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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. Zarnecki J. 《Space Science Reviews》2002,104(1-4):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.
This revised version was published online in August 2006 with corrections to the Cover Date. 相似文献
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