P41C:
Rosetta 2014 IV Posters

Session ID#: 4554

Thursday, 18 December 2014: 8:00 AM-12:20 PM
Poster Hall (Moscone_South)
Chairs:  Matthew G Taylor, ESA/ESTEC, Noordwijk, Netherlands and Claudia J Alexander, JPL, Pasadena, CA, United States
Primary Convener:  Matthew G Taylor, ESA/ESTEC, Noordwijk, Netherlands
Co-Convener:  Claudia J Alexander, JPL, Pasadena, CA, United States
Co-Sponsor(s):
  • SH - SPA-Solar and Heliospheric Physics
Index Terms:

6008 Composition [PLANETARY SCIENCES: COMETS AND SMALL BODIES]
6015 Dust [PLANETARY SCIENCES: COMETS AND SMALL BODIES]
6040 Origin and evolution [PLANETARY SCIENCES: COMETS AND SMALL BODIES]
6099 General or miscellaneous [PLANETARY SCIENCES: COMETS AND SMALL BODIES]
Virtual Option?: No
Swirl Theme: Dust and Aerosols

Abstracts Submitted to this Session:

 
Rosetta Mission Status Update (4106)
Matthew G Taylor1, Nicolas Altobelli2, Claudia J Alexander3, Gerhard H Schwehm1, Fred Jansen1,4, Michael Küppers5, Laurence O'Rourke4, Maud Barthelemy4, Bernhard Geiger4, Bjorn Grieger5, Richard Moissl4, Claire Vallat2 and Rosetta Instrument Science and Operations teams, (1)ESTEC, Noordwijk, Netherlands, (2)ESAC, Villafranca del Castillo, Spain, (3)Jet Propulsion Laboratory, Pasadena, CA, United States, (4)European Space Agency, Villanueva de la Canada, Spain, (5)European Space Agency, Villanueva De La Can, Spain
 
Philae - Landing on a Comet (9212)
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 (22150)
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 (15474)
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 (15423)
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 (9321)
Mael Cardiet1, Alain Herique1, Yves Rogez2, Sylvain Douté3 and Wlodek W Kofman1, (1)University Joseph Fourier Grenoble, Grenboble, France, (2)University Grenoble Alpes, CNRS, IPAG, Grenoble, France, (3)Institut de Planétologie et d'Astrophysique de Grenoble (IPAG), Grenoble Cedex 09, France
 
First Results from the RPC Magnetometer Experiment during the Approach Phase to 67P/Churyumov-Gerasimenko (15244)
Ingo Richter1, Karl-Heinz Glassmeier2, Christoph Koenders1, Chris Carr3, Emanuele Cupido3, Claire Vallat4, Uwe M Motschmann5, Bruce Tsurutani6 and Martin Volwerk7, (1)Technical University of Braunschweig, Braunschweig, Germany, (2)Institute of Geophysics and extraterrestrial Physics, Technical University of Braunschweig, Braunschweig, Germany, (3)Imperial College London, London, United Kingdom, (4)ESAC, Villafranca del Castillo, Spain, (5)DLR Institute of Planetary Research, Berlin, Germany, (6)NASA Jet Propulsion Laboratory, Pasadena, CA, United States, (7)Austrian Academy of Sciences, Vienna, Austria
 
First Rosetta Observations of the Cometary Plasma at Churyumov–Gerasimenko with the Mutual Impedance Probe (RPC-MIP) (22921)
Pierre Henri1, Jean-Pierre Lebreton2, Christian Béghin1, Pierrette Décréau1, Anders I Eriksson3, Johann Geiswiller4, Rejean Grard5, Michel Hamelin6, Christian Xavier Mazelle7, Orélien Randriamboarison1, Walter Schmidt8, Jean-Gabriel Trotignon1, Gaétan Wattieaux9, Daniel Winterhalter10, Youcef Aouad1, Dominique Lagoutte1, Xavier Vallières1, Chris Carr11 and Emanuele Cupido11, (1)Laboratoire de Physique et Chimie de l'Environnement et de l'Espace (LPC2E) - CNRS - Université d'Orléans, Orléans, France, (2)Laboratoire de Physique et Chimie de l'Environnement et de l'Espace, CNRS / Université d’Orléans, Orléans, France, (3)IRF Swedish Institute of Space Physics Uppsala, Uppsala, Sweden, (4)DGA/DO/UM AMS/SM-ACEA, Bagneux, France, (5)European Space Research and Technology Centre, Noordwijk, Netherlands, (6)UPMC (Univ. Paris) / LATMOS, Paris, France, (7)University Paul Sabatier Toulouse III, Toulouse Cedex 09, France, (8)Finnish Meteorological Institute, Helsinki, Finland, (9)University Paul Sabatier Toulouse III, Laboratoire Plasma et Conversion d'Energie, Toulouse Cedex 09, France, (10)NASA Jet Propulsion Laboratory, Pasadena, CA, United States, (11)Imperial College London, London, United Kingdom
 
