-
Zhang, Y., D. J. Seidel, J.-C. Golaz, C. Deser, and R. A. Tomas, 2011:
Climatological characteristics of Arctic and Antarctic surface-based
inversions.
J. Climate, 24, 5167-5186,
doi: 10.1175/2011JCLI4004.1
(pdf, 15M)
Abstract
Surface-based inversions (SBIs) are frequent features of the Arctic and Antarctic atmospheric boundary
layer. They influence vertical mixing of energy, moisture and pollutants, cloud formation, and surface ozone
destruction. Their climatic variability is related to that of sea ice and planetary albedo, important factors in
climate feedback mechanisms. However, climatological polar SBI properties have not been fully characterized
nor have climate model simulations of SBIs been compared comprehensively to observations. Using 20
years of twice-daily observations from 39 Arctic and 6 Antarctic radiosonde stations, this study examines the
spatial and temporal variability of three SBI characteristic—frequency of occurrence, depth (from the surface
to the inversion top), and intensity (temperature difference over the SBI depth)—and relationships among
them. In both polar regions, SBIs are more frequent, deeper, and stronger in winter and autumn than in
summer and spring. In the Arctic, these tendencies increase from the Norwegian Sea eastward toward the
East Siberian Sea, associated both with (seasonal and diurnal) variations in solar elevation angle at the
standard radiosonde observation times and with differences between continental and maritime climates. Two
state-of-the-art climate models and one reanalysis dataset show similar seasonal patterns and spatial distributions
of SBI properties as the radiosonde observations, but with biases in their magnitudes that differ
among the models and that are smaller in winter and autumn than in spring and summer. SBI frequency,
depth, and intensity are positively correlated, both spatially and temporally, and all three are anticorrelated
with surface temperature.
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Guo, H., J.-C. Golaz, and L. J. Donner, 2011:
Aerosol effects on stratocumulus water paths in a PDF‐based parameterization.
Geophys. Res. Lett., 38, L17808,
doi: 10.1029/2011GL048611
(pdf, 406k)
Abstract
Successful simulation of aerosol indirect effects in
climate models requires parameterizations that capture the
full range of cloud‐aerosol interactions, including positive
and negative liquid water path (LWP) responses to
increasing aerosol concentrations, as suggested by large
eddy simulations (LESs). A parameterization based on
multi‐variate probability density functions with dynamics
(MVD PDFs) has been incorporated into the single‐column
version of GFDL AM3, extended to treat aerosol activation,
and coupled with a two‐moment microphysics scheme. We
use it to explore cloud‐aerosol interactions. In agreement
with LESs, our single‐column simulations produce both
positive and negative LWP responses to increasing aerosol
concentrations, depending on precipitation and free
atmosphere relative humidity. We have conducted sensitivity
tests to vertical resolution and droplet sedimentation
parameterization. The dependence of sedimentation on cloud
droplet size is essential to capture the full LWP responses to
aerosols. Further analyses reveal that the MVD PDFs are
able to represent changes in buoyancy profiles induced by
sedimentation as well as enhanced entrainment efficiency
with aerosols comparable to LESs.
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Golaz, J.-C., M. Salzmann, L. J. Donner, L. W. Horowitz, Y. Ming, and M. Zhao, 2011:
Sensitivity of the aerosol indirect effect to subgrid variability in the cloud
parameterization of the GFDL Atmosphere General Circulation Model AM3.
J. Climate, 24, 3145-3160,
doi: 10.1175/2010JCLI3945.1
(pdf, 778k)
Abstract
The recently developed GFDL Atmospheric Model version 3 (AM3), an atmospheric general circulation
model (GCM), incorporates a prognostic treatment of cloud drop number to simulate the aerosol indirect
effect. Since cloud drop activation depends on cloud-scale vertical velocities, which are not reproduced in
present-day GCMs, additional assumptions on the subgrid variability are required to implement a local activation
parameterization into a GCM.
This paper describes the subgrid activation assumptions in AM3 and explores
sensitivities by constructing alternate configurations. These alternate model configurations exhibit only
small differences in their present-day climatology. However, the total anthropogenic radiative flux perturbation
(RFP) between present-day and preindustrial conditions varies by +/-50% from the reference, because
of a large difference in the magnitude of the aerosol indirect effect. The spread in RFP does not originate
directly from the subgrid assumptions but indirectly through the cloud retuning necessary to maintain
a realistic radiation balance. In particular, the paper shows a linear correlation between the choice of
autoconversion threshold radius and the RFP.
Climate sensitivity changes only minimally between the reference and alternate configurations. If implemented
in a fully coupled model, these alternate configurations would therefore likely produce substantially
different warming from preindustrial to present day.
