Clouds and the Faint Young Sun Paradox
Colin Goldblatt, Kevin J. Zahnle

TL;DR
This study examines how different cloud types and properties could have influenced Earth's early climate to address the Faint Young Sun Paradox, concluding clouds alone cannot fully resolve it.
Contribution
It provides a detailed radiative analysis of cloud effects on early Earth's climate, constraining their potential role in resolving the FYSP.
Findings
Low clouds contribute up to +15 Wm-2 forcing.
High clouds can provide up to +15 Wm-2 forcing with extreme modifications.
Cloud effects alone are insufficient to resolve the FYSP.
Abstract
We investigate the role which clouds could play in resolving the Faint Young Sun Paradox (FYSP). Lower solar luminosity in the past means that less energy was absorbed on Earth (a forcing of -50 Wm-2 during the late Archean), but geological evidence points to the Earth being at least as warm as it is today, with only very occasional glaciations. We perform radiative calculations on a single global mean atmospheric column. We select a nominal set of three layered, randomly overlapping clouds, which are both consistent with observed cloud climatologies and reproduce the observed global mean energy budget of Earth. By varying the fraction, thickness, height and particle size of these clouds we conduct a wide exploration of how changed clouds could affect climate, thus constraining how clouds could contribute to resolving the FYSP. Low clouds reflect sunlight but have little greenhouse…
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