In the framework of the Cassini-Huygens mission towards the Saturnian system, the Huygens Atmospheric Structure Instrument (HASI) is a multisensor package which has been designed to measure the physical quantities characterizing the atmosphere of Titan, Saturn's largest satellite. HASI sensors are devoted to the study of Titan's atmospheric structure and electric properties, and also to provide information on the surface, whatever its phase, solid or liquid. A description of the experiment, its subsystems and sensors package is reported together with their performances. © 2002 International Astronautical Federation. Published by Elsevier Science Ltd. All rights reserved. © 2002 International Astronautical Federation. Published by Elsevier Science Ltd. All rights resreved.
Huygens atmospheric structure instrument of Huygens probe on Cassini mission
Ferri F.;
2002
Abstract
In the framework of the Cassini-Huygens mission towards the Saturnian system, the Huygens Atmospheric Structure Instrument (HASI) is a multisensor package which has been designed to measure the physical quantities characterizing the atmosphere of Titan, Saturn's largest satellite. HASI sensors are devoted to the study of Titan's atmospheric structure and electric properties, and also to provide information on the surface, whatever its phase, solid or liquid. A description of the experiment, its subsystems and sensors package is reported together with their performances. © 2002 International Astronautical Federation. Published by Elsevier Science Ltd. All rights reserved. © 2002 International Astronautical Federation. Published by Elsevier Science Ltd. All rights resreved.
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