-
Donner, L. J., B. L. Wyman, R. S. Hemler, L. W. Horowitz, Y. Ming, M. Zhao,
J.-C. Golaz, J. Austin, W. F. Cooke, S. R. Freidenreich, P. Ginoux, C.T. Gordon,
S. Griffies, I. M. Held, W. J. Hurlin, S. A. Klein, A. R. Langenhorst, H.-C. Lee,
S.-J. Lin, S. L. Maleyshev, P.C.D. Milly, M. J. Nath, R. Pincus, J. J. Ploshay,
V. Ramaswamy, M. D. Schwarzkopf, C. J. Seman, E. Shevliakova, J. J. Sirutis,
W. F. Stern, R. J. Stouffer, R. J. Wilson, M. Winton, and A. T. Wittenberg, 2011:
The dynamical core, physical parameterizations, and basic simulation characteristics of
the atmospheric component of the GFDL Global Coupled Model CM3.
J. Climate, 24, 3484-3519,
doi: 10.1175/2011JCLI3955.1
(pdf, 13M)
Abstract
The Geophysical Fluid Dynamics Laboratory (GFDL) has developed a coupled general circulation model (CM3) for the atmosphere,
oceans, land, and sea ice. The goal of CM3 is to address emerging issues in climate change, including aerosol–cloud interactions,
chemistry–climate interactions, and coupling between the troposphere and stratosphere. The model is also designed to serve as the
physical system component of earth system models and models for decadal prediction in the near-term future—for example, through
improved simulations in tropical land precipitation relative to earlier-generation GFDL models. This paper describes the dynamical core, physical parameterizations, and basic simulation characteristics of the atmospheric component (AM3) of this model. Relative to GFDL AM2, AM3 includes new treatments of deep and shallow cumulus convection, cloud droplet activation by aerosols, subgrid variability of stratiform vertical velocities for droplet activation, and atmospheric chemistry driven by emissions with advective, convective, and turbulent transport. AM3 employs a cubed-sphere implementation of a finite-volume dynamical core and is coupled to LM3, a new land model with ecosystem dynamics and hydrology. Its horizontal resolution is approximately 200 km, and its vertical resolution ranges approximately from 70 m near the earth’s surface to 1 to 1.5 km near the tropopause and 3 to 4 km in much of the stratosphere. Most basic circulation features in AM3 are simulated as realistically, or more so, as in AM2. In particular, dry biases have been reduced over South America. In coupled mode, the simulation of Arctic sea ice concentration has improved. AM3 aerosol optical depths, scattering properties, and surface clear-sky downward shortwave radiation are more realistic than in AM2. The simulation of marine stratocumulus decks remains problematic, as in AM2. The most intense 0.2% of precipitation rates occur less frequently in AM3 than observed. The last two decades of the twentieth century warm in CM3 by 0.32 C relative to 1881–1920. The Climate Research Unit (CRU) and Goddard Institute for Space Studies analyses of observations show warming of 0.56 and 0.52 C, respectively, over this period. CM3 includes anthropogenic cooling by aerosol–cloud interactions, and its warming by the late twentieth century is somewhat less realistic than in CM2.1, which warmed 0.66 C but did not include aerosol–cloud interactions. The improved simulation of the direct aerosol effect (apparent in surface clear-sky downward radiation) in CM3 evidently acts in concert with its simulation of cloud–aerosol interactions to limit greenhouse gas warming.
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G. L. Stephens, T. L'Ecuyer, R. Forbes, A. Gettelmen, J.-C. Golaz, A. Bodas-Salcedo, K. Suzuki, P. Gabriel and J. Haynes, 2010: Dreary state of precipitation in global models.
J. Geophys. Res, 115, D24211,
doi: 10.1029/2010JD014532
(pdf, 6.2M)
Abstract
New, definitive measures of precipitation frequency provided by CloudSat are used to
assess the realism of global model precipitation. The character of liquid precipitation
(defined as a combination of accumulation, frequency, and intensity) over the global
oceans is significantly different from the character of liquid precipitation produced by
global weather and climate models. Five different models are used in this comparison
representing state‐of‐the‐art weather prediction models, state‐of‐the‐art climate models,
and the emerging high‐resolution global cloud “resolving” models. The differences
between observed and modeled precipitation are larger than can be explained by
observational retrieval errors or by the inherent sampling differences between observations
and models. We show that the time integrated accumulations of precipitation produced by
models closely match observations when globally composited. However, these models
produce precipitation approximately twice as often as that observed and make rainfall far
too lightly. This finding reinforces similar findings from other studies based on surface
accumulated rainfall measurements. The implications of this dreary state of model
depiction of the real world are discussed.
-
H. Guo, J.-C. Golaz, L. J. Donner, V. E. Larson, D. P. Schanen and B. M. Griffin, 2010: Multi-variate probability density functions with dynamics for cloud droplet
activation in large-scale models: single column tests.
