Correlations between Cassini VIMS spectra and RADAR SAR images: Implications for Titan's surface composition and the character of the Huygens Probe Landing Site

By L. Soderblom, R. Kirk, Jonathan I. Lunine, Jeffrey A. Anderson, K. Baines, Jason W. Barnes, J. Barrett, Robert H. Brown, B. Buratti, R. Clark and 17 more. 2007

190 citations recorded by the source corpus.

Subfields: Astronomy and Astrophysics, Atmospheric Science

View Paper: https://www.semanticscholar.org/paper/a203ea7c888a9794a0dbaa630f9b0795e71bda44

How researchers see this paper

The researchers whose trusted networks rank it highest, strongest advocate first. Every researcher gets a different order.

In Astronomy and Astrophysics

1. Jason W. Barnes
2. R. Clark
3. Ralf Jaumann
4. Jon Fortney
5. Sara Seager
6. Leslie A. Rogers

In Atmospheric Science

1. Ralf Jaumann

Citations in the corpus

• Spectroscopy, morphometry, and photoclinometry of Titan's dunefields from Cassini/VIMS (2008, methodology): “…calling the areas “sand” is arbitrary Near the west end of the swath, at 15.9 ◦ N 63.2 ◦ W, is an outcrop of the equatorial bright spectral unit [as described in Barnes et al. (2007a); this unit corresponds to the bright neutral unit from Soderblom et al. (2007) near the equator] 5–10 km across .”