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The characterisation of Titan's atmospheric physical properties by the Huygens Atmospheric Structure Instrument (HASI)

Fulchignoni, M.; Ferri, F.; Angrilli, F.; Bar-Nun, A.; Barucci, M.A.; Bianchini, G.; Borucki, W.; Coradini, M.; Coustenis, A.; Falkner, P.; Flamini, E.; Grard, R.; Hamelin, M.; Harri, A.M.; Leppelmeier, G.W.; Lopez-Moreno, J.J.; McDonnell, J.A.M.; McKay, C.P.; Neubauer, F.H.; Pedersen, A.; Picardi, G.; Pirronello, V.; Rodrigo, R.; Schwingenschuh, K.; Seiff, A.; Svedhem, H.; Vanzani, V. and Zarnecki, J. (2002). The characterisation of Titan's atmospheric physical properties by the Huygens Atmospheric Structure Instrument (HASI). Space Science Reviews, 104(1-4) pp. 395–431.

DOI (Digital Object Identifier) Link: http://dx.doi.org/10.1023/A:1023688607077
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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.

Item Type: Journal Article
ISSN: 0038-6308
Academic Unit/Department: Other Departments > Other Departments
Science > Physical Sciences
Interdisciplinary Research Centre: Centre for Earth, Planetary, Space and Astronomical Research (CEPSAR)
Item ID: 4794
Depositing User: Users 6044 not found.
Date Deposited: 11 Jul 2006
Last Modified: 24 Jul 2014 09:25
URI: http://oro.open.ac.uk/id/eprint/4794
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