman2, (1)Dresden University of Technology, Dresden, Germany, (2)University Joseph Fourier Grenoble, Grenboble, France
 
Reconstructing the Surface Permittivity Distribution from Data Measured by the CONSERT Instrument aboard Rosetta: Method and Simulations
Dirk Plettemeier1, Christoph Statz1, Sebastian Hegler1, Alain Herique2 and Wlodek W Kofman2, (1)Dresden University of Technology, Dresden, Germany, (2)University Joseph Fourier Grenoble, Grenboble, France
 
Rosetta Consert Radio Sounding Experiment: A Numerical Method for the Inverse Problem
Mael Cardiet1, Alain Herique1, Yves Rogez1, Sylvain Douté2 and Wlodek W Kofman1, (1)University Joseph Fourier Grenoble, Grenboble, France, (2)CNRS, Grenoble Cedex 09, France
 
First Results from the RPC Magnetometer Experiment during the Approach Phase to 67P/Churyumov-Gerasimenko
Ingo Richter1, Karl-Heinz Glassmeier1, Christoph Koenders1, Chris Carr2, Emanuele Cupido2, Claire Vallat3, Uwe M Motschmann1, Bruce T. Tsurutani4 and Martin Volwerk5, (1)Technical University of Braunschweig, Braunschweig, Germany, (2)Imperial College London, London, United Kingdom, (3)ESAC, Villanueva, Spain, (4)NASA Jet Propulsion Laboratory, Pasadena, CA, United States, (5)Austrian Academy of Sciences, Graz, Austria
 
First Rosetta Observations of the Cometary Plasma at Churyumov–Gerasimenko with the Mutual Impedance Probe (RPC-MIP)
Pierre Henri1, Jean-Pierre Lebreton1, Christian Béghin1, Pierrette Décréau1, Anders I Eriksson2, Johann Geiswiller3, Rejean Grard4, Michel Hamelin5, Christian Xavier Mazelle6, Orélien Randriamboarison1, Walter Schmidt7, Jean-Gabriel Trotignon1, Gaétan Wattieaux8, Daniel Winterhalter9, Youcef Aouad1, Dominique Lagoutte1, Xavier Vallières1, Chris Carr10 and Emanuele Cupido10, (1)Laboratoire de Physique et Chimie de l'Environnement et de l'Espace (LPC2E) - CNRS - Université d'Orléans, Orléans, France, (2)IRF Swedish Institute of Space Physics Uppsala, Uppsala, Sweden, (3)DGA/DO/UM AMS/SM-ACEA, Bagneux, France, (4)European Space Research and Technology Centre, Noordwijk, Netherlands, (5)UPMC (Univ. Paris) / LATMOS, Paris, France, (6)University Paul Sabatier Toulouse III, Toulouse Cedex 09, France, (7)Finnish Meteorological Institute, Helsinki, Finland, (8)University Paul Sabatier Toulouse III, Laboratoire Plasma et Conversion d'Energie, Toulouse Cedex 09, France, (9)NASA Jet Propulsion Laboratory, Pasadena, CA, United States, (10)Imperial College London, London, United Kingdom
 
Recommended values and correlations of thermophysical properties for comet modelling
Ivanka Pelivan1, Jens Biele2, Ekkehard Kuhrt3, Björn Davidsson4, Mathieu Choukroun5 and Claudia J Alexander5, (1)German Aerospace Center DLR Berlin, Berlin, Germany, (2)German Aerospace Center DLR Cologne, Cologne, Germany, (3)DLR, Berlin, Germany, (4)Uppsala University, Uppsala, Sweden, (5)Jet Propulsion Laboratory, Pasadena, CA, United States
 
CONSERT Link Budget Simulator for the Direct Path
Ronny Hahnel1, Christoph Statz1, Dirk Plettemeier1, Wlodek W Kofman2, Alain Herique2 and Sonia Zine2, (1)Dresden University of Technology, Dresden, Germany, (2)University Joseph Fourier Grenoble, Grenboble, France
 
First Results at 67P/Churyumov-Gerasimenko with the Ion Composition Analyzer of the Rosetta Plasma Consortium
Hans Nilsson1, Gabriella Stenberg1, Etienne Behar1, Rickard N A Lundin2, Stas Barabash1, Chris Carr3, Emanuele Cupido3, James L Burch4, Andrei Fedorov5, Jean-Andre Sauvaud6, Hannu E J Koskinen7, Esa Jukka Kallio8, Jean-Pierre Lebreton9, Anders I Eriksson10, Karl-Heinz Glassmeier11, Raymond Goldstein12, Pierre Henri13, Christoph Koenders11, Pat Mokashi4, Zoltan Nemeth14, Ingo Richter11, Karoly Szego15 and Claire Vallat16, (1)IRF Swedish Institute of Space Physics Kiruna, Kiruna, Sweden, (2)IRF Swedish Institute of Space Physics Umeå, Umeå, Sweden, (3)Imperial College London, London, United Kingdom, (4)Southwest Research Institute San Antonio, San Antonio, TX, United States, (5)IRAP, Toulouse, France, (6)IRAP/CNRS, Toulouse, France, (7)University of Helsinki, Helsinki, Finland, (8)Finnish Meteorological Institute, Helsinki, Finland, (9)University of Orleans, Orleans, France, (10)IRF Swedish Institute of Space Physics Uppsala, Uppsala, Sweden, (11)Technical University of Braunschweig, Braunschweig, Germany, (12)Southwest Research Institute, San Antonio, TX, United States, (13)Laboratoire de Physique et Chimie de l'Environnement et de l'Espace, Orléans Cedex 2, France, (14)Wigner Research Center for Physics, Budapest, Hungary, (15)Hungarian Academy of Sciences, Budapest, Hungary, (16)ESAC, Villanueva, Spain
 
