The Characterisation of Titan's Atmospheric Physical Properties by the Huygens Atmospheric Structure Instrument (Hasi)

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 atmosphe...

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Bibliographic Details
Published in:Space science reviews 2002-01, Vol.104 (1-4), p.395-431
Main 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
Format: Article
Language:English
Subjects:
Physical properties
Saturn
Sciences of the Universe
Space exploration
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Summary: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.
ISSN:0038-6308
1572-9672
DOI:10.1023/A:1023688607077