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1-62 of about 62 matches for site:www.giss.nasa.gov abs regime
https://www.giss.nasa.gov/pubs/abs/ze07000h.html
Pubs.GISS: Zelinka et al. 2023: Detailing cloud property feedbacks with a regime-based decomposition Go to Main
https://www.giss.nasa.gov/pubs/abs/re08000i.html
Pubs.GISS: Rémillard and Tselioudis 2015: Cloud regime variability over the Azores and its application
https://www.giss.nasa.gov/pubs/abs/ch03010w.html
Pubs.GISS: Chen et al. 2011: Projected regime shift in Arctic cloud and water vapor feedbacks Go
https://www.giss.nasa.gov/pubs/abs/su03100m.html
Pubs.GISS: Su et al. 2013: Diagnosis of regime-dependent cloud simulation errors in CMIP5 models using
https://www.giss.nasa.gov/pubs/abs/mc07100r.html
Pubs.GISS: McCoy et al. 2020: A regime-oriented approach to observationally constraining extratropical shortwave... Go to
https://www.giss.nasa.gov/pubs/abs/mi02310d.html
Pubs.GISS: Miller et al. 2007: Future regime shift in feedbacks during Arctic winter Go to Main
https://www.giss.nasa.gov/pubs/abs/al03000u.html
1995: Richardson number constraints for the Jupiter and outer planet wind regime Go to Main
https://www.giss.nasa.gov/pubs/abs/pa05700x.html
on the atmospheric boundary layer is described by means of a regime classification based on Self
https://www.giss.nasa.gov/pubs/abs/ca04900a.html
model underestimates the convective flux F c in the high-efficiency regime, while it overestimates F
https://www.giss.nasa.gov/pubs/abs/ta05200z.html
novel "double decomposition method" that employs the "cloud radiative kernel" and "cloud regime" concepts, to two
https://www.giss.nasa.gov/pubs/abs/wi05100g.html
the cloud response to climate change is analysed in the cloud-regime framework. Most of
https://www.giss.nasa.gov/pubs/abs/ca01200l.html
so strong that it suppresses the energy cascade process and no inertial regime can develop. In
https://www.giss.nasa.gov/pubs/abs/we07300l.html
the planet was dominated by higher mantle temperatures (by about 200°C), an uncertain tectonic regime that likely included squishy
https://www.giss.nasa.gov/pubs/abs/ch04510y.html
interest. The main results are as follows: In the non-degenerate regime the reaction
https://www.giss.nasa.gov/pubs/abs/de05000n.html
of superrotating zonal winds increases with rotation rate in the slowly rotating regime when other parameters are
https://www.giss.nasa.gov/pubs/abs/ch06500y.html
the energy loss rate is significantly reduced both in the low-density regime ρ ≲ 10 7 g
https://www.giss.nasa.gov/pubs/abs/ca04720o.html
2011 (SR11) using the following mesoscale model. The adiabatic (A) regime was modeled with the
https://www.giss.nasa.gov/pubs/abs/ca04710r.html
In the ocean, there are two main regimes where non-local transport is important. One regime is where storms release
https://www.giss.nasa.gov/pubs/abs/cr02100m.html
subset of latest climate models participating in CMIP6. We strive for regime-oriented model validation and
https://www.giss.nasa.gov/pubs/abs/ca05900x.html
3, in accord with recent data; (2) in the inertial-conductive regime, the model
https://www.giss.nasa.gov/pubs/abs/ji07300l.html
drought is severe enough to cause a shift from an energy-limited regime to a
https://www.giss.nasa.gov/pubs/abs/de04200b.html
the equatorial Venus atmosphere and the possibility of a similar regime on Titan are examined
https://www.giss.nasa.gov/pubs/abs/ch09800r.html
I). In this study, it is shown that one of several PDV interdecadal regime shifts occurred during the
https://www.giss.nasa.gov/pubs/abs/ja03300h.html
a planet's surface that falls in the 0 ≤ T ≤ 100°C temperature regime, we find a
https://www.giss.nasa.gov/pubs/abs/de01200l.html
profile. Relative humidity just below cloud top is low in the moist convective regime but increases steadily with
https://www.giss.nasa.gov/pubs/abs/la00200p.html
to a few ×10 6 years, depending on the chemistry and regime. The time
https://www.giss.nasa.gov/pubs/abs/ca05710o.html
two arguments most frequently cited to neglect Σ: (1) in an adiabatic regime, fluxes across isopycnal surfaces
https://www.giss.nasa.gov/pubs/abs/dr01100t.html
importance of sensible versus latent heating in maintaining the summertime regime. Armed with a
https://www.giss.nasa.gov/pubs/abs/ca08320k.html
that the presence of vorticity in a stably stratified regime, such as the
https://www.giss.nasa.gov/pubs/abs/mi00220m.html
and the favored assumption was found to be sensitive to cloud regime (cumuliform/stratiform). Confirming previous
https://www.giss.nasa.gov/pubs/abs/in02000x.html