Recommended values and correlations of thermophysical properties for comet modelling (15440)
Ivanka Pelivan, German Aerospace Center DLR Berlin, Berlin, Germany, Jens Biele, German Aerospace Center DLR Cologne, Cologne, Germany, Ekkehard Kuhrt, DLR, Berlin, Germany, Bjorn Johan Ragnar Davidsson, Jet Propulsion Laboratory, California Institute of Technology, Pasadena, CA, United States, Mathieu Choukroun, Jet Propulsion Laboratory, Pasadena, United States and Claudia J Alexander, Jet Propulsion Laboratory, Pasadena, CA, United States
 
CONSERT Link Budget Simulator for the Direct Path (15484)
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 (22935)
Hans Nilsson1, Gabriella Stenberg Wieser1, Etienne Behar1, Rickard N A Lundin2, Stas Barbash1, 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 Koenders14, Pat Mokashi15, Zoltan Nemeth16, Ingo Richter14, Karoly Szego17 and Claire Vallat18, (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, 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)Institute of Geophysics and extraterrestrial Physics, 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)Technical University of Braunschweig, Braunschweig, Germany, (15)Southwest Research Institute San Antonio, San Antonio, TX, United States, (16)Wigner Research Center for Physics, Budapest, Hungary, (17)Hungarian Academy of Sciences, Budapest, Hungary, (18)ESAC, Villafranca del Castillo, Spain
 
The Rosetta Ion and Electron Sensor (IES) Measurement of the Development of Pickup Ions from Comet 67P/Churyumov-Gerasimenko (29712)
Raymond Goldstein1, James L Burch2, Pat Mokashi1, Craig J Pollock3, Thomas W Broiles1, Kathleen Mandt4, Thomas Cravens5, Marilia Samara6, Anders I Eriksson7, Chris Carr8, Jean-Pierre Lebreton9, Pierre Henri10, Karl-Heinz Glassmeier11, Hans Nilsson12 and Christoph Koenders13, (1)Southwest Research Institute, San Antonio, TX, United States, (2)Southwest Research Institute, San Antonio, United States, (3)NASA Goddard Space Flight Center, Greenbelt, United States, (4)Johns Hopkins University Applied Physics Laboratory, Space Exploration Sector, Laurel, United States, (5)University of Kansas, Physics and Astronomy, Lawrence, KS, United States, (6)NASA Goddard Space Flight Center, Greenbelt, MD, United States, (7)IRF Swedish Institute of Space Physics Uppsala, Uppsala, Sweden, (8)Imperial College, London, United Kingdom, London, United Kingdom, (9)University of Orleans, Orleans, France, (10)Laboratoire de Physique et Chimie de l'Environnement et de l'Espace, Orléans Cedex 2, France, (11)Institute of Geophysics and extraterrestrial Physics, Technical University of Braunschweig, Braunschweig, Germany, (12)IRF Swedish Institute of Space Physics Kiruna, Kiruna, Sweden, (13)Technical University of Braunschweig, Braunschweig, Germany
 
Early Observations with the Rosetta Langmuir Probe Instrument at the Target Comet (29056)
Anders I Eriksson1, Niklas J. T. Edberg1, Reine Gill1, Fredrik Leffe Johansson1, Elias Odelstad1, Jan-Erik Wahlund1, Erik Vigren1, Tomas Karlsson2, Per-Arne Lindqvist3, Riku Jarvinen4, Bjorn Lybekk5, Wojciech J. Miloch5, Arne Pedersen5, Jean-Pierre Lebreton6, Chris Carr7 and Emanuele Cupido7, (1)IRF Swedish Institute of Space Physics Uppsala, Uppsala, Sweden, (2)KTH Royal Institute of Technology, Division of Space and Plasma Physics, Stockholm, Sweden, (3)KTH Royal Institute of Technology, Stockholm, Sweden, (4)Finnish Meteorological Inst, Helsinki, Finland, (5)University of Oslo, Department of Physics, Oslo, Norway, (6)University of Orleans, Orleans, France, (7)Imperial College London, London, United Kingdom
 
Ion and Electron Sensor Observations on Photoelectrons and Coma Development at Comet 67P/Churyumov-Gerasimenko (29257)
James L Burch1, Raymond Goldstein2, Pat Mokashi2, Craig J Pollock3, Thomas W Broiles2, Kathleen Mandt4, Thomas Cravens5, Marilia Samara6, Anders I Eriksson7, Chris Carr8, Jean-Pierre Lebreton9, Pierre Henri9, Karl-Heinz Glassmeier10, Hans Nilsson11 and Christoph Koenders12, (1)Southwest Research Institute, San Antonio, United States, (2)Southwest Research Institute, San Antonio, TX, United States, (3)NASA Goddard Space Flight Center, Greenbelt, United States, (4)Applied Physics Laboratory Johns Hopkins, Laurel, MD, United States, (5)University of Kansas, Physics and Astronomy, Lawrence, KS, United States, (6)NASA Goddard Space Flight Center, Greenbelt, MD, United States, (7)IRF Swedish Institute of Space Physics Uppsala, Uppsala, Sweden, (8)Imperial College London, London, United Kingdom, (9)Laboratoire de Physique et Chimie de l'Environnement et de l'Espace, Orléans Cedex 2, France, (10)Institute of Geophysics and extraterrestrial Physics, Technical University of Braunschweig, Braunschweig, Germany, (11)IRF Swedish Institute of Space Physics Kiruna, Kiruna, Sweden, (12)Technical University of Braunschweig, Braunschweig, Germany
 
