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={M. Tomasko and B. Archinal and T. Becker and B. B{\'e}zard and M. Bushroe and M. Combes and D. Cook and A. Coustenis and C. Bergh and L. E. Dafoe and L. Doose and S. Dout{\'e} and A. Eibl and S. Engel and F. Gliem and B. Grieger and K. Holso and E. Howington-Kraus and E. Karkoschka and H. Keller and R. Kirk and R. Kramm and M. K{\"u}ppers and P. Lanagan and E. Lellouch and M. Lemmon and J. Lunine and E. McFarlane and J. Moores and G. Prout and B. Rizk and M. Rosiek and P. Rueffer and S. Schr{\"o}der and B. Schmitt and C. See and P. Smith and L. Soderblom and N. Thomas and R. 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… Expand
Composition of Titan's Surface
Titan's Tropical Storms in an Evolving Atmosphere
...
1
2
3
4
5
...

References

SHOWING 1-10 OF 43 REFERENCES
Imaging of Titan from the Cassini spacecraft
A physical model of Titan's aerosols.
The vertical profile of winds on Titan
In situ measurements of the physical characteristics of Titan's environment
Maps of Titan's surface from 1 to 2.5 μm
...
1
2
3
4
5
...