The Rosetta Ion and Electron Sensor (IES) Measurement of the Development of Pickup Ions from Comet 67P/Churyumov-Gerasimenko
Raymond Goldstein1, James L Burch2, Pat Mokashi1, Craig J Pollock3, Tom Broiles1, Kathleen Mandt2, Thomas Cravens4, Marilia Samara3, Anders I Eriksson5, Chris Carr6, Jean-Pierre Lebreton7, Pierre Henri8, Karl-Heinz Glassmeier9, Hans Nilsson10 and Christoph Koenders9, (1)Southwest Research Institute, San Antonio, TX, United States, (2)Southwest Research Institute San Antonio, San Antonio, TX, United States, (3)NASA Goddard Space Flight Center, Greenbelt, MD, United States, (4)University of Kansas, Lawrence, KS, United States, (5)IRF Swedish Institute of Space Physics Uppsala, Uppsala, Sweden, (6)Imperial College, London, United Kingdom, London, United Kingdom, (7)University of Orleans, Orleans, France, (8)Laboratoire de Physique et Chimie de l'Environnement et de l'Espace, Orléans Cedex 2, France, (9)Technical University of Braunschweig, Braunschweig, Germany, (10)IRF Swedish Institute of Space Physics Kiruna, Kiruna, Sweden
 
Early Observations with the Rosetta Langmuir Probe Instrument at the Target Comet
Anders I Eriksson1, Niklas J. T. Edberg1, Reine Gill1, Fredrik Johansson1, Elias Odelstad1, Jan-Erik Wahlund1, Erik Vigren1, Tomas Karlsson2, Per-Arne Lindqvist2, Riku Jarvinen3, Bjorn Lybekk4, Wojciech Miloch4, Arne Pedersen4, Jean-Pierre Lebreton5, Chris Carr6 and Emanuele Cupido6, (1)IRF Swedish Institute of Space Physics Uppsala, Uppsala, Sweden, (2)KTH Royal Institute of Technology, Stockholm, Sweden, (3)Finnish Meteorological Inst, Helsinki, Finland, (4)University of Oslo, Department of Physics, Oslo, Norway, (5)University of Orleans, Orleans, France, (6)Imperial College London, London, United Kingdom
 
Ion and Electron Sensor Observations on Photoelectrons and Coma Development at Comet 67P/Churyumov-Gerasimenko
James L Burch1, Raymond Goldstein1, Pat Mokashi1, Craig J Pollock2, Tom Broiles1, Kathleen Mandt1, Thomas Cravens3, Marilia Samara2, Anders I Eriksson4, Chris Carr5, Jean-Pierre Lebreton6, Pierre Henri6, Karl-Heinz Glassmeier7, Hans Nilsson8 and Christoph Koenders7, (1)Southwest Research Institute, San Antonio, TX, United States, (2)NASA Goddard Space Flight Center, Greenbelt, MD, United States, (3)University of Kansas, Lawrence, KS, United States, (4)IRF Swedish Institute of Space Physics Uppsala, Uppsala, Sweden, (5)Imperial College London, London, United Kingdom, (6)Laboratoire de Physique et Chimie de l'Environnement et de l'Espace, Orléans Cedex 2, France, (7)Technical University of Braunschweig, Braunschweig, Germany, (8)IRF Swedish Institute of Space Physics Kiruna, Kiruna, Sweden
 
Can Rosetta IES Measure Charged Dust Grains at Comet 67P/C-G?
George B Clark1,2, Craig J Pollock2, Raymond Goldstein3, Marilia Samara2, Thomas W Broiles3, Kathleen Mandt4, James L Burch4 and Zoltan Sternovsky5, (1)Catholic University of America, Washington, DC, United States, (2)NASA Goddard Space Flight Center, Greenbelt, MD, United States, (3)Southwest Research Institute, San Antonio, TX, United States, (4)Southwest Research Institute San Antonio, San Antonio, TX, United States, (5)Colorado Univ, Boulder, CO, United States
 
