| Article ID | Journal | Published Year | Pages | File Type |
|---|---|---|---|---|
| 1782766 | Planetary and Space Science | 2006 | 12 Pages |
Abstract
The Cassini orbital tour offers the opportunity for VIMS to image the same parts of Titan's surface repeatedly at many different illumination and observation geometries. This creates the possibility of understanding the properties of Titan's atmosphere and haze by iteratively adapting models to create a best fit to the surface reflectance properties.
Related Topics
Physical Sciences and Engineering
Earth and Planetary Sciences
Geophysics
Authors
R.M. Nelson, R.H. Brown, B.W. Hapke, W.D. Smythe, L. Kamp, M.D. Boryta, F. Leader, K.H. Baines, G. Bellucci, J.-P. Bibring, B.J. Buratti, F. Capaccioni, P. Cerroni, R.N. Clark, M. Combes, A. Coradini, D.P. Cruikshank, P. Drossart, C. Sotin,