Disclaimer: This material is being kept online for historical purposes. Though accurate at the time of publication, it is no longer being updated. The page may contain broken links or outdated information, and parts may not function in current web browsers. Visit espo.nasa.gov for information about our current projects.

 

Simulations of Titan’s brightness by a two-dimensional haze model

Hutzell, W. T., C. P. McKay, O. B. Toon, and F. Hourdin (1996), Simulations of Titan’s brightness by a two-dimensional haze model, Icarus, 119, 112-129.