Can Rosetta IES Measure Charged Dust Grains at Comet 67P/C-G? (10446)
George B Clark1,2, Craig J Pollock3, Raymond Goldstein4, Marilia Samara2, Thomas W Broiles4, Kathleen Mandt5, James L Burch6 and Zoltan Sternovsky7, (1)Johns Hopkins University Applied Physics Laboratory, Laurel, MD, United States, (2)NASA Goddard Space Flight Center, Greenbelt, MD, United States, (3)NASA Goddard Space Flight Center, Greenbelt, United States, (4)Southwest Research Institute, San Antonio, TX, United States, (5)Johns Hopkins University Applied Physics Laboratory, Space Exploration Sector, Laurel, United States, (6)Southwest Research Institute, San Antonio, United States, (7)University of Colorado, Smead Aerospace Engineering Sciences Department, Boulder, CO, United States
 
Structure and Dynamics of the Interaction Region at Comet 67P/Churyumov-Gerasimenko: Comparing Numerical Simulations and RPC Magnetic Field Observations (14996)
Christoph Koenders1, Karl-Heinz Glassmeier2, Ingo Richter1, Charlotte Goetz1, Chris Carr3, Emanuele Cupido3, Claire Vallat4 and Uwe M Motschmann5, (1)Technical University of Braunschweig, Braunschweig, Germany, (2)Institute of Geophysics and extraterrestrial Physics, Technical University of Braunschweig, Braunschweig, Germany, (3)Imperial College London, London, United Kingdom, (4)ESAC, Villafranca del Castillo, Spain, (5)DLR Institute of Planetary Research, Berlin, Germany
 
Does 67P/C-G Have a Dusty Plasma Environment? (4644)
Tamas I Gombosi, University of Michigan, Climate and Space Sciences and Engineering, Ann Arbor, United States
 
A Multi-neutral-fluid model of comet 67P/Churyumov-Gerasimenko (25662)
Yinsi Shou1, Michael R Combi2, Tamas I Gombosi3, Xianzhe Jia4, Gabor Toth3, Kenneth C Hansen1, Valeriy Tenishev3 and Nicolas Fougere5, (1)University of Michigan, Ann Arbor, MI, United States, (2)Univ Michigan, Ann Arbor, MI, United States, (3)University of Michigan, Climate and Space Sciences and Engineering, Ann Arbor, United States, (4)University of Michigan, Department of Climate and Space Sciences and Engineering, Ann Arbor, United States, (5)University of Michigan Ann Arbor, Ann Arbor, MI, United States
 
Giada improved calibration of measurement subsystems (29385)
Vincenzo Della Corte1, Alessandra Rotundi2, Roberto Sordini3, Mario Accolla2, Marco Ferrari4, Stavro Lambrov Ivanovski1, Francesca Lucarelli2, Elena Mazzotta Epifani5 and Pasquale Palumbo6, (1)IAPS-INAF, Rome, Italy, (2)Parthenope University of Naples, Scienze e Tecnologie, Naples, Italy, (3)INAF-IAPS, Rome, Italy, (4)Istituto Nazionale di Astrofisica (INAF), Istituto di Astrofisica e Planetologia Spaziali (IAPS), Rome, Italy, (5)INAF, OAC, Naples, Italy, (6)Università Parthenope, Napoli, Italy
 
A Computer-assisted Method for the Calibration of Raw Data from the DFMS sensor on Rosetta (25016)
Frederik Dhooghe1, Johan De Keyser1, Romain Maggiolo1, Kathrin Altwegg2, Ursina Calmonte2, Stephen A Fuselier3, Myrtha Hässig4, Jean-Jacques Berthelier5, Urs A. Mall6, Tamas I Gombosi7 and Björn Fiethe8, (1)Belgian Institute for Space Aeronomy, Brussels, Belgium, (2)University of Bern, Bern, Switzerland, (3)Southwest Research Institute, San Antonio, TX, United States, (4)Southwest Research Institute San Antonio, San Antonio, TX, United States, (5)LATMOS Laboratoire Atmosphères, Milieux, Observations Spatiales, Paris Cedex 05, France, (6)Max Planck Institute for Solar System Research, Katlenburg-Lindau, Germany, (7)University of Michigan, Climate and Space Sciences and Engineering, Ann Arbor, United States, (8)Technical University of Braunschweig, Braunschweig, Germany
 