Structure and Dynamics of the Interaction Region at Comet 67P/Churyumov-Gerasimenko: Comparing Numerical Simulations and RPC Magnetic Field Observations
Christoph Koenders1, Karl-Heinz Glassmeier1, Ingo Richter1, Charlotte Goetz1, Chris Carr2, Emanuele Cupido2, Claire Vallat3 and Uwe M Motschmann1, (1)Technical University of Braunschweig, Braunschweig, Germany, (2)Imperial College London, London, United Kingdom, (3)ESAC, Villanueva, Spain
 
Does 67P/C-G Have a Dusty Plasma Environment?
Tamas I Gombosi, Univ of Michigan, Ann Arbor, MI, United States
 
A Multi-neutral-fluid model of comet 67P/Churyumov-Gerasimenko
Yinsi Shou1, Michael R Combi2, Tamas I Gombosi3, Xianzhe Jia1, Gabor Toth2, Kenneth C Hansen1, Valeriy Tenishev1 and Nicolas Fougere4, (1)University of Michigan, Ann Arbor, MI, United States, (2)Univ Michigan, Ann Arbor, MI, United States, (3)Univ of Michigan, Ann Arbor, MI, United States, (4)University of Michigan Ann Arbor, Ann Arbor, MI, United States
 
Giada improved calibration of measurement subsystems
Vincenzo Della Corte1, Alessandra Rotundi2, Roberto Sordini1, Mario Accolla2, Marco Ferrari1, Stavro Ivanovski1, Francesca Lucarelli2, Elena Mazzotta Epifani3 and Pasquale Palumbo2, (1)IAPS-INAF, Rome, Italy, (2)Parthenope University of Naples, Scienze e Tecnologie, Naples, Italy, (3)INAF, OAC, Naples, Italy
 
A Computer-assisted Method for the Calibration of Raw Data from the DFMS sensor on Rosetta
Frederik Dhooghe1, Johan De Keyser1, Romain Maggiolo1, Kathrin Altwegg2, Ursina Calmonte2, Stephen Fuselier3, Myrtha Hässig3, Jean-Jacques Berthelier4, Urs A. Mall5, Tamas I Gombosi6 and Björn Fiethe7, (1)Belgian Institute for Space Aeronomy, Brussels, Belgium, (2)University of Bern, Bern, Switzerland, (3)Southwest Research Institute San Antonio, San Antonio, TX, United States, (4)LATMOS Laboratoire Atmosphères, Milieux, Observations Spatiales, Paris Cedex 05, France, (5)Max Planck Institute for Solar System Research, Katlenburg-Lindau, Germany, (6)Univ of Michigan, Ann Arbor, MI, United States, (7)Technische Universitat Braunschweig, Braunschweig, Germany
 
First insights on the organic species from the high resolution mass spectrometer ROSINA DFMS on-board the Rosetta spacecraft
Lena Le Roy1, Kathrin Altwegg1, Jean-Jacques Berthelier2, Ursina Calmonte1, Frederik Dhooghe3, Bjoern Fiethe4, Stephen Fuselier5, Tamas I Gombosi6, Martin Rubin1 and Chia-yu Tzou1, (1)University of Bern, Bern, Switzerland, (2)LATMOS Laboratoire Atmosphères, Milieux, Observations Spatiales, Paris Cedex 05, France, (3)Belgian Institute for Space Aeronomy, Brussels, Belgium, (4)Technical University of Braunschweig, Braunschweig, Germany, (5)Southwest Research Institute San Antonio, San Antonio, TX, United States, (6)Univ of Michigan, Ann Arbor, MI, United States
 
Multifluid MHD Simulations of the Plasma Environment of Comet Churyumov-Gerasimenko at Different Heliocentric Distances
Zhenguang Huang1, Xianzhe Jia1, Martin Rubin2, Nicolas Fougere1, Tamas I Gombosi1, Valeriy Tenishev1, Michael R Combi1, Andre Michel Bieler1, Gabor Toth1, Kenneth C Hansen1 and Yinsi Shou1, (1)University of Michigan, Ann Arbor, MI, United States, (2)University of Bern, Bern, Switzerland
 
In Situ Space Gas Dynamic Measurements by the ROSINA Comet Pressure Sensor COPS on the Rosetta Spacecraft
Chia-yu Tzou1, Kathrin Altwegg1, Björn Fiethe2, Sébastien Gasc1 and Martin Rubin1, (1)University of Bern, Bern, Switzerland, (2)Technical University of Braunschweig, Braunschweig, Germany
 
