Saturn's south polar clouds are best explained by a four-layer model in which a thin upper haze lets ammonia ice show through, and shadows are cast by sharp steps in thin layers, not eyewalls.
Title resolution pending
1 Pith paper cite this work. Polarity classification is still indexing.
1
Pith paper citing it
fields
astro-ph.EP 1years
2019 1verdicts
CONDITIONAL 1representative citing papers
citing papers explorer
-
Saturn's south polar cloud composition and structure inferred from 2006 Cassini/VIMS spectra and ISS images
Saturn's south polar clouds are best explained by a four-layer model in which a thin upper haze lets ammonia ice show through, and shadows are cast by sharp steps in thin layers, not eyewalls.