First insights on the organic species from the high resolution mass spectrometer ROSINA DFMS on-board the Rosetta spacecraft (13291)
Lena Le Roy1, Kathrin Altwegg1, Jean-Jacques Berthelier2, Ursina Calmonte1, Frederik Dhooghe3, Bjoern Fiethe4, Stephen A Fuselier5, Tamas I Gombosi6, Martin Rubin7 and Chia-yu Tzou8, (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, TX, United States, (6)University of Michigan, Climate and Space Sciences and Engineering, Ann Arbor, United States, (7)University of Bern, Physics Institute, Space Research and Planetary Sciences, Bern, Switzerland, (8)University of Bern, Physikalisches Institut, Bern, Switzerland
 
Multifluid MHD Simulations of the Plasma Environment of Comet Churyumov-Gerasimenko at Different Heliocentric Distances (20132)
Zhenguang Huang1, Xianzhe Jia2, Martin Rubin3, Nicolas Fougere2, Tamas I Gombosi2, Valeriy Tenishev2, Michael R Combi2, Andre Michel Bieler2, Gabor Toth2, Kenneth C Hansen2 and Yinsi Shou2, (1)University of Michigan, Climate and Space Sciences and Engineering, Ann Arbor, United States, (2)University of Michigan, Ann Arbor, MI, United States, (3)University of Bern, Physics Institute, Space Research and Planetary Sciences, Bern, Switzerland
 
In Situ Space Gas Dynamic Measurements by the ROSINA Comet Pressure Sensor COPS on the Rosetta Spacecraft (16342)
Chia-yu Tzou1, Kathrin Altwegg2, Björn Fiethe3, Sébastien Gasc1 and Martin Rubin4, (1)University of Bern, Physikalisches Institut, Bern, Switzerland, (2)University of Bern, Bern, Switzerland, (3)Technical University of Braunschweig, Braunschweig, Germany, (4)University of Bern, Physics Institute, Space Research and Planetary Sciences, Bern, Switzerland
 
A 3D Description of the Coma of Comet 67P/Churyumov-Gerasimenko Constrained by Rosetta Observations (13270)
Nicolas Fougere1, Valeriy Tenishev2, Andre Michel Bieler1, Michael R Combi1, Tamas I Gombosi1, Kenneth C Hansen1, Xianzhe Jia3, Yinsi Shou1, Zhenguang Huang2, Gabor Toth1, Kathrin Altwegg4, Peter Wurz5, Hans Balsiger4, Annette Jäckel6, Lena Le Roy4, Sébastien Gasc6, Ursina Calmonte4, Martin Rubin7, Chia-yu Tzou6, Myrtha Hässig8, Stephen A Fuselier9, Johan De Keyser10, Jean-Jacques Berthelier11, Urs A. Mall12, Henri Rème13 and Björn Fiethe14, (1)University of Michigan, Ann Arbor, MI, United States, (2)University of Michigan, Climate and Space Sciences and Engineering, Ann Arbor, United States, (3)University of Michigan, Department of Climate and Space Sciences and Engineering, Ann Arbor, United States, (4)University of Bern, Bern, Switzerland, (5)University of Bern, Space Research and Planetary Sciences, Bern, Switzerland, (6)University of Bern, Physikalisches Institut, Bern, Switzerland, (7)University of Bern, Physics Institute, Space Research and Planetary Sciences, Bern, Switzerland, (8)Southwest Research Institute San Antonio, San Antonio, TX, United States, (9)Southwest Research Institute, San Antonio, TX, United States, (10)Belgian Institute for Space Aeronomy, Brussels, Belgium, (11)CNRS-LATMOS, Paris, France, (12)Max Planck Institute for Solar System Research, Katlenburg-Lindau, Germany, (13)IRAP, Institut de Recherche en Astrophysique et Planétologie, Toulouse, France, (14)Technical University of Braunschweig, Braunschweig, Germany
 