Geosci. Model Dev., 3, 475-486,
doi: 10.5194/gmd-3-475-2010
(pdf, 6.9M)
Abstract
Successful simulation of cloud-aerosol interactions (indirect aerosol effects) in climate models requires relating grid-scale aerosol, dynamic, and thermodynamic fields to small-scale processes like aerosol activation. A turbulence and cloud parameterization, based on multi-variate probability density functions of sub-grid vertical velocity, temperature, and moisture, has been extended to treat aerosol activation. Multi-variate probability density functions with dynamics (MVD PDFs) offer a solution to the problem of the gap between the resolution of climate models and the scales relevant for aerosol activation and a means to overcome the limitations of diagnostic estimates of cloud droplet number concentration based only on aerosol concentration.
Incorporated into the single-column version of GFDL AM3, the MVD PDFs successfully simulate cloud properties including precipitation for cumulus, stratocumulus, and cumulus-under-stratocumulus. The extension to treat aerosol activation predicts droplet number concentrations in good agreement with large eddy simulations (LES). The droplet number concentrations from the MVD PDFs match LES results more closely than diagnostic relationships between aerosol concentration and droplet concentration.
In the single-column model simulations, as aerosol concentration increases, droplet concentration increases, precipitation decreases, but liquid water path can increase or decrease.
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M. Salzmann, Y. Ming, J.-C. Golaz, P. A. Ginoux, H. Morrisson, A. Gettelman, M. Krämer,
and L. J. Donner, 2010: Two-moment bulk stratiform cloud microphysics in the GFDL AM3
GCM: description, evaluation, and sensitivity tests.
Atmos. Chem. Phys., 10, 8037-8064,
doi: 10.5194/acp-10-8037-2010
(pdf, 3M)
Abstract
A new stratiform cloud scheme including a two-moment bulk microphysics module, a cloud cover parameterization allowing ice supersaturation, and an ice nucleation parameterization has been implemented into the recently developed GFDL AM3 general circulation model (GCM) as part of an effort to treat aerosol-cloud-radiation interactions more realistically. Unlike the original scheme, the new scheme facilitates the study of cloud-ice-aerosol interactions via influences of dust and sulfate on ice nucleation. While liquid and cloud ice water path associated with stratiform clouds are similar for the new and the original scheme, column integrated droplet numbers and global frequency distributions (PDFs) of droplet effective radii differ significantly. This difference is in part due to a difference in the implementation of the Wegener-Bergeron-Findeisen (WBF) mechanism, which leads to a larger contribution from super-cooled droplets in the original scheme. Clouds are more likely to be either completely glaciated or liquid due to the WBF mechanism in the new scheme. Super-saturations over ice simulated with the new scheme are in qualitative agreement with observations, and PDFs of ice numbers and effective radii appear reasonable in the light of observations. Especially, the temperature dependence of ice numbers qualitatively agrees with in-situ observations. The global average long-wave cloud forcing decreases in comparison to the original scheme as expected when super-saturation over ice is allowed. Anthropogenic aerosols lead to a larger decrease in short-wave absorption (SWABS) in the new model setup, but outgoing long-wave radiation (OLR) decreases as well, so that the net effect of including anthropogenic aerosols on the net radiation at the top of the atmosphere (netradTOA = SWABS-OLR) is of similar magnitude for the new and the original scheme.
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S. Xie, R. B. McCoy, S. A. Klein, R. T. Cederwall, W. J. Wiscombe, E. E. Clothiaux, K. L. Gaustad, J.-C. Golaz, S. D. Hall, M. P. Jensen, K. L. Johnson, Y. Lin, C. N. Long, J. H. Mather, R. A. McCord, S. A. McFarlane, G. Palanisamy, Y. Shi, and D. D. Turner, 2010:
CLOUDS AND MORE: ARM Climate Modeling Best Estimate Data.
Bull. Amer. Meteor. Soc.,
91, 1, 13-20, doi: 10.1175/2009BAMS2891.1.
(pdf, 4M)
Abstract
No Abstract available.
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Golaz, J.-C., J. D. Doyle and S. Wang, 2009:
One-way nested large-eddy simulation over the Askervein Hill.
J. Adv. Model. Earth Syst.,
1, 6, 1-6, doi: 10.3894/JAMES.2009.1.6.
(pdf, 418K)
Abstract
Large-eddy simulation (LES) models have been used extensively to study atmospheric boundary layer turbulence
over flat surfaces; however, LES applications over topography are less common. We evaluate the ability of
an existing model -- COAMPS(R)-LES -- to simulate flow over terrain using data from the Askervein Hill Project.
A new approach is suggested for the treatment of the lateral boundaries using one-way grid nesting. LES wind
profile and speed-up are compared with observations at various locations around the hill. The COAMPS-LES model
performs generally well. This case could serve as a useful benchmark for evaluating LES models for
applications over topography.
Additional files related to Askervein work:
- Electronic supplement (data, scripts, figures): data.tar.gz (1.4M)
- Askervein related files (terrain, observations): askervn.zip (523K; courtesy Wensong Weng)
- Askervein technical reports can be found here.