A 3D Description of the Coma of Comet 67P/Churyumov-Gerasimenko Constrained by Rosetta Observations
Nicolas Fougere1, Valeriy Tenishev1, Andre Michel Bieler1, Michael R Combi1, Tamas I Gombosi1, Kenneth C Hansen1, Xianzhe Jia1, Yinsi Shou1, Zhenguang Huang1, Gabor Toth1, Kathrin Altwegg2, Peter Wurz2, Hans Balsiger2, Annette Jäckel2, Lena Le Roy2, Sébastien Gasc2, Ursina Calmonte2, Martin Rubin2, Chia-yu Tzou2, Myrtha Hässig3, Stephen Fuselier3, Johan De Keyser4, Jean-Jacques Berthelier5, Urs A. Mall6, Henri Rème7 and Björn Fiethe8, (1)University of Michigan, Ann Arbor, MI, United States, (2)University of Bern, Bern, Switzerland, (3)Southwest Research Institute San Antonio, San Antonio, TX, United States, (4)Belgian Institute for Space Aeronomy, Brussels, Belgium, (5)LATMOS Laboratoire Atmosphères, Milieux, Observations Spatiales, Paris Cedex 05, France, (6)Max Planck Institute for Solar System Research, Katlenburg-Lindau, Germany, (7)IRAP, Institut de Recherche en Astrophysique et Planétologie, Toulouse, France, (8)Technical University of Braunschweig, Braunschweig, Germany
 
3D Direct Simulation Monte Carlo Modeling of the Spacecraft Environment of Rosetta
Andre Michel Bieler1, Valeriy Tenishev1, Nicolas Fougere1, Tamas I Gombosi1, Kenneth C Hansen1, Michael R Combi1, Zhenguang Huang1, Xianzhe Jia1, Gabor Toth1, Kathrin Altwegg2, Peter Wurz2, Annette Jäckel2, Lena Le Roy2, Sébastien Gasc2, Ursina Calmonte2, Martin Rubin2, Chia-yu Tzou2, Myrtha Hässig3, Stephen Fuselier3, Johan De Keyser4, Jean-Jacques Berthelier5, Urs A. Mall6, Henri Rème7, Björn Fiethe8 and Hans Balsiger2, (1)University of Michigan, Ann Arbor, MI, United States, (2)University of Bern, Bern, Switzerland, (3)Southwest Research Institute San Antonio, San Antonio, TX, United States, (4)Belgian Institute for Space Aeronomy, Brussels, Belgium, (5)LATMOS Laboratoire Atmosphères, Milieux, Observations Spatiales, Paris Cedex 05, France, (6)Max Planck Institute for Solar System Research, Katlenburg-Lindau, Germany, (7)IRAP, Institut de Recherche en Astrophysique et Planétologie, Toulouse, France, (8)Technical University of Braunschweig, Braunschweig, Germany
 
Measuring Oxygen Isotopes with COSIMA
John Anthony Paquette1, Cécile Engrand2, Oliver Stenzel1 and Martin Hilchenbach1, (1)Max Planck Institute for Solar System Research, Katlenburg-Lindau, Germany, (2)Centre de Sciences Nucléaires et de Sciences de la Matiere - CSNSM, 91405 Orsay, France
 
Optical Detection and Characterization of Cometary Grains Collected for Analysis by the COSIMA Mass Spectrometer on-board ROSETTA.
Yves Langevin1, Klaus Hornung2, Martin Hilchenbach3, Jochen Kissel3, Johan V Silen4, Christelle Briois5, Rita Schulz6, Donia Baklouti1 and Pascal Eng1, (1)IAS Institut d'Astrophysique Spatiale, Orsay Cedex, France, (2)Universität der Bundeswehr, 85577 Neubiberg, Germany, (3)Max Planck Institute for Solar System Research, Katlenburg-Lindau, Germany, (4)Finnish Meteorological Institute, Helsinki, Finland, (5)Laboratoire de Physique et Chimie de l'Environnement et de l'Espace, LPC2E, Orléans Cedex 2, France, (6)European Space Research and Technology Centre, Noordwijk, Netherlands
 
On the Inorganic Composition of Cometary Dust from Comet 67P/Churyumov-Gerasimenko, as Seen by COSIMA on Board ROSETTA.
Cécile Engrand1, Donia Baklouti2, Christelle Briois3, Hervé Cottin4, Henning Fischer5, Nicolas Fray4, Marie Godard1, Hartmut Henkel6, Martin Hilchenbach5, Klaus Hornung7, Jochen Kissel5, Andreas Koch6, Yves Langevin2, Harry Lehto8, Sihane Merouane5, François-Régis Orthous-Daunay9, Jouni Rynö10, Rita Schulz11, Johan V Silen10, Sandra Siljeström12, Thomas Stephan13, Laurent Thirkell3 and Kurt Varmuza14, (1)Centre de Sciences Nucléaires et de Sciences de la Matiere - CSNSM, 91405 Orsay, France, (2)IAS Institut d'Astrophysique Spatiale, Orsay Cedex, France, (3)Laboratoire de Physique et Chimie de l'Environnement et de l'Espace, CNRS / Université d’Orléans, 45071 Orléans, France, (4)LISA Laboratoire Interuniversitaire des Systèmes Atmosphériques, CRETEIL, France, (5)Max Planck Institute for Solar System Research, Katlenburg-Lindau, Germany, (6)von Hoerner und Sulger GmbH, 68723 Schwetzingen, Germany, (7)Universität der Bundeswehr, 85577 Neubiberg, Germany, (8)University of Turku, Turku, Finland, (9)IPAG - Institut de Planetologie et d'Astrophysique de Grenoble, Grenoble, France, (10)Finnish Meteorological Institute, Helsinki, Finland, (11)European Space Research and Technology Centre, Noordwijk, Netherlands, (12)SP Technical Research Institute of Sweden, Borås, Sweden, (13)The University of Chicago, Chicago, United States, (14)Technische Universität Wien, Wien, Austria
 