3D Direct Simulation Monte Carlo Modeling of the Spacecraft Environment of Rosetta (15835)
Andre Michel Bieler1, Valeriy Tenishev2, Nicolas Fougere1, Tamas I Gombosi1, Kenneth C Hansen1, Michael R Combi1, Zhenguang Huang2, Xianzhe Jia3, Gabor Toth1, Kathrin Altwegg4, Peter Wurz5, Annette Jäckel6, Lena Le Roy4, Sébastien Gasc6, Ursina Calmonte4, Martin Rubin7, Chia-yu Tzou6, Myrtha Hässig8, Stephen A Fuselier9, Johan De Keyser10, Jean-Jacques Berthelier11, Urs A. Mall12, Henri Rème13, Björn Fiethe14 and Hans Balsiger4, (1)University of Michigan, Ann Arbor, MI, United States, (2)University of Michigan, Climate and Space Sciences and Engineering, Ann Arbor, United States, (3)University of Michigan, Department of Climate and Space Sciences and Engineering, Ann Arbor, United States, (4)University of Bern, Bern, Switzerland, (5)University of Bern, Space Research and Planetary Sciences, Bern, Switzerland, (6)University of Bern, Physikalisches Institut, Bern, Switzerland, (7)University of Bern, Physics Institute, Space Research and Planetary Sciences, Bern, Switzerland, (8)Southwest Research Institute San Antonio, San Antonio, TX, United States, (9)Southwest Research Institute, San Antonio, TX, United States, (10)Belgian Institute for Space Aeronomy, Brussels, Belgium, (11)LATMOS Laboratoire Atmosphères, Milieux, Observations Spatiales, Paris Cedex 05, France, (12)Max Planck Institute for Solar System Research, Katlenburg-Lindau, Germany, (13)IRAP, Institut de Recherche en Astrophysique et Planétologie, Toulouse, France, (14)Technical University of Braunschweig, Braunschweig, Germany
 
Measuring Oxygen Isotopes with COSIMA (13298)
John Anthony Paquette1, Cécile Engrand2, Oliver Stenzel1 and Martin Hilchenbach1, (1)Max Planck Institute for Solar System Research, Göttingen, 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. (24604)
Yves Langevin1, Klaus Hornung2, Martin Hilchenbach3, Jochen Kissel3, Johan V Silen4, Christelle Briois5, Rita Schulz6, Donia Baklouti7, Pascal Eng7 and COSIMA Team, (1)Institut d'Astrophysique Spatiale, CNRS/Université Paris Saclay, Orsay Cedex, France, (2)Universität der Bundeswehr, 85577 Neubiberg, Germany, (3)Max Planck Institute for Solar System Research, Göttingen, 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 Agency, Noordwijk, Netherlands, (7)IAS Institut d'Astrophysique Spatiale, Orsay Cedex, France
 
On the Inorganic Composition of Cometary Dust from Comet 67P/Churyumov-Gerasimenko, as Seen by COSIMA on Board ROSETTA. (22575)
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 Langevin8, Harry Lehto9, Sihane Merouane5, François-Régis Orthous-Daunay10, Jouni Rynö11, Rita Schulz12, Johan V Silen11, Sandra Siljeström13, Thomas Stephan14, Laurent Thirkell3, Kurt Varmuza15 and COSIMA Team, (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, Orléans, France, (4)LISA Laboratoire Interuniversitaire des Systèmes Atmosphériques, Créteil, France, (5)Max Planck Institute for Solar System Research, Göttingen, Germany, (6)von Hoerner und Sulger GmbH, 68723 Schwetzingen, Germany, (7)Universität der Bundeswehr, 85577 Neubiberg, Germany, (8)Institut d'Astrophysique Spatiale, CNRS/Université Paris Saclay, Orsay Cedex, France, (9)University of Turku, Department of Physics and Astronomy, Tuorla Observatory, Piikkiö, Finland, (10)IPAG - Institut de Planetologie et d'Astrophysique de Grenoble, Grenoble, France, (11)Finnish Meteorological Institute, Helsinki, Finland, (12)European Space Agency, Noordwijk, Netherlands, (13)RISE Research Institutes of Sweden, Stockholm, Sweden, (14)The University of Chicago, Chicago, United States, (15)Technische Universität Wien, Wien, Austria
 
Morphological Forms of Cometary Activity (24656)
Horst Uwe Keller1, Michael F A'Hearn2, Olivier Groussin3, Stubbe Faurschou Hviid4, Ekkehard Kuhrt5, Nicolas Thomas6, Sebastien Besse7, Stefan Schroeder5, Jean-Baptiste Vincent8 and the OSIRIS Team, (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 (10018)
Anne-Thérèse Auger1,2, Olivier Groussin1, Laurent Jorda1, Sylvain Bouley3, Philippe L Lamy1, Gabriele Cremonese4, Nicolas Thomas5, Holger Sierks6 and the OSIRIS Team, (1)Laboratoire d'Astrophysique de Marseille, Marseille, France, (2)Laboratoire GEOPS, Orsay, France, (3)Université Paris Sud, GEOPS, Orsay, France, (4)INAF-OAPd, Padova, Italy, (5)University of Bern, Bern, Switzerland, (6)Max-Planck Institute for Solar System Research, Goettingen, Germany
 