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Klein, S. A., R. B. McCoy, H. Morrison, A. S. Ackerman, A. Avramov, G. de Boer, M. Chen, J. N. S. Cole, A. D. Del Genio,
M. Falk, M. J. Foster, A. Fridlind, J.-C. Golaz, T. Hashino,
J. Y. Harrington, C. Hoose, M. F. Khairoutdinov, V. E. Larson,
X. Liu, Y. Luo, G. M. McFarquhar, S. Menon, R. A. J. Neggers,
S. Park, M. R. Poellot, J. M. Schmidt, I. Sednev, B. J. Shipway,
M. D. Shupe, D. A. Spangenberg, Y. C. Sud, D. D. Turner,
D. E. Veron, K. von Salzen, G. K. Walker, Z. Wang, A. B. Wolf, S. Xie, K.-M. Xu, F. Yang and G. Zhang, 2009:
Intercomparison of model simulations of mixed-phase clouds observed during
the ARM Mixed-Phase Arctic Cloud Experiment. Part I: Single layer cloud.
Quart. J. Roy. Meteor. Soc., 135, 979-1002.
(pdf, 652K;
doi: 10.1002/qj.416)
Abstract
Results are presented from an intercomparison of single-column and cloud-resolving model simulations
of a cold-air outbreak mixed-phase stratocumulus cloud observed during the Atmospheric Radiation
Measurement (ARM) programme's Mixed-Phase Arctic Cloud Experiment. The observed cloud occurred in a
well-mixed boundary layer with a cloud-top temperature of -15 C. The average liquid water path of around
160 g m-2 was about two-thirds of the adiabatic value and far greater than the average mass of ice which
when integrated from the surface to cloud top was around 15 g m-2 . Simulations of 17 single-column
models (SCMs) and 9 cloud-resolving models (CRMs) are compared. While the simulated ice water path is
generally consistent with observed values, the median SCM and CRM liquid water path is a factor-of-three
smaller than observed. Results from a sensitivity study in which models removed ice microphysics suggest
that in many models the interaction between liquid and ice-phase microphysics is responsible for the large
model underestimate o f liquid water path. Despite this underestimate, the simulated liquid and ice water
paths of several models are consistent with observed values. Furthermore, models with more sophisticated
microphysics simulate liquid and ice water paths that are in better agreement with the observed values,
although considerable scatter exists. Although no single factor guarantees a good simulation, these results
emphasize the need for improvement in the model representation of mixed-phase microphysics.
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Ackerman, A. S., M. C. vanZanten, B. Stevens, V. Savic-Jovcic, C. S. Bretherton, A. Chlond,
J.-C. Golaz, H. Jiang, M. Khairoutdinov, S. K. Krueger, D. C. Lewellen, A. Lock, C.-H. Moeng,
K. Nakamura, M. D. Petters, J. R. Snider, S. Weinbrecht, and M. Zulauf, 2009:
Large-eddy simulations of a drizzling, stratocumulus-topped marine boundary layer
Mon. Wea. Rev., 137, 1083-1110.
(pdf, 1.5M;
doi: 10.1175/2008MWR2582.1)
Abstract
Cloud water sedimentation and drizzle in a stratocumulus-topped boundary layer are the focus of an intercomparison of large-eddy simulations. The context is an idealized case study of nocturnal stratocumulus under a dry inversion, with embedded pockets of heavily drizzling open cellular convection. Results from 11 groups are used. Two models resolve the size distributions of cloud particles, and the others parameterize cloud water sedimentation and drizzle. For the ensemble of simulations with drizzle and cloud water sedimentation, the mean liquid water path (LWP) is remarkably steady and consistent with the measurements, the mean entrainment rate is at the low end of the measured range, and the ensemble-average maximum vertical wind variance is roughly half that measured. On average, precipitation at the surface and at cloud base is smaller, and the rate of precipitation evaporation greater, than measured. Including drizzle in the simulations reduces convective intensity, increases boundary layer stratification, and decreases LWP for nearly all models. Including cloud water sedimentation substantially decreases entrainment, decreases convective intensity, and increases LWP for most models. In nearly all cases, LWP responds more strongly to cloud water sedimentation than to drizzle. The omission of cloud water sedimentation in simulations is strongly discouraged, regardless of whether or not precipitation is present below cloud base.
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Haywood, J., L. Donner, A. Jones, and J.-C. Golaz, 2009:
Global indirect radiative forcing caused by aerosols: IPCC (2007) and beyond.
Clouds in the perturbed climate system: their relationship to energy balance, atmospheric dynamics, and precipitation.