plasmons) in a hot, dense stellar plasma is calculated for a regime of temperatures
https://www.giss.nasa.gov/pubs/abs/ha02100q.html
wetland areas. Scenarios indicate higher temperatures and greater evapotranspiration altering the hydrologic regime such that fresh-water
https://www.giss.nasa.gov/pubs/abs/ts00300k.html
derived WSs with vertical velocity measurements shows a normal progression in dynamic regime when moving from the
https://www.giss.nasa.gov/pubs/abs/mi09600g.html
zero independently of the compaction state. In the geometrical optics regime, the asymmetry
https://www.giss.nasa.gov/pubs/abs/ca00410c.html
values of densities and temperatures. In the low density regime (ρ ≲ 10 7 g
https://www.giss.nasa.gov/pubs/abs/ri00800v.html
opportunity to assess how atmospheric circulation changes when in a different climate regime, one characterized by much
https://www.giss.nasa.gov/pubs/abs/ma02300a.html
GCM. The realistic depiction of evaporation also affects the thermal regime in the
https://www.giss.nasa.gov/pubs/abs/st03900e.html
simple model for the structure of a non-rotating Hadley regime in an
https://www.giss.nasa.gov/pubs/abs/ca05700m.html
and the horizontal extent may be small in a weak dynamic regime or large in
https://www.giss.nasa.gov/pubs/abs/cr03000u.html
the Aral Sea resulted in dramatic changes in the salinity regime and, consequently
https://www.giss.nasa.gov/pubs/abs/du03100n.html
1 (WS1) deep convection cloud state and an independent, microwave-based deep convective precipitation regime developed here. The
https://www.giss.nasa.gov/pubs/abs/bl03000u.html
transition of D 2 in helium in the low pressure regime where Dicke narrowing is
https://www.giss.nasa.gov/pubs/abs/ku03100m.html
the tropical atmosphere. This study examines the evolution of the hydrologic regime from before the
https://www.giss.nasa.gov/pubs/abs/ca01620b.html
The resulting vertical velocity depends on the extent of the SM regime, the horizontal
https://www.giss.nasa.gov/pubs/abs/de09600r.html
gas concentrations do not necessarily produce more open ocean area because of possible dynamic regime transitions. For an
https://www.giss.nasa.gov/pubs/abs/ts06000k.html
complicated behavior that could be related to changes in the dynamical regime in which
https://www.giss.nasa.gov/pubs/abs/ha04510h.html
regimes. The regimes associated with cyclones have the highest in-regime shortwave cloud radiative effect
https://www.giss.nasa.gov/pubs/abs/al07100z.html
The diagnostic analysis of numerical simulations of the Venus/Titan wind regime reveals an overlooked constraint
https://www.giss.nasa.gov/pubs/abs/ot00100w.html
and cirrus optical depth, which was found in the subvisual/threshold-visible regime, confirming the utility
https://www.giss.nasa.gov/pubs/abs/ro02800o.html
particular, the Northern Hemisphere (NH) subtropics undergo a change in dynamic regime during the local
https://www.giss.nasa.gov/pubs/abs/he03300h.html
past several years has resulted in significant changes of the percolation regime of the
https://www.giss.nasa.gov/pubs/abs/al07000g.html
off not only for large particle sizes but also in small particles regime which prevents the
https://www.giss.nasa.gov/pubs/abs/ji00100k.html
reduce the capacity for carbon sequestration as RDOC. The nutrient regime enabling maximum carbon storage
https://www.giss.nasa.gov/pubs/abs/ka08300m.html
to exoplanet demographics that can be placed in the potential runaway greenhouse regime where Venus analogs are
https://www.giss.nasa.gov/pubs/abs/mc06100q.html
and aerosol to cloud. Here, we restrict our analysis to the regime of extratropical
https://www.giss.nasa.gov/pubs/abs/ca04320y.html
Southern Ocean, where there is the largest CO 2 absorption, the dominant regime is diffusive convection discussed
https://www.giss.nasa.gov/pubs/abs/pe03100m.html
the Holocene warming appears to be greater than that generated by an equivalent insolation regime 80 ka. A
https://www.giss.nasa.gov/pubs/abs/ne00100k.html
layer schemes for weather and climate models for this cloud regime, using large-eddy simulations
https://www.giss.nasa.gov/pubs/abs/ri00200p.html
that the stratospheric response is very individualistic to the particular climate regime, and the
https://www.giss.nasa.gov/pubs/abs/fa09000j.html
and they can be considered to be in an eddy saturated regime. Larger contrasts arise when
https://www.giss.nasa.gov/pubs/abs/ca09220p.html
model reproduces. Heat to salt flux ratio. In the Ri ≫ 1 regime, the RSM
https://www.giss.nasa.gov/pubs/abs/ca01400w.html
lies the fact that we are dealing with a highly nonlinear, turbulent regime under the action