Morphological Forms of Cometary Activity
Horst Uwe Keller1, Michael F A'Hearn2, Olivier Groussin3, Stubbe Faurschou Hviid4, Ekkehard Kuhrt5, Nicolas Thomas6, Sebastien Besse7, Stefan Schroeder5 and Jean-Baptiste Vincent8, (1)Technical University of Braunschweig, Braunschweig, Germany, (2)University of Maryland, College Park, MD, United States, (3)Aix Marseille University, Marseille Cedex 03, France, (4)German Aerospace Center DLR Berlin, Berlin, Germany, (5)German Aerospace Center DLR Berlin, Institute of Planetary Research, Berlin, Germany, (6)University of Bern, Bern, Switzerland, (7)European Space Research and Technology Centre, Noordwijk, Netherlands, (8)Max-Planck Institute for Solar System Research, Germany, Goettigen, Germany
 
Geomorphology of Active Regions on Comet 67P/Churyumov-Gerasimenko from Osiris Observations
Anne-Thérèse Auger1,2, Olivier Groussin1, Laurent Jorda1, Sylvain Bouley2, Philippe L Lamy1, Gabriele Cremonese3, Nicolas Thomas4 and Holger Sierks5, (1)Laboratoire d'Astrophysique de Marseille, Marseille, France, (2)Laboratoire GEOPS, Orsay, France, (3)INAF - Astronomical Observatory of Padova, Padova, Italy, (4)University of Bern, Bern, Switzerland, (5)Max Planck Institute for Solar System Research, Katlenburg-Lindau, Germany
 
The Nucleus of Comet 67P/Churyumov-Gerasimenko : a New Case of Contact Binary ?
Philippe L Lamy1, Michael F A'Hearn2, Olivier Groussin1, Laurent Jorda1, Horst Uwe Keller3 and Hans Rickman4, (1)Laboratoire d'Astrophysique de Marseille, Marseille, France, (2)University of Maryland College Park, College Park, MD, United States, (3)Technical University of Braunschweig, Braunschweig, Germany, (4)Uppsala University, Department of Physics and Astronomy, Uppsala, Sweden
 
67P/Churyumov-Gerasimenko Spectrophotometric Properties
Sebastien Besse1, Sonia Fornasier2, Holger Sierks3, M. Antonietta Barucci2, Cedric Leyrat4, Stubbe Faurschou Hviid5, Laurent Jorda6, Horst Uwe Keller7, Michael Küppers1, Sara Magrin8, Matteo Massironi9, Nilda Oklay3, M. Pajola10, Nicolas Thomas11, C. Tubiana3, Colin Snodgrass12 and Jean-Baptiste Vincent13, (1)European Space Agency, Villanueva De La Can, Spain, (2)LESIA Observatoire de Paris, Meudon, France, (3)Max Planck Institute for Solar System Research, Katlenburg-Lindau, Germany, (4)Paris Observatory Meudon, Meudon, France, (5)German Aerospace Center DLR Berlin, Berlin, Germany, (6)Observatoire Astrophysique Marseille, Marseille, France, (7)Technical University of Braunschweig, Braunschweig, Germany, (8)CISAS - Center for Studies and Activities for Space, University of Padova, Padova, Italy, (9)Univ Padova, Padova, Italy, (10)CISAS-University of Padova, Padova, Italy, (11)University of Bern, Bern, Switzerland, (12)Max-Planck Institute for Solar System Research, Goettingen, Germany, (13)Max-Planck Institute for Solar System Research, Germany, Goettigen, Germany
 
Jets of 67P/Churyumov-Gerasimenko as Observed by Rosetta/OSIRIS
Wing-Huen Ip1, Z.-Y. Lin1, Luisa Lara2, Pedro Gutiérrez2, Rafael Rodrigo3, Michael F A'Hearn4, Jean-Baptiste Vincent5, Jessica Agarwal6, Ivano Bertini7, Steven Lowry8, A. Rozek8, M. Pajola9, Ian Lai10 and Yng Liao11, (1)NCU National Central University of Taiwan, Jhongli, Taiwan, (2)Instituto de Astrophisica de Andalucia-CSIC, Spain, Dept. of Solar System, Andalucia, Spain, (3)IAA-CSIC, Granada, Spain, (4)University of Maryland College Park, College Park, MD, United States, (5)Max-Planck Institute for Solar System Research, Goettingen, Germany, (6)Max-Planck Institute for Solar System Research, Germany, Goettigen, Germany, (7)CISAS - Center for Studies and Activities for Space, University of Padova, Padova, Italy, (8)University of Kent, UK, Center for Astrophysics and Planetary Science, Kent, United Kingdom, (9)CISAS-University of Padova, Padova, Italy, (10)Institute of Space Science National Central University, Jhongli, Taiwan, (11)University of Bern, Institute of Physics, Bern, Switzerland
 
