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The Characterisation of Titan's Atmospheric Physical Properties by the Huygens Atmospheric Structure Instrument (Hasi) |
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| Authors: | Fulchignoni M Ferri F Angrilli F Bar-Nun A Barucci MA Bianchini G Borucki W Coradini M Coustenis A Falkner P Flamini E Grard R Hamelin M Harri AM Leppelmeier GW Lopez-Moreno JJ McDonnell JAM McKay CP Neubauer FH Pedersen A Picardi G Pirronello V Rodrigo R Schwingenschuh K Seiff A Svedhem H Vanzani V Zarnecki J |
| Institution: | 1.Département de Recherche Spatiale (DESPA), Obs, Paris-Meudon, France ;2.Université Denis Diderot - Paris 7, France ;3.C.I.S.A.S. Centre of Studies and Activities for Space G. Colombo, Univ. Padova (UPD), Italy ;4.Dept. Of Geophysics and Planetary Sciences, Univ. Tel Aviv, Israel ;5.NASA/AMES, Moffett Field, CA, 94035, USA ;6.ESA, Science Directorate, Paris, France ;7.Solar System Division (SSD), ESTEC, Noordwijk, The Netherlands ;8.Agenzia Spaziale Italiana, Roma, Italy ;9.Laboratoire de Physique et Chimie de l'Environnement (LPCE), Orleans, France ;10.Finnish Meteorological Institute (FMI), Helsinki, Finland ;11.Instituto de Astrofisica de Andalucia (IAA-CSIC), Granada, Spain ;12.University of Kent (UKC), Canterbury, UK ;13.University of K?ln, Germany ;14.University of Oslo, Norway ;15.University La Sapienza, Roma, Italy ;16.Osservatorio Astrofisico di Catania, Italy ;17.Space Research Institute, Austrian Academy of Sciences (IWF), Graz, Austria ;18.Dept. of Meteorology, San José State University Foundation, San José, CA, 95192-0104 ; |
| Abstract: | The Huygens Atmospheric Structure Instrument (HASI) is a multi-sensor package which has been designed to measure the physical quantities characterising the atmosphere of Titan during the Huygens probe descent on Titan and at the surface. HASI sensors are devoted to the study of Titan's atmospheric structure and electric properties, and to provide information on its surface, whether solid or liquid. This revised version was published online in August 2006 with corrections to the Cover Date. |
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