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Fulchignoni M Ferri F Angrilli F Ball AJ Bar-Nun A Barucci MA Bettanini C Bianchini G Borucki W Colombatti G Coradini M Coustenis A Debei S Falkner P Fanti G Flamini E Gaborit V Grard R Hamelin M Harri AM Hathi B Jernej I Leese MR Lehto A Lion Stoppato PF López-Moreno JJ Mäkinen T McDonnell JA McKay CP Molina-Cuberos G Neubauer FM Pirronello V Rodrigo R Saggin B Schwingenschuh K Seiff A Simões F Svedhem H Tokano T Towner MC Trautner R Withers P Zarnecki JC 《Nature》2005,438(7069):785-791
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. 相似文献
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Zarnecki JC Leese MR Hathi B Ball AJ Hagermann A Towner MC Lorenz RD McDonnell JA Green SF Patel MR Ringrose TJ Rosenberg PD Atkinson KR Paton MD Banaszkiewicz M Clark BC Ferri F Fulchignoni M Ghafoor NA Kargl G Svedhem H Delderfield J Grande M Parker DJ Challenor PG Geake JE 《Nature》2005,438(7069):792-795
The surface of Saturn's largest satellite--Titan--is largely obscured by an optically thick atmospheric haze, and so its nature has been the subject of considerable speculation and discussion. The Huygens probe entered Titan's atmosphere on 14 January 2005 and descended to the surface using a parachute system. Here we report measurements made just above and on the surface of Titan by the Huygens Surface Science Package. Acoustic sounding over the last 90 m above the surface reveals a relatively smooth, but not completely flat, surface surrounding the landing site. Penetrometry and accelerometry measurements during the probe impact event reveal that the surface was neither hard (like solid ice) nor very compressible (like a blanket of fluffy aerosol); rather, the Huygens probe landed on a relatively soft solid surface whose properties are analogous to wet clay, lightly packed snow and wet or dry sand. The probe settled gradually by a few millimetres after landing. 相似文献
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本文证明了公式β(n)=σ(n-1)+1其中α(n-1)是n-1次多项式微分系统的不为直线的最多条数,βn)是n次多项式微分系统的不变直线的不同斜率的最大个数。这里假设所讨论的多项式系统只有限条不变直线。 相似文献
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