The Geomorphology of Comet Churymov-Gerasimenko As Revealed By Rosetta/Osiris: Implicationsfor Past Collisional Evolution
Simone Marchi1, Michael F A'Hearn2, Cesare Barbieri3, M. Antonietta Barucci4, Sebastien Besse5, Gabriele Cremonese6, Wing-Huen Ip7, Horst Uwe Keller8, Detlef Koschny9, Ekkehard Kuhrt10, Philippe L Lamy11, Francesco Marzari3, Matteo Massironi12, Maurizio Pajola13, Hans Rickman14, Rafael Rodrigo15, Holger Sierks16, Colin Snodgrass17, Nicolas Thomas18 and Jean-Baptiste Vincent17, (1)Southwest Research Institute Boulder, Boulder, CO, United States, (2)University of Maryland College Park, College Park, MD, United States, (3)University of Padua, Padua, Italy, (4)Observatoire Paris, Paris, France, (5)European Space Agency, Villanueva De La Can, Spain, (6)INAF - Astronomical Observatory of Padova, Padova, Italy, (7)NCU National Central University of Taiwan, Jhongli, Taiwan, (8)Institute for Geophysics and Extraterrestrial Physics, Braunschweig, Germany, (9)European Space Research and Technology Centre, Noordwijk, Netherlands, (10)German Aerospace Center DLR Berlin, Berlin, Germany, (11)Astrophysics Laboratory of Marseilles, Marseilles, France, (12)Univ Padova, Padova, Italy, (13)CISAS - Center for Studies and Activities for Space, University of Padova, Padova, Italy, (14)Uppsala University, Department of Physics and Astronomy, Uppsala, Sweden, (15)IAA-CSIC, Granada, Spain, (16)Max Planck Institute for Solar System Research, Katlenburg-Lindau, Germany, (17)Max-Planck Institute for Solar System Research, Goettingen, Germany, (18)University of Bern, Bern, Switzerland
 
Multi-Resolution Stereophotoclinometry by Deformation, a New 3D Shape Reconstruction Method Applied to ROSETTA/OSIRIS Images
Claire Capanna1, Laurent Jorda1, Gilles Gesquière2, Robert W Gaskell3, Olivier Groussin1, Pedro Gutiérrez4, Stubbe Faurschou Hviid5, Philippe L Lamy1, Frank Preusker5, Sergey Rodionov1, Frank Scholten5 and Didier Vibert1, (1)Laboratoire d'Astrophysique de Marseille, Marseille, France, (2)Université Lumière, CNRS,, Laboratoire LIRIS (Laboratoire d'InfoRmatique en Image et Systèmes d'information) , UMR 5205, Lyon, France, (3)Planetary Science Institute Tucson, Tucson, AZ, United States, (4)Instituto de Astrofisica de Andalucia, Granada, Spain, (5)German Aerospace Center (DLR), Berlin, Germany
 
Color Variegation on 67P/Churyumov-Gerasimenko
Stubbe Faurschou Hviid1, Knollenberg Joerg1, Frank Preusker2, Stefano Mottola1, Ekkehard Kuhrt3, Stefan Schroeder2, Laurent Jorda4, Sonia Fornasier5, Jean-Baptiste Vincent6, Cedric Leyrat7, Nicolas Thomas8, Antoine Pommerol8, Maurizio Pajola9, Sebastien Besse10, Horst Uwe Keller11, Nilda Oklay12 and Pedro Hasselmann5, (1)German Aerospace Center DLR Berlin, Berlin, Germany, (2)German Aerospace Center (DLR), Berlin, Germany, (3)DLR, Berlin, Germany, (4)Observatoire Astrophysique Marseille, Marseille, France, (5)LESIA Observatoire de Paris, Meudon, France, (6)Max-Planck Institute for Solar System Research, Goettingen, Germany, (7)Paris Observatory Meudon, Meudon, France, (8)University of Bern, Bern, Switzerland, (9)CISAS - Center for Studies and Activities for Space, University of Padova, Padova, Italy, (10)European Space Agency, Villanueva De La Can, Spain, (11)Technical University of Braunschweig, Braunschweig, Germany, (12)Max Planck Institute for Solar System Research, Katlenburg-Lindau, Germany
 
