Overview of the coordinated ground-based observations of Titan during the Huygens mission

Autor: Theodor Kostiuk, Glen Langston, William M. Folkner, Olivier Witasse, Emily L. Schaller, Christophe O. Laux, Jean-Pierre Lebreton, R. Dutta-Roy, Sergei Pogrebenko, Hayley Bignall, Frank D. Ghigo, Arpad Szomoru, Robert M. Campbell, Thierry Magin, Huib Jan van Langevelde, Máté Ádámkovics, Ralph D. Lorenz, Cormac Reynolds, John Reynolds, Bonnie J. Buratti, Robert J. Sault, Ari Mujunen, Imke de Pater, M. A. Garrett, Stephen M. Parsley, Jonathan D. Romney, Eric Gendron, Thierry Blancquaert, Timothy A. Livengood, Anastasios Tzioumis, Chad Trujillo, Michael E. Brown, Robert A. Preston, Antonin Bouchez, Chris Phillips, Walter Brisken, Michael K. Bird, Sami W. Asmar, Bruno Sicardy, Mathieu Hirtzig, Jouko Ritakari, Steven Tingay, Anne Bourdon, C.G.M. van 't Klooster, Alberto Negrao, David Luz, Lise Caillault, I. M. Avruch, Richard Dodson, Henry G. Roe, Markus Hartung, Athena Coustenis, Leonid I. Gurvits
Přispěvatelé: European Space Research and Technology Centre (ESTEC), European Space Agency (ESA), RadioAstronomisches Institut [Bonn] (RAIUB), Rheinische Friedrich-Wilhelms-Universität Bonn, Jet Propulsion Laboratory (JPL), NASA-California Institute of Technology (CALTECH), Joint Institute for VLBI in Europe (JIVE ERIC), Australia Telescope National Facility (ATNF), Commonwealth Scientific and Industrial Research Organisation [Canberra] (CSIRO), National Radio Astronomy Observatory [Green Bank] (NRAO), National Radio Astronomy Observatory (NRAO), National Radio Astronomy Observatory [Socorro] (NRAO), Metsähovi Radio Observatory, Aalto University, Swinburne University of Technology (Hawthorn campus), Observatorio Astronomico Nacional, Madrid, Laboratoire d'études spatiales et d'instrumentation en astrophysique (LESIA), Université Pierre et Marie Curie - Paris 6 (UPMC)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS), Laboratoire de Planétologie et Géodynamique [UMR 6112] (LPG), Université d'Angers (UA)-Université de Nantes - UFR des Sciences et des Techniques (UN UFR ST), Université de Nantes (UN)-Université de Nantes (UN)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS), Observatório Astronómico de Lisboa, Johns Hopkins University Applied Physics Laboratory [Laurel, MD] (APL), Laboratoire d'Énergétique Moléculaire et Macroscopique, Combustion (EM2C), Université Paris Saclay (COmUE)-Centre National de la Recherche Scientifique (CNRS)-CentraleSupélec, von Karman Institute for Fluid Dynamics (VKI), Agence Spatiale Européenne = European Space Agency (ESA), CentraleSupélec-Centre National de la Recherche Scientifique (CNRS)-Université Paris Saclay (COmUE)
Jazyk: angličtina
Rok vydání: 2006
Předmět:
Zdroj: Journal of Geophysical Research. Planets
Journal of Geophysical Research. Planets, Wiley-Blackwell, 2006, 111, pp.12. ⟨10.1029/2005JE002640⟩
Journal of Geophysical Research, 111, e07S01. American Geophysical Union (AGU) / Wiley
Journal of Geophysical Research. Planets, 2006, 111, pp.12. ⟨10.1029/2005JE002640⟩
ISSN: 2169-9097
2169-9100
Popis: Coordinated ground-based observations of Titan were performed around or during the Huygens atmospheric probe mission at Titan on 14 January 2005, connecting the momentary in situ observations by the probe with the synoptic coverage provided by continuing ground-based programs. These observations consisted of three different categories: (1) radio telescope tracking of the Huygens signal at 2040 MHz, (2) observations of the atmosphere and surface of Titan, and (3) attempts to observe radiation emitted during the Huygens Probe entry into Titan's atmosphere. The Probe radio signal was successfully acquired by a network of terrestrial telescopes, recovering a vertical profile of wind speed in Titan's atmosphere from 140 km altitude down to the surface. Ground-based observations brought new information on atmosphere and surface properties of the largest Saturnian moon. No positive detection of phenomena associated with the Probe entry was reported. This paper reviews all these measurements and highlights the achieved results. The ground-based observations, both radio and optical, are of fundamental importance for the interpretation of results from the Huygens mission.
Databáze: OpenAIRE