Results 1 to 10 of about 2,267 (263)
Convective Self‐Aggregation Occurs Without Radiative Feedbacks in Warm Climates
Geophysical Research Letters, 2023 Previous research showed that radiative feedbacks are essential to the spontaneous development of convective aggregation (CSA) in idealized atmosphere models.
Lin Yao
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Radiative Feedbacks From Stochastic Variability in Surface Temperature and Radiative Imbalance [PDF]
Geophysical Research Letters, 2018 AbstractEstimates of radiative feedbacks obtained by regressing fluctuations in top‐of‐atmosphere (TOA) energy imbalance and surface temperature depend critically on the sampling interval and on assumptions about the nature of the stochastic forcing driving internal variability.
Gérard Roe +2 more
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Radiative feedbacks on global precipitation
Environmental Research Letters, 2010 The radiative kernel technique is employed to quantify twenty-first century changes to the tropospheric energy budget in the Intergovernmental Panel on Climate Change (IPCC) Fourth Assessment Report (AR4) models in order to better understand changes in global-mean precipitation. The strongest feedbacks on the tropospheric radiative cooling are found to
Michael Previdi
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Journal of Climate, 2015 AbstractIn this study, radiative kernels are used to separate direct radiative forcing from radiative adjustments to that forcing to quantify the magnitude and intermodel spread of tropospheric and stratospheric adjustments in coupled ocean–atmosphere climate models.
Brian Soden, Eui-Seok Chung
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Geophysical Research Letters, 2023 Radiative feedbacks govern the Earth's climate sensitivity and elucidate the geographic patterns of climate change in response to a carbon‐dioxide forcing.
Nicole Feldl, Timothy M. Merlis
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Radiative Feedback in Galaxies [PDF]
Proceedings of the International Astronomical Union, 2007 AbstractWe examine the fate of ionizing radiation from massive stars on global scales. First, we compare the observed Hα luminosities of LMC Hii regions with those predicted by the latest generation of stellar atmosphere models. Our results imply that classical Hii regions are on average radiation-bounded, rather than density-bounded, as we found a ...
M. S. Oey +5 more
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Effects of alternative cloud radiation parameterizations in a general circulation model [PDF]
Annales Geophysicae, 1996 Using the National Center for Atmospheric Research (NCAR) general circulation model (CCM2), a suite of alternative cloud radiation parameterizations has been tested.
W.-H. Lee, R. C. J. Somerville
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Detectable signatures of cosmic radiative feedback [PDF]
Monthly Notices of the Royal Astronomical Society, 2008 9 pages, 7 figures, accepted for publication in ...
Schneider, R. +6 more
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Simulations of galaxy formation with radiative transfer: Hydrogen reionization and radiative feedback [PDF]
Monthly Notices of the Royal Astronomical Society, 2010 We carry out hydrodynamical simulations of galaxy formation that simultaneously follow radiative transfer of hydrogen-ionizing photons, based on the optically-thin variable Eddington tensor approximation as implemented in the {\small GADGET} code. We consider only star-forming galaxies as sources and examine to what extent they can yield a reasonable ...
Petkova, M., Springel, V.
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On the diagnosis of radiative feedback in the presence of unknown radiative forcing [PDF]
Journal of Geophysical Research: Atmospheres, 2010 The impact of time‐varying radiative forcing on the diagnosis of radiative feedback from satellite observations of the Earth is explored. Phase space plots of variations in global average temperature versus radiative flux reveal linear striations and spiral patterns in both satellite measurements and in output from coupled climate models.
Roy W. Spencer, William D. Braswell
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