| Literature DB >> 16319827 |
M Fulchignoni1, F Ferri, F Angrilli, A J Ball, A Bar-Nun, M A Barucci, C Bettanini, G Bianchini, W Borucki, G Colombatti, M Coradini, A Coustenis, S Debei, P Falkner, G Fanti, E Flamini, V Gaborit, R Grard, M Hamelin, A M Harri, B Hathi, I Jernej, M R Leese, A Lehto, P F Lion Stoppato, J J López-Moreno, T Mäkinen, J A M McDonnell, C P McKay, G Molina-Cuberos, F M Neubauer, V Pirronello, R Rodrigo, B Saggin, K Schwingenschuh, A Seiff, F Simões, H Svedhem, T Tokano, M C Towner, R Trautner, P Withers, J C Zarnecki.
Abstract
On the basis of previous ground-based and fly-by information, we knew that Titan's atmosphere was mainly nitrogen, with some methane, but its temperature and pressure profiles were poorly constrained because of uncertainties in the detailed composition. The extent of atmospheric electricity ('lightning') was also hitherto unknown. Here we report the temperature and density profiles, as determined by the Huygens Atmospheric Structure Instrument (HASI), from an altitude of 1,400 km down to the surface. In the upper part of the atmosphere, the temperature and density were both higher than expected. There is a lower ionospheric layer between 140 km and 40 km, with electrical conductivity peaking near 60 km. We may also have seen the signature of lightning. At the surface, the temperature was 93.65 +/- 0.25 K, and the pressure was 1,467 +/- 1 hPa.Entities:
Year: 2005 PMID： 16319827 DOI： 10.1038/nature04314
Source DB: PubMed Journal: Nature ISSN： 0028-0836 Impact factor: 49.962