The Nucleus of Comet 67P/Churyumov-Gerasimenko : a New Case of Contact Binary ? (13889)
Philippe L Lamy1, Michael F A'Hearn2, Olivier Groussin1, Laurent Jorda1, Horst Uwe Keller3, Hans Rickman4 and OSIRIS team, (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 (15654)
Sebastien Besse1, Sonia Fornasier2, Holger Sierks3, M. Antonietta Barucci4, Cedric Leyrat5, Stubbe Faurschou Hviid6, Laurent Jorda7, Horst Uwe Keller8, Michael Küppers9, Sara Magrin10, Matteo Massironi11, Nilda Oklay12, M. Pajola13, Nicolas Thomas14, C. Tubiana12, Colin Snodgrass3, Jean-Baptiste Vincent15 and OSIRIS Team, (1)Aurora Technology B.V., European Space Astronomy Centre/ESA, Madrid, Spain., Villanueva De La Canada, Spain, (2)LESIA Observatoire de Paris, Meudon, France, (3)Max-Planck Institute for Solar System Research, Goettingen, Germany, (4)LESIA Observatoire de Paris, Université PSL, CNRS, Sorbonne Université, Université Paris-Diderot, Meudon, France, (5)Paris Observatory Meudon, Meudon, France, (6)German Aerospace Center DLR Berlin, Berlin, Germany, (7)Observatoire Astrophysique Marseille, Marseille, France, (8)Technical University of Braunschweig, Braunschweig, Germany, (9)European Space Agency, Villanueva De La Can, Spain, (10)CISAS - Center for Studies and Activities for Space, University of Padova, Padova, Italy, (11)Univ Padova, Padova, Italy, (12)Max Planck Institute for Solar System Research, Katlenburg-Lindau, Germany, (13)CISAS-University of Padova, Padova, Italy, (14)University of Bern, Bern, Switzerland, (15)Max-Planck Institute for Solar System Research, Germany, Goettigen, Germany
 
The Geomorphology of Comet Churymov-Gerasimenko As Revealed By Rosetta/Osiris: Implicationsfor Past Collisional Evolution (8089)
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 Marzari12, Matteo Massironi13, Maurizio Pajola14, Hans Rickman15, Rafael Rodrigo16, Holger Sierks17, Colin Snodgrass17, Nicolas Thomas18, Jean-Baptiste Vincent19 and OSIRIS Team, (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)Aurora Technology B.V., European Space Astronomy Centre/ESA, Madrid, Spain., Villanueva De La Canada, Spain, (6)INAF-OAPd, Padova, Italy, (7)National Central University, Institute of Astronomy, Taoyuan City, 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)University of Padova, Padova, Italy, (13)Univ Padova, Padova, Italy, (14)CISAS - Center for Studies and Activities for Space, University of Padova, Padova, Italy, (15)Uppsala University, Department of Physics and Astronomy, Uppsala, Sweden, (16)IAA-CSIC, Granada, Spain, (17)Max-Planck Institute for Solar System Research, Goettingen, Germany, (18)University of Bern, Bern, Switzerland, (19)DLR Institute of Planetary Research, Berlin, Germany
 
Multi-Resolution Stereophotoclinometry by Deformation, a New 3D Shape Reconstruction Method Applied to ROSETTA/OSIRIS Images (21936)
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, Didier Vibert1 and The OSIRIS Team, (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 (22395)
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 Pommerol9, Maurizio Pajola10, Sebastien Besse11, Horst Uwe Keller12, Nilda Oklay13, Pedro Hasselmann5 and The OSIRIS Team, (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)DLR Institute of Planetary Research, Berlin, Germany, (7)Paris Observatory Meudon, Meudon, France, (8)University of Bern, Bern, Switzerland, (9)University of Bern, Space Research & Planetary Sciences, Bern, Switzerland, (10)CISAS - Center for Studies and Activities for Space, University of Padova, Padova, Italy, (11)Aurora Technology B.V., European Space Astronomy Centre/ESA, Madrid, Spain., Villanueva De La Canada, Spain, (12)Technical University of Braunschweig, Braunschweig, Germany, (13)Max Planck Institute for Solar System Research, Katlenburg-Lindau, Germany
 
The Shape of Comet 67P/Churyumov-Gerasimenko from Rosetta/Osiris Images (11420)
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 Vincent8, Simone Marchi9, Matteo Massironi10 and OSIRIS Team, (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)DLR Institute of Planetary Research, Berlin, Germany, (9)Southwest Research Institute, Boulder, United States, (10)Univ Padova, Padova, Italy
 
Simulations of impact features on comet 67P/Churyumov-Gerasimenko, as imaged by OSIRIS/ROSETTA (20701)
Gabriele Cremonese1, Alice Lucchetti2,3, Simone Marchi4, Elena Martellato2,5, Matteo Massironi6, Nilda Oklay7, Holger Sierks8, Jean-Baptiste Vincent9 and OSIRIS team, (1)INAF-OAPd, Padova, Italy, (2)INAF - Astronomical Observatory of Padova, Padova, Italy, (3)Universita' di Padova, CISAS, Padova, Italy, (4)Southwest Research Institute, Boulder, United States, (5)Universita' di Padova, dep. Physics and Astronomy, Padova, Italy, (6)Univ Padova, Padova, Italy, (7)Max Planck Institute for Solar System Research, Katlenburg-Lindau, Germany, (8)Max-Planck Institute for Solar System Research, Goettingen, Germany, (9)DLR Institute of Planetary Research, Berlin, Germany
 
