Results 11 to 20 of about 2,949 (160)

Observationally Constrained Cloud Phase Unmasks Orbitally Driven Climate Feedbacks

open access: yesGeophysical Research Letters, 2021
The mechanisms which amplify orbitally driven changes in insolation and drive the glacial cycles of the past 2.6 million years, the Pleistocene, are poorly understood.
Navjit Sagoo   +6 more
doaj   +1 more source

An observation-based method to assess tropical stratocumulus and shallow cumulus clouds and feedbacks in CMIP6 and CMIP5 models

open access: yesEnvironmental Research Communications, 2023
In the Earth system models (ESMs) participating in the Coupled Models Intercomparison Project phase 6 (CMIP6), the tropical low-cloud feedback is 50% more positive than its predecessors (CMIP5) and continues to dominate the spread in simulated climate ...
G V Cesana   +4 more
doaj   +1 more source

Acidity and the multiphase chemistry of atmospheric aqueous particles and clouds [PDF]

open access: yesAtmospheric Chemistry and Physics, 2021
The acidity of aqueous atmospheric solutions is a key parameter driving both the partitioning of semi-volatile acidic and basic trace gases and their aqueous-phase chemistry.
A. Tilgner   +11 more
doaj   +1 more source

Investigating the impact of cloud-radiative feedbacks on tropical precipitation extremes

open access: yesnpj Climate and Atmospheric Science, 2021
Although societally important, extreme precipitation is difficult to represent in climate models. This study shows one robust aspect of extreme precipitation across models: extreme precipitation over tropical oceans is strengthened through a positive ...
Brian Medeiros   +3 more
doaj   +1 more source

The impact of parametrized convection on cloud feedback [PDF]

open access: yesPhilosophical Transactions of the Royal Society A: Mathematical, Physical and Engineering Sciences, 2015
We investigate the sensitivity of cloud feedbacks to the use of convective parametrizations by repeating the CMIP5/CFMIP-2 AMIP/AMIP + 4K uniform sea surface temperature perturbation experiments with 10 climate models which have had their convective parametrizations turned off.
Webb, Mark J.   +17 more
openaire   +4 more sources

An underestimated negative cloud feedback from cloud lifetime changes

open access: yesNature Climate Change, 2021
As the atmosphere warms, part of the cloud population shifts from ice and mixed-phase (‘cold’) to liquid (‘warm’) clouds. Because warm clouds are more reflective and longer-lived, this phase change reduces the solar flux absorbed by the Earth and constitutes a negative radiative feedback.
Johannes Mülmenstädt   +8 more
openaire   +2 more sources

A cloud feedback emulator (CFE, version 1.0) for an intermediate complexity model [PDF]

open access: yesGeoscientific Model Development, 2017
The dominant source of inter-model differences in comprehensive global climate models (GCMs) are cloud radiative effects on Earth's energy budget. Intermediate complexity models, while able to run more efficiently, often lack cloud feedbacks.
D. J. Ullman, A. Schmittner
doaj   +1 more source

Explicitly Resolved Cloud Feedbacks in the Radiative‐Convective Equilibrium Model Intercomparison Project

open access: yesJournal of Advances in Modeling Earth Systems, 2023
Radiative‐convective equilibrium (RCE) is particularly well suited for studying tropical deep‐convection, a regime of clouds that contributes some of the highest uncertainties to the estimates of total cloud feedback.
C. L. Stauffer, A. A. Wing
doaj   +1 more source

Technical note: Recommendations for diagnosing cloud feedbacks and rapid cloud adjustments using cloud radiative kernels [PDF]

open access: yesAtmospheric Chemistry and Physics
The cloud radiative kernel method is a popular approach to quantify cloud feedbacks and rapid cloud adjustments to increased CO2 concentrations and to partition contributions from changes in cloud amount, altitude, and optical depth.
M. D. Zelinka   +5 more
doaj   +1 more source

Molecular cloud evolution – V. Cloud destruction by stellar feedback [PDF]

open access: yesMonthly Notices of the Royal Astronomical Society, 2013
We present a numerical study of the evolution of molecular clouds, from their formation by converging flows in the warm ISM, to their destruction by the ionizing feedback of the massive stars they form. We improve with respect to our previous simulations by including a different stellar-particle formation algorithm, which allows them to have masses ...
Colin, Pedro   +2 more
openaire   +2 more sources

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