The Shape of Comet 67P/Churyumov-Gerasimenko from Rosetta/Osiris Images
Laurent Jorda1, Robert W Gaskell2, Stubbe F Hviid3, Claire Capanna1, Olivier Groussin1, Pedro Gutiérrez4, Lamy Philippe1, Frank Scholten3, Frank Preusker3, Horst Uwe Keller5, Knollenberg Joerg3, Ekkehard Kuhrt3, Stefano Mottola3, Holger Sierks6, Colin Snodgrass6, Nicolas Thomas7, Jean-Baptiste Vincent6, Simone Marchi8 and Matteo Massironi9, (1)Laboratoire d'Astrophysique de Marseille, Marseille, France, (2)Planetary Science Institute Tucson, Tucson, AZ, United States, (3)German Aerospace Center (DLR), Berlin, Germany, (4)Instituto de Astrofisica de Andalucia, Granada, Spain, (5)Technical University of Braunschweig, Braunschweig, Germany, (6)Max-Planck Institute for Solar System Research, Goettingen, Germany, (7)University of Bern, Bern, Switzerland, (8)NASA Lunar Science Institute, Boulder, CO, United States, (9)Univ Padova, Padova, Italy
 
Simulations of impact features on comet 67P/Churyumov-Gerasimenko, as imaged by OSIRIS/ROSETTA
Gabriele Cremonese1, Alice Lucchetti1,2, Simone Marchi3, Elena Martellato1,4, Matteo Massironi5, Nilda Oklay6, Holger Sierks6 and Jean-Baptiste Vincent7, (1)INAF - Astronomical Observatory of Padova, Padova, Italy, (2)Universita' di Padova, CISAS, Padova, Italy, (3)NASA Lunar Science Institute, Boulder, CO, United States, (4)Universita' di Padova, dep. Physics and Astronomy, Padova, Italy, (5)Univ Padova, Padova, Italy, (6)Max Planck Institute for Solar System Research, Katlenburg-Lindau, Germany, (7)Max-Planck Institute for Solar System Research, Goettingen, Germany
 
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 Hartogh1, Samuel Gulkis2, Mark Allen3, Paul A A Von Allmen3, Gerard Beaudin4, Nicolas Biver5, Dominique Bockelée-Morvan6, Mathieu Choukroun7, Jacques Crovisier8, Pierre Encrenaz4, Therese Encrenaz8, Margaret A. Frerking7, Mark D Hofstadter7, Wing-Huen Ip9, Michael A Janssen3, Seungwon Lee3, Emmanuel Lellouch4, Cedric Leyrat10, F. Peter Schloerb11 and Thomas R Spilker12, (1)Max Planck Institute for Solar System Research, Katlenburg-Lindau, Germany, (2)California Institute of Technology, Pasadena, CA, United States, (3)NASA Jet Propulsion Laboratory, Pasadena, CA, United States, (4)Observatoire de Paris, LERMA, Paris, France, (5)Observatoire de Paris, Paris, France, (6)Paris Observatory, Paris, France, (7)Jet Propulsion Laboratory, Pasadena, CA, United States, (8)LESIA Observatoire de Paris, Meudon, France, (9)NCU National Central University of Taiwan, Jhongli, Taiwan, (10)Paris Observatory Meudon, Meudon, France, (11)University of Massachusetts Amherst, Amherst, MA, United States, (12)Retired, Monrovia, CA, United States
 
Inferring the Thermal and Electrical Properties of Comet 67P/Churyumov-Gerasimenko from the Continuum Measurements of the Microwave Instrument on the Rosetta Orbiter (MIRO)
Stephen Joseph Keihm1, Samuel Gulkis2, Mark D Hofstadter3, Paul Von Allmen4, F. Peter Schloerb5, Mathieu Choukroun3, Seungwon Lee4 and Michael A Janssen4, (1)JPL/NASA/Caltech, Pasadena, CA, United States, (2)California Institute of Technology, Pasadena, CA, United States, (3)Jet Propulsion Laboratory, Pasadena, CA, United States, (4)NASA Jet Propulsion Laboratory, Pasadena, CA, United States, (5)University of Massachusetts Amherst, Amherst, MA, United States
 
Dust thermal properties in the coma of comet 67P/CG as observed by from Rosetta/VIRTIS
Cedric Leyrat1, Dominique Bockelée-Morvan2, Stéphane Erard3, Fabrizio Capaccioni4, Gianrico Filacchione5, Gian Paolo Tozzi6 and Pierre Drossart3, (1)Paris Observatory Meudon, Meudon, France, (2)Paris Observatory, Paris, France, (3)LESIA Observatoire de Paris, Meudon, France, (4)Organization Not Listed, Washington, DC, United States, (5)IAPS-INAF, Rome, Italy, (6)INAF - Osservatorio Astrofisico di Arcetri, Firenze, Italy
 