J. Heintzenberg and R. J. Charlson, Eds., MIT Press, 451-467.
(pdf, 1.4M)
Abstract
Anthropogenic aerosols are thought to exert a significant indirect radiative forcing because they act as cloud condensation nuclei in warm cloud-forming processes and ice nuclei in cold cloud-forming processes. Although many of the processes associated with the perturbation of cloud microphysics by anthropogenic aerosols were discussed, IPCC (2007) provided only an estimate of full quantification of the radiative forcing attributable to the first indirect effect (which they referred to as the cloud albedo effect). Here we explain that this approach is necessary if one is to compare the radiative forcing from the indirect effect of aerosols with those from other radiative forcing components such as that from changes in well-mixed greenhouse gases. We also highlight the problems in assessing the effect of anthropogenic aerosols upon clouds under the strict definitions of radiative forcing provided by the IPCC (2007). Although results from global climate models, at their current state of development, suggest that an analysis of indirect aerosol effects in terms of forcing and feedback is possible, a key rationale for the IPCC's definition of radiative forcing, a straightforward scaling between an agent's forcing and the temperature change it induces, is significantly compromised. Feedbacks from other radiative forcings are responses to radiative perturbations, whereas feedbacks from indirect aerosol effects are responses to both radiative and cloud microphysical perturbations. This inherent difference in forcing mechanism breaks down the consistency between forcing and temperature response. It is likely that additional characterization, such as climate efficacy, will be required when comparing indirect aerosol effects with other radiative forcings. We suggest using the radiative flux perturbation associated with a change from preindustrial to present-day composition,
calculated in a global climate model using fixed sea surface temperature and sea ice, as a supplement to IPCC forcing.
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Wang, S., J.-C. Golaz and Q. Wang, 2008:
Effect of intense wind shear across the inversion on stratocumulus clouds
Geophys. Res. Lett.,
35, L15814, doi: 10.1029/2008GL033865.
(pdf, 231K)
Abstract
A large-eddy simulation model is used to examine the impact of the intense cross-inversion
wind shear on the stratocumulus cloud structure. The wind shear enhanced entrainment mixing
effectively reduces the cloud water and thickens the inversion layer. It leads to a reduction
of the turbulence kinetic energy (TKE) production in the cloud layer due to the weakened
cloud-top radiative cooling and the formation of a turbulent and cloud free sublayer within
the inversion. The thickness of the sublayer increases with the enhanced wind shear intensity.
Under the condition of a weaker inversion, the enhanced shear mixing within the inversion
layer even lowers the cloud-top height and reduces the entrainment velocity. Finally,
increasing wind shear or reducing inversion strength tends to create an inversion layer with
a constant bulk Richardson number (~0.3), suggesting that an equilibrium value of the Richardson
number is reached.
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Teixeira J., B. Stevens, C. S. Bretherton, R. Cederwall, J. D. Doyle, J.-C. Golaz,
A. A. M. Holtslag, S. A. Klein, J. K. Lundquist, D. A. Randall,
A. P. Siebesma, and P. M. M. Soares, 2008:
Parameterization of the atmospheric boundary layer: A view from just above the inversion
Bull. Amer. Meteor. Soc.,
89, 453-458.
(pdf, 655K;
doi: 10.1175/BAMS-89-4-453)
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Golaz, J.-C, V. E. Larson, J. A. Hansen, D. P. Schanen, and B. M. Griffin, 2007:
Elucidating model inadequacies in a cloud parameterization by use of an ensemble-based
calibration framework Mon. Wea. Rev.,
135, 4077-4096.
(pdf, 2.1M;
doi: 10.1175/2007MWR2008.1)
Abstract
Every cloud parameterization contains structural model errors. The source of these errors is
difficult to pinpoint because cloud parameterizations contain nonlinearities and feedbacks.
To elucidate these model inadequacies, this paper uses a general-purpose ensemble parameter
estimation technique. In principle, the technique is applicable to any parameterization that
contains a number of adjustable coefficients. It optimizes or calibrates parameter values by
attempting to match predicted fields to reference datasets. Rather than striving to find the
single best set of parameter values, the output is instead an ensemble of parameter sets. This
ensemble provides a wealth of information. In particular, it can help uncover model deficiencies
and structural errors that might not otherwise be easily revealed. The calibration technique
is applied to an existing single-column model (SCM) that parameterizes boundary layer clouds.
The SCM is a higher-order turbulence closure model. It is closed using a multivariate probability
density function (PDF) that represents subgrid-scale variability. Reference datasets are
provided by large-eddy simulations (LES) of a variety of cloudy boundary layers. The calibration
technique locates some model errors in the SCM. As a result, empirical modifications are
suggested. These modifications are evaluated with independent datasets and found to lead to an
overall improvement in the SCM's performance.
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Larson, V. E., A. J. Smith, M. J. Falk, K. E. Kotenberg, and J.-C. Golaz, 2006:
What determines altocumulus dissipation time? J. Geophys. Res.,
111, D19207, doi:10.1029/2005JD007002.
