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

被引：62

作者：

Fulchignoni, M ^{[1
]}

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

机构：

[1] Observ Paris, Dept Rech Spatiale, DESPA, Meudon, France

[2] Univ Padua, CISAS, Ctr Studies & Activ Space G Colombo, I-35100 Padua, Italy

[3] Univ Paris 07, F-75221 Paris 05, France

[4] Tel Aviv Univ, Dept Geophys & Planetary Sci, IL-69978 Tel Aviv, Israel

[5] NASA, AMES, Moffett Field, CA 94035 USA

[6] ESA, Sci Directorate, F-75738 Paris 15, France

[7] ESTEC, Solar Syst Div, Noordwijk, Netherlands

[8] Agenzia Spaziale Italiana, Rome, Italy

[9] LPCE, Orleans, France

[10] Finnish Meteorol Inst, FIN-00101 Helsinki, Finland

[11] CSIC, IAA, Granada, Spain

[12] Univ Kent, Canterbury, Kent, England

[13] Univ Cologne, D-5000 Cologne 41, Germany

[14] Univ Oslo, N-0316 Oslo, Norway

[15] Univ Roma La Sapienza, Rome, Italy

[16] Osserv Astrofis Catania, I-95125 Catania, Italy

[17] Austrian Acad Sci, Space Res Inst, A-8010 Graz, Austria

[18] San Jose State Univ Fdn, Dept Meteorol, San Jose, CA 95192 USA

来源：

SPACE SCIENCE REVIEWS | 2002年 / 104卷 / 1-2期

关键词：

D O I：

10.1023/A:1023688607077

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

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.

引用

页码：395 / 431

页数：37

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