Photometric Properties of Comet 67P/CG as Seen by VIRTIS-M Onboard Rosetta: Light Curves and Disk-integrated Phase Curves.
Mauro Ciarniello1, Fabrizio Capaccioni1, Gianrico Filacchione1, Stéphane Erard2, Andrea Raponi1, Maria Cristina De Sanctis1, Federico Tosi1, Maria Teresa Capria1, Giuseppe Piccioni1, Cedric Leyrat3, Dominique Bockelée-Morvan4, Ernesto Palomba1, Andrea Longobardo1, Stefan Schroeder5, Pierre Drossart2, Eric Quirico6, Pierre Beck6 and Bernard Schmitt7, (1)IAPS-INAF, Rome, Italy, (2)LESIA Observatoire de Paris, Meudon, France, (3)Paris Observatory Meudon, Meudon, France, (4)Paris Observatory, Paris, France, (5)German Aerospace Center DLR Berlin, Berlin, Germany, (6)University Joseph Fourier Grenoble, Grenboble, France, (7)Laboratoire de Planétologie de Grenoble (LPG), Grenoble, France
 
Rosetta/VIRTIS-M spectral data: Comet 67P/CG compared to other primitive small bodies.
Maria Cristina De Sanctis1, Fabrizio Capaccioni1, Gianrico Filacchione1, Stephan Erard2, Federico Tosi1, Mauro Ciarniello1, Andrea Raponi1, Giuseppe Piccioni1, Cedric Leyrat2, Dominique Bockelée-Morvan2, Pierre Drossart2 and Sonia Fornasier2, (1)IAPS-INAF, Rome, Italy, (2)LESIA Observatoire de Paris, Meudon, France
 
Distant Coma Composition of Comet 67P/Churyumov-Gerasimenko as Observed from Rosetta/VIRTIS
Dominique Bockelée-Morvan1, Stéphane Erard1, Cedric Leyrat1, Fabrizio Capaccioni2, Gianrico Filacchione2, Giuseppe Piccioni2, Pierre Drossart1, Vincent Debout1, Jacques Crovisier1 and Therese Encrenaz1, (1)LESIA Observatoire de Paris, Meudon, France, (2)IAPS-INAF, Rome, Italy
 
Thermal Properties of the Surface of 67P/Chryumov-Gerasimenko: Initial Results
Maria Teresa Capria1, Federico Tosi1, Ekkehard Kuhrt2, Andrea Raponi1, Michelangelo Formisano1, Maria Cristina De Sanctis1, Fabrizio Capaccioni3, Gianrico Filacchione1, Ernesto Palomba1, Andrea Longobardo1, Mauro Ciarniello1, Dominique Bockelée-Morvan4, Stephan Erard4, Cedric Leyrat5, Pierre Drossart6 and Gabriele Arnold2, (1)IAPS-INAF, Rome, Italy, (2)German Aerospace Center DLR Berlin, Berlin, Germany, (3)Organization Not Listed, Washington, DC, United States, (4)Paris Observatory, Paris, France, (5)LESIA Observatoire de Paris, Meudon, France, (6)Paris Observatory Meudon, Meudon, France
 
Looking for minor spectral features on 67P
Stéphane Erard1, Fabrizio Capaccioni2, Gianrico Filacchione3, Cedric Leyrat4, Federico Tosi3, Maria Cristina De Sanctis3, Dominique Bockelée-Morvan1 and Pierre Drossart5, (1)Paris Observatory, Paris, France, (2)Organization Not Listed, Washington, DC, United States, (3)IAPS-INAF, Rome, Italy, (4)Paris Observatory Meudon, Meudon, France, (5)LESIA Observatoire de Paris, Meudon, France
 
Comet 67P/C-G: Surface Temperatures as Derived by Rosetta/VIRTIS in the Mapping Phase
Federico Tosi1, Maria Teresa Capria1, Fabrizio Capaccioni1, Gianrico Filacchione1, Maria Cristina De Sanctis1, Stéphane Erard2, Cedric Leyrat2, Dominique Bockelée-Morvan2 and Ekkehard Kuhrt3, (1)IAPS-INAF, Rome, Italy, (2)LESIA Observatoire de Paris, Meudon, France, (3)German Aerospace Center DLR Berlin, Institute of Planetary Research, Berlin, Germany
 
Modeling the Spectrophotometric Properties of 67/P Churyumov-Gerasimenko as Seen by VIRTIS-M Onboard Rosetta
Andrea Raponi1, Fabrizio Capaccioni1, Gianrico Filacchione1, Mauro Ciarniello1, Maria Teresa Capria1, Stéphane Erard2, Ernesto Palomba1, Andrea Longobardo1, Maria Cristina De Sanctis1, Federico Tosi1, Giuseppe Piccioni1, Cedric Leyrat3, Dominique Bockelée-Morvan4, M. Antonietta Barucci5, Pierre Drossart2, Bernard Schmitt6 and Pierre Beck7, (1)IAPS-INAF, Rome, Italy, (2)LESIA Observatoire de Paris, Meudon, France, (3)Paris Observatory Meudon, Meudon, France, (4)Paris Observatory, Paris, France, (5)Observatoire Paris, Paris, France, (6)Laboratoire de Planétologie de Grenoble (LPG), Grenoble, France, (7)University Joseph Fourier Grenoble, Grenboble, France
 
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