On the Spatial Homogeneity of the H2O Coma of 67P/C.-G. at 3.9-3.5 AU as Seen from MIRO (28884)
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
 
Inferring the Thermal and Electrical Properties of Comet 67P/Churyumov-Gerasimenko from the Continuum Measurements of the Microwave Instrument on the Rosetta Orbiter (MIRO) (30584)
Stephen Joseph Keihm1, Samuel Gulkis2, Mark D Hofstadter3, Paul Von Allmen4, F. Peter Schloerb5, Mathieu Choukroun6, Seungwon Lee7 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/California Institute of Technology, Pasadena, CA, United States, (4)NASA Jet Propulsion Laboratory, Pasadena, CA, United States, (5)University of Massachusetts Amherst, Amherst, MA, United States, (6)Jet Propulsion Laboratory, Pasadena, United States, (7)NASA Jet Propulsion Laboratory, Pasadena, United States
 
Dust thermal properties in the coma of comet 67P/CG as observed by from Rosetta/VIRTIS (21657)
Cedric Leyrat, Paris Observatory Meudon, Meudon, France, Dominique Bockelée-Morvan, Paris Observatory, Paris, France, Stéphane Erard, LESIA, Observatoire de Paris, Université PSL, CNRS, Sorbonne Université, Univ. Paris Diderot, Sorbonne Paris Cité, 5 place Jules Janssen, 92195 Meudon, France, LESIA - Observatoire de Paris, Meudon, France, Fabrizio Capaccioni, Organization Not Listed, Washington, DC, United States, Gianrico Filacchione, IAPS-INAF, Rome, Italy, Gian Paolo Tozzi, INAF - Osservatorio Astrofisico di Arcetri, Firenze, Italy, Pierre Drossart, LESIA Observatoire de Paris, Meudon, France and Rosetta VIRTIS Team
 
Photometric Properties of Comet 67P/CG as Seen by VIRTIS-M Onboard Rosetta: Light Curves and Disk-integrated Phase Curves. (22117)
Mauro Ciarniello1, Fabrizio Capaccioni2, Gianrico Filacchione2, Stéphane Erard3, Andrea Raponi4, Maria Cristina De Sanctis2, Federico Tosi5, Maria Teresa Capria2, Giuseppe Piccioni2, Cedric Leyrat6, Dominique Bockelée-Morvan7, Ernesto Palomba2, Andrea Longobardo2, Stefan Schroeder8, Pierre Drossart9, Eric Quirico10, Pierre Beck10, Bernard Schmitt11 and Rosetta-VIRTIS team, (1)Istituto di Astrofisica e Planetologia Spatiazli IAPS-INAF, Roma, Italy, (2)IAPS-INAF, Rome, Italy, (3)LESIA, Observatoire de Paris, Université PSL, CNRS, Sorbonne Université, Univ. Paris Diderot, Sorbonne Paris Cité, 5 place Jules Janssen, 92195 Meudon, France, LESIA - Observatoire de Paris, Meudon, France, (4)Istituto Nazionale di Astrofisica (INAF), Istituto di Astrofisica e Planetologia Spaziali (IAPS), Rome, Italy, (5)INAF-IAPS, Rome, Italy, (6)Paris Observatory Meudon, Meudon, France, (7)Paris Observatory, Paris, France, (8)German Aerospace Center DLR Berlin, Berlin, Germany, (9)LESIA Observatoire de Paris, Meudon, France, (10)University Joseph Fourier Grenoble, Grenboble, France, (11)Laboratoire de Planétologie de Grenoble (LPG), Grenoble, France
 
Rosetta/VIRTIS-M spectral data: Comet 67P/CG compared to other primitive small bodies. (21507)
Maria Cristina De Sanctis1, Fabrizio Capaccioni1, Gianrico Filacchione1, Stephan Erard2, Federico Tosi3, Mauro Ciarniello4, Andrea Raponi5, Giuseppe Piccioni1, Cedric Leyrat2, Dominique Bockelée-Morvan2, Pierre Drossart2, Sonia Fornasier2 and Rosetta-VIRTIS, (1)IAPS-INAF, Rome, Italy, (2)LESIA Observatoire de Paris, Meudon, France, (3)INAF-IAPS, Rome, Italy, (4)Istituto di Astrofisica e Planetologia Spatiazli IAPS-INAF, Roma, Italy, (5)Istituto Nazionale di Astrofisica (INAF), Istituto di Astrofisica e Planetologia Spaziali (IAPS), Rome, Italy
 