(pdf, 726K)
Abstract
This paper asks what factors influence the dissipation time of altocumulus clouds. The
question is addressed using three-dimensional, large-eddy simulations of a thin, midlevel
cloud that was observed by aircraft. The cloud might be aptly described as "altostratocumulus"
because it was overcast and contained radiatively driven turbulence. The simulations are used to
construct a budget equation of cloud water. This equation allows one to directly compare the
four processes that diminish liquid: diffusional growth of ice crystals, large-scale subsidence,
radiative heating, and turbulent mixing of dry air into the cloud. Various sensitivity studies
are used to find the "equivalent sensitivity" of cloud decay time to changes in various
parameters. A change from no sunlight to direct overhead sunlight decreases the lifetime of
our simulated cloud as much as increasing subsidence by 1.2 cm s-1, increasing ice number
concentration by 780 m-3, or decreasing above-cloud total water mixing ratio by 0.60 g kg-1.
Finally, interactions among the terms in the cloud water budget are summarized in a "budget
term feedback matrix." It is able to diagnose, for instance, that in our particular simulations,
the diffusional growth of ice is a negative feedback.
-
Beare, R. J., M. K. MacVean, A. A. M. Holtslag, J. Cuxart, I. Esau, J.-C.
Golaz, M. A. Jimenez, M. Khairoutdinov, B. Kosovic, D. Lewellen, T. S. Lund,
J. K. Lundquist, A. McCabe, A. F. Moene, Y. Noh, S. Raasch, and
P. Sullivan, 2006: An intercomparison of large-eddy simulations of the stable
boundary layer. Bound.-Layer Meteor., 118, 247-272.
(pdf, 657K;
doi: 10.1007/s10546-004-2820-6)
Abstract
Results are presented from the first intercomparison of large-eddy simulation
(LES) models for the stable boundary layer (SBL), as part of the Global Energy
and Water Cycle Experiment Atmospheric Boundary Layer Study initiative. A moderately
stable case is used, based on Arctic observations. All models produce successful
simulations, in as much as they generate resolved turbulence and reflect many of
the results from local scaling theory and observations. Simulations performed at
1-m and 2-m resolution show only small changes in the mean profiles compared to
coarser resolutions. Also, sensitivity to subgrid models for individual models
highlights their importance in SBL simulation at moderate resolution (6.25 m).
Stability functions are derived from the LES using typical mixing lengths used in
numerical weather prediction (NWP) and climate models. The functions have smaller
values than those used in NWP. There is also support for the use of K-profile
similarity in parametrizations. Thus, the results provide improved understanding
and motivate future developments of the parametrization of the SBL.
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Golaz, J.-C., S. Wang, J. D. Doyle, and J. M. Schmidt, 2005: COAMPS®
-LES: Model evaluation and analysis of second and third
moment vertical velocity budgets. Bound.-Layer Meteor., 116,
487-517.
(pdf, 975K;
doi: 10.1007/s10546-004-7300-5)
Abstract
The Naval Research Laboratory Coupled Ocean/Atmosphere Mesoscale Prediction
System (COAMPS®) has been extended to perform as a large-eddy simulation
(LES) model. It has been validated with a series of boundary-layer experiments
spanning a range of cloud nighttime, and includes a nighttime stratocumulus case,
a trade wind cumulus layer, shallow cumulus convection over land, and a mixed
regime consisting of cumulus clouds under broken stratocumulus. COAMPS-LES results
are in good agreement with other models for all the cases simulated. Exact numerical
budgets for the vertical velocity second (w'2) and third moment (w'3) have been
derived for the stratocumulus and trade wind cumulus cases. For the w'3 budget in
the stratocumulus, the buoyancy contribution from the updraughts and downdraughts
largely cancel each other due to their similar magnitudes but opposite signs.
In contrast, for the cumulus layer, the negative buoyancy contribution from the
environmental downdraughts is negligible and the positive contribution from the
updraughts completely dominates due to the conditional instability in the environment.
As a result, w'3 is significantly larger in the cumulus than in the stratocumulus layer.
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Larson, V. E., J.-C. Golaz, H. Jiang, and W. R. Cotton, 2005: Supplying local
microphysics parameterizations with information about subgrid variability:
Latin hypercube sampling. J. Atmos. Sci., 62, 4010-4026.
(pdf, 997K;
doi: 10.1175/JAS3624.1)
Abstract
One problem in computing cloud microphysical processes in coarse-resolution numerical
models is that many microphysical processes are nonlinear and small in scale.
Consequently, there are inaccuracies if microphysics parameterizations are forced
with grid box averages of model fields, such as liquid water content. Rather,
the model needs to determine information about subgrid variability and input it
into the microphysics parameterization. One possible solution is to assume the shape
of the family of probability density functions (PDFs) associated with a grid box and
sample it using the Monte Carlo method. In this method, the microphysics subroutine
is called repeatedly, once with each sample point. In this way, the Monte Carlo method
acts as an interface between the host model's dynamics and the microphysical
parameterization. This avoids the need to rewrite the microphysics subroutines.
