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Revisiting the scattering greenhouse effect of CO2 ice clouds
Earth and Planetary Astrophysics · Submitted 6 Jan 2016
abstract compiled · 2026-09-23 · no language-model review
The authors' main claim Using accurate radiative transfer models with a general discrete ordinate method, this study revisits this important effect and shows that the positive climatic impact of carbon dioxide clouds was strongly overestimated in the past.
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The abstract, sentence by sentence
Carbon dioxide ice clouds are thought to play an important role for cold terrestrial planets with thick CO2 dominated atmospheres. Various previous studies showed that a scattering greenhouse effect by carbon dioxide ice clouds could result in a massive warming of the planetary surface. However, all of these studies only employed simplified two-stream radiative transfer schemes to describe the anisotropic scattering. Using accurate radiative transfer models with a general discrete ordinate method, this study revisits this important effect and shows that the positive climatic impact of carbon dioxide clouds was strongly overestimated in the past. The revised scattering greenhouse effect can have important implications for the early Mars, but also for planets like the early Earth or the position of the outer boundary of the habitable zone.
background contribution method result interpretation main claim
| # | sentence | role | the authors' own work | states the main conclusion | strength |
|---|---|---|---|---|---|
| s0 | Carbon dioxide ice clouds are thought to play an important role for cold terrestrial planets with thick CO2 dominated atmospheres. | background 1.00 | 0.04 | 0.02 | hedged possibility 0.90 |
| s1 | Various previous studies showed that a scattering greenhouse effect by carbon dioxide ice clouds could result in a massive warming of the planetary surface. | background 1.00 | 0.03 | 0.03 | hedged possibility 0.95 |
| s2 | However, all of these studies only employed simplified two-stream radiative transfer schemes to describe the anisotropic scattering. | gap 0.97 | 0.06 | 0.03 | asserted 1.00 |
| s3 | Using accurate radiative transfer models with a general discrete ordinate method, this study revisits this important effect and shows that the positive climatic impact of carbon dioxide clouds was strongly overestimated in the past. | contribution 0.52 | 0.96 | 0.95 | asserted 1.00 |
| s4 | The revised scattering greenhouse effect can have important implications for the early Mars, but also for planets like the early Earth or the position of the outer boundary of the habitable zone. | interpretation 1.00 | 0.48 | 0.09 | hedged possibility 0.94 |
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The paper
Original abstract
Carbon dioxide ice clouds are thought to play an important role for cold terrestrial planets with thick CO2 dominated atmospheres. Various previous studies showed that a scattering greenhouse effect by carbon dioxide ice clouds could result in a massive warming of the planetary surface. However, all of these studies only employed simplified two-stream radiative transfer schemes to describe the anisotropic scattering. Using accurate radiative transfer models with a general discrete ordinate method, this study revisits this important effect and shows that the positive climatic impact of carbon dioxide clouds was strongly overestimated in the past. The revised scattering greenhouse effect can have important implications for the early Mars, but also for planets like the early Earth or the position of the outer boundary of the habitable zone.
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How the literature uses it
1 arXiv paper cite this in 1 sentence
Papers whose main result relates to this one's
States the same result 1 paper
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Consequently, the scattering greenhouse effect of CO2 ice particles seems to be less effective than previously estimated.
Papers citing it
Contests it 1 paper
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As demonstrated in [ref] by using a multi-stream radiative transfer scheme ( [ref] ), the study, based two-stream radiative transfer scheme, overestimated the surface warming due to the scattering greenhouse effect by up to 80 K.
NCCR PlanetS: Observational and computational characterization of exoplanet atmospheres · Radiative transfer · contest 0.79
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