Rain, winds and haze during the Huygens probe's descent to Titan's surface

@article{Tomasko2005RainWA,
  title={Rain, winds and haze during the Huygens probe's descent to Titan's surface},
  author={Martin George Tomasko and Brent A. Archinal and T. L. Becker and Bruno B{\'e}zard and M. Bushroe and Michel Combes and Debbie Cook and Athena Coustenis and Catherine de Bergh and L. E. Dafoe and Lyn Doose and Sylvain Dout{\'e} and Andrew M. Eibl and S. Engel and Fritz Gliem and Bjoern Grieger and K. Holso and Elpitha Howington-Kraus and Erich Karkoschka and H. Uwe Keller and Randolf L. Kirk and Rainer Kramm and Michael K{\"u}ppers and Peter Lanagan and Emmanuel Lellouch and Mark T. Lemmon and J. L. Lunine and Elisabeth Ann McFarlane and John E. Moores and G. M. Prout and Bashar Rizk and Mark R. Rosiek and P. Rueffer and Stefan E. Schr{\"o}der and Bernard Schmitt and Charles See and P. H. Smith and Laurence A. Soderblom and Nicolas Thomas and Robert Mac West},
  journal={Nature},
  year={2005},
  volume={438},
  pages={765-778}
}
The irreversible conversion of methane into higher hydrocarbons in Titan's stratosphere implies a surface or subsurface methane reservoir. Recent measurements from the cameras aboard the Cassini orbiter fail to see a global reservoir, but the methane and smog in Titan's atmosphere impedes the search for hydrocarbons on the surface. Here we report spectra and high-resolution images obtained by the Huygens Probe Descent Imager/Spectral Radiometer instrument in Titan's atmosphere. Although these… 
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