A difficulty with the Monte Carlo method is that it introduces into the simulation
statistical noise or variance, associated with the finite sample size. If the family
of PDFs is tractable, one can sample solely from cloud, thereby improving estimates
of in-cloud processes. If one wishes to mitigate the noise further, one needs a
method for reduction of variance. One such method is Latin hypercube sampling, which
reduces noise by spreading out the sample points in a quasi-random fashion. This
paper formulates a sampling interface based on the Latin hypercube method. The
associated family of PDFs is assumed to be a joint normal/lognormal
(i.e., Gaussian/lognormal) mixture. This method of variance reduction has a
couple of advantages. First, the method is general: the same interface can be
used with a wide variety of microphysical parameterizations for various processes.
Second, the method is flexible: one can arbitrarily specify the number of hydrometeor
categories and the number of calls to the microphysics parameterization per grid box
per time step. This paper performs a preliminary test of Latin hypercube sampling.
As a prototypical microphysical formula, this paper uses the Kessler autoconversion
formula. The PDFs that are sampled are extracted diagnostically from large-eddy
simulations (LES). Both stratocumulus and cumulus boundary layer cases are tested.
In this diagnostic test, the Latin hypercube can produce somewhat less noisy
time-averaged estimates of Kessler autoconversion than a traditional Monte Carlo
estimate, with no additional calls to the microphysics parameterization. However,
the instantaneous estimates are no less noisy. This paper leaves unanswered the
question of whether the Latin hypercube method will work well in a prognostic,
interactive cloud model, but this question will be addressed in a future manuscript.
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Larson, V. E. and J.-C. Golaz, 2005: Using probability density functions to
derive consistent closure relationships among higher-order moments. Mon.
Wea. Rev., 133, 1023-1042.
(pdf, 621K;
doi: 10.1175/MWR2902.1)
Abstract
Parameterizations of turbulence often predict several lower-order moments
and make closure assumptions for higher-order moments. In principle, the low-
and high-order moments share the same probability density function (PDF). One
closure assumption, then, is the shape of this family of PDFs. When the higher-order
moments involve both velocity and thermodynamic scalars, often the PDF shape has
been assumed to be a double or triple delta function. This is equivalent to
assuming a mass-flux model with no subplume variability. However, PDF families
other than delta functions can be assumed. This is because the assumed PDF
methodology is fairly general. This paper proposes closures for several third-
and fourth-order moments. To derive the closures, the moments are assumed to
be consistent with a particular PDF family, namely, a mixture of two trivariate
Gaussians. (This PDF is also called a double Gaussian or binormal PDF by some
authors.) Separately from the PDF assumption, the paper also proposes a simplified
relationship between scalar and velocity skewnesses. This PDF family and skewness
relationship are simple enough to yield simple, analytic closure formulas relating
the moments. If certain conditions hold, this set of moments is specifically realizable.
By this it is meant that the set of moments corresponds to a real Gaussian-mixture
PDF, one that is normalized and nonnegative everywhere. This paper compares the
new closure formulas with both large eddy simulations (LESs) and closures based
on double and triple delta PDFs. This paper does not implement the closures in
a single-column model and test them interactively. Rather, the comparisons are
diagnostic; that is, low-order moments are extracted from the LES and treated
as givens that are input into the closures. This isolates errors in the closures
from errors in a single-column model. The test cases are three atmospheric boundary
layers: a trade wind cumulus layer, a stratocumulus layer, and a clear convective
case. The new closures have shortcomings, but nevertheless are superior to the double
or triple delta closures in most of the cases tested.
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Stevens, B., C.-H. Moeng, A. S. Ackerman, C. S. Bretherton, A. Chlond,
S. de Roode, J. Edwards, J.-C. Golaz, H. Jiang, M. Khairoutdinov, M. P.
Kirkpatrick, D. C. Lewellen, A. Lock, F. Müller, D. E. Stevens,
E. Whelan, and P. Zhu, 2005: Evaluation of large-eddy simulations via
observations of nocturnal marine stratocumulus. Mon. Wea. Rev., 133, 1443-1462.
(pdf, 869K;
doi: 10.1175/MWR2930.1)
Abstract
Data from the first research flight (RF01) of the second Dynamics and Chemistry
of Marine Stratocumulus (DYCOMS-II) field study are used to evaluate the fidelity
with which large-eddy simulations (LESs) can represent the turbulent structure of
stratocumulus-topped boundary layers. The initial data and forcings for this case
placed it in an interesting part of parameter space, near the boundary where
cloud-top mixing is thought to render the cloud layer unstable on the one hand, or
tending toward a decoupled structure on the other hand. The basis of this evaluation
consists of sixteen 4-h simulations from 10 modeling centers over grids whose vertical
spacing was 5 m at the cloud-top interface and whose horizontal spacing was 35 m.
