Sign Up to like & get
recommendations!
0
Published in 2018 at "Monthly Notices of the Royal Astronomical Society"
DOI: 10.1093/mnras/stx2428
Abstract: At optical wavelengths, Titan's brightness for large Sun-Titan-observer phase angles significantly exceeds its dayside brightness. The brightening that occurs near back-illumination is due to moderately large haze particles in the moon's extended atmosphere that forward-scatter…
read more here.
Keywords:
phase;
exoplanet phase;
forward scattering;
phase angles ... See more keywords