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

@article{Fulchignoni2002TheCO,
  title={The Characterisation of Titan's Atmospheric Physical Properties by the Huygens Atmospheric Structure Instrument (Hasi)},
  author={M. Fulchignoni and F. Ferri and F. Angrilli and A. Bar-Nun and M. Barucci and G. Bianchini and W. Borucki and M. Coradini and A. Coustenis and P. Falkner and E. Flamini and R. Grard and M. Hamelin and A. Harri and G. Leppelmeier and J. Lopez-Moreno and J. McDonnell and C. McKay and F. Neubauer and A. Pedersen and G. Picardi and V. Pirronello and R. Rodrigo and K. Schwingenschuh and A. Seiff and H. Svedhem and V. Vanzani and J. Zarnecki},
  journal={Space Science Reviews},
  year={2002},
  volume={104},
  pages={395-431}
}
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. 
Huygens' measurements of the speed of sound on Titan
In situ measurements of the physical characteristics of Titan's environment
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