Distant Coma Composition of Comet 67P/Churyumov-Gerasimenko as Observed from Rosetta/VIRTIS (22131)
Dominique Bockelée-Morvan1, Stéphane Erard2, Cedric Leyrat1, Fabrizio Capaccioni3, Gianrico Filacchione3, Giuseppe Piccioni3, Pierre Drossart1, Vincent Debout1, Jacques Crovisier1, Therese Encrenaz4 and The Rosetta/VIRTIS Team, (1)LESIA Observatoire de Paris, Meudon, France, (2)LESIA, Observatoire de Paris, Université PSL, CNRS, Sorbonne Université, Univ. Paris Diderot, Sorbonne Paris Cité, 5 place Jules Janssen, 92195 Meudon, France, LESIA - Observatoire de Paris, Meudon, France, (3)IAPS-INAF, Rome, Italy, (4)Paris Observatory-PSL, LIRA, Meudon, France
 
Thermal Properties of the Surface of 67P/Chryumov-Gerasimenko: Initial Results (21134)
Maria Teresa Capria1, Federico Tosi2, Ekkehard Kuhrt3, Andrea Raponi4, Michelangelo Formisano1, Maria Cristina De Sanctis1, Fabrizio Capaccioni5, Gianrico Filacchione1, Ernesto Palomba1, Andrea Longobardo1, Mauro Ciarniello6, Dominique Bockelée-Morvan7, Stephan Erard7, Cedric Leyrat8, Pierre Drossart9, Gabriele Arnold3 and VIRTIS-Rosetta Team, (1)IAPS-INAF, Rome, Italy, (2)INAF-IAPS, Rome, Italy, (3)German Aerospace Center DLR Berlin, Berlin, Germany, (4)Istituto Nazionale di Astrofisica (INAF), Istituto di Astrofisica e Planetologia Spaziali (IAPS), Rome, Italy, (5)Organization Not Listed, Washington, DC, United States, (6)Istituto di Astrofisica e Planetologia Spatiazli IAPS-INAF, Roma, Italy, (7)Paris Observatory, Paris, France, (8)LESIA Observatoire de Paris, Meudon, France, (9)Paris Observatory Meudon, Meudon, France
 
Looking for minor spectral features on 67P (26608)
Stéphane Erard1, Fabrizio Capaccioni2, Gianrico Filacchione3, Cedric Leyrat4, Federico Tosi5, Maria Cristina De Sanctis3, Dominique Bockelée-Morvan1, Pierre Drossart6 and the Rosetta/VIRTIS Team, (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)INAF-IAPS, Rome, Italy, (6)LESIA Observatoire de Paris, Meudon, France
 
Comet 67P/C-G: Surface Temperatures as Derived by Rosetta/VIRTIS in the Mapping Phase (20954)
Federico Tosi1, Maria Teresa Capria2, Fabrizio Capaccioni2, Gianrico Filacchione2, Maria Cristina De Sanctis2, Stéphane Erard3, Cedric Leyrat4, Dominique Bockelée-Morvan4, Ekkehard Kuhrt5 and Rosetta/VIRTIS Team, (1)INAF-IAPS, Rome, Italy, (2)IAPS-INAF, Rome, Italy, (3)LESIA, Observatoire de Paris, Université PSL, CNRS, Sorbonne Université, Univ. Paris Diderot, Sorbonne Paris Cité, 5 place Jules Janssen, 92195 Meudon, France, LESIA - Observatoire de Paris, Meudon, France, (4)LESIA Observatoire de Paris, Meudon, France, (5)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 (22366)
Andrea Raponi1, Fabrizio Capaccioni2, Gianrico Filacchione2, Mauro Ciarniello3, Maria Teresa Capria2, Stéphane Erard4, Ernesto Palomba2, Andrea Longobardo2, Maria Cristina De Sanctis2, Federico Tosi5, Giuseppe Piccioni2, Cedric Leyrat6, Dominique Bockelée-Morvan7, M. Antonietta Barucci8, Pierre Drossart9, Bernard Schmitt10, Pierre Beck11 and Rosetta-VIRTIS team, (1)Istituto Nazionale di Astrofisica (INAF), Istituto di Astrofisica e Planetologia Spaziali (IAPS), Rome, Italy, (2)IAPS-INAF, Rome, Italy, (3)Istituto di Astrofisica e Planetologia Spatiazli IAPS-INAF, Roma, Italy, (4)LESIA, Observatoire de Paris, Université PSL, CNRS, Sorbonne Université, Univ. Paris Diderot, Sorbonne Paris Cité, 5 place Jules Janssen, 92195 Meudon, France, LESIA - Observatoire de Paris, Meudon, France, (5)INAF-IAPS, Rome, Italy, (6)Paris Observatory Meudon, Meudon, France, (7)Paris Observatory, Paris, France, (8)Observatoire Paris, Paris, France, (9)LESIA Observatoire de Paris, Meudon, France, (10)Laboratoire de Planétologie de Grenoble (LPG), Grenoble, France, (11)University Joseph Fourier Grenoble, Grenboble, France
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