Extensive sensitivity studies of both the configuration of the case and the numerical
setup also enhanced the analysis. Overall it was found that (i) if efforts are made
to reduce spurious mixing at cloud top, either by refining the vertical grid or limiting
the effects of the subgrid model in this region, then the observed turbulent and
thermodynamic structure of the layer can be reproduced with some fidelity; (ii)
the base, or native configuration of most simulations greatly overestimated mixing
at cloud top, tending toward a decoupled layer in which cloud liquid water path and
turbulent intensities were grossly underestimated; (iii) the sensitivity of the
simulations to the representation of mixing at cloud top is, to a certain extent,
amplified by particulars of this case. Overall the results suggest that the use of
LESs to map out the behavior of the stratocumulus-topped boundary layer in this
interesting region of parameter space requires a more compelling representation
of processes at cloud top. In the absence of significant leaps in the understanding
of subgrid-scale (SGS) physics, such a representation can only be achieved by a
significant refinement in resolution--a refinement that, while conceivable given
existing resources, is probably still beyond the reach of most centers.
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Zhu, P., C. S. Bretherton, M. Köhler, A. Cheng, A. Chlond, Q.Geng,
P. Austin, J.-C. Golaz, G. Lenderink, A. Lock, and B. Stevens, 2005:
Intercomparison and interpretation of single-column model simulations of a
nocturnal stratocumulus-topped marine boundary layer. Mon. Wea. Rev.,
133, 2741-2758.
(pdf, 1.3M;
doi: 10.1175/MWR2997.1)
Abstract
Ten single-column models (SCMs) from eight groups are used to simulate a nocturnal
nonprecipitating marine stratocumulus-topped mixed layer as part of an intercomparison
organized by the Global Energy and Water Cycle Experiment Cloud System Study, Working
Group 1. The case is idealized from observations from the Dynamics and Chemistry of
Marine Stratocumulus II, Research Flight 1. SCM simulations with operational resolution
are supplemented by high-resolution simulations and compared with observations and
large-eddy simulations. All participating SCMs are able to maintain a sharp inversion
and a mixed cloud-topped layer, although the moisture profiles show a slight gradient
in the mixed layer and produce entrainment rates broadly consistent with observations,
but the liquid water paths vary by a factor of 10 after only 1 h of simulation at both
high and operational resolution. Sensitivity tests show insensitivity to activation of
precipitation and shallow convection schemes in most models, as one would observationally
expect for this case.
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Cheng, A., K.-M. Xu, and J.-C. Golaz, 2004: The liquid water oscillation in
modeling boundary layer cumuli with third-order turbulence closure models.
J. Atmos. Sci., 61, 1621-1629.
(pdf, 778K;
doi: 10.1175/1520-0469(2004)061<1621:tlwoim>2.0.CO;2)
Abstract
A hierarchy of third-order turbulence closure models are used to simulate boundary
layer cumuli in this study. An unrealistically strong liquid water oscillation (LWO)
is found in the fully prognostic model, which predicts all third moments. The LWO
propagates from cloud base to cloud top with a speed of 1 m s-1. The period of the
oscillation is about 1000 s. Liquid water buoyancy (LWB) terms in the third-moment
equations contribute to the LWO. The LWO mainly affects the vertical profiles of cloud
fraction, mean liquid water mixing ratio, and the fluxes of liquid water potential
temperature and total water, but has less impact on the vertical profiles of other
second and third moments. In order to minimize the LWO, a moderately large diffusion
coefficient and a large turbulent dissipation at its originating level are needed.
However, this approach distorts the vertical distributions of cloud fraction and
liquid water mixing ratio. A better approach is to parameterize LWB more reasonably.
A minimally prognostic model, which diagnoses all third moments except for the vertical
velocity, is shown to produce better results, compared to a fully prognostic model.
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Larson, V. E., J.-C. Golaz, and W. R. Cotton, 2002: Small-scale and mesoscale
variability in cloudy boundary layers: Joint probability density functions.
J. Atmos. Sci., 59, 3519-3539.
(pdf, 574K;
doi: 10.1175/1520-0469(2002)059<3519:ssamvi>2.0.CO;2)
Abstract
The joint probability density function (PDF) of vertical velocity and conserved
scalars is important for at least two reasons. First, the shape of the joint PDF
determines the buoyancy flux in partly cloudy layers. Second, the PDF provides a
wealth of information about subgrid variability and hence can serve as the foundation
of a boundary layer cloud and turbulence parameterization. This paper analyzes PDFs
of stratocumulus, cumulus, and clear boundar y layers obtained from both aircraft
observations and large eddy simulations. The data are used to fit five families of
PDFs: a double delta function, a single Gaussian, and three PDF families based on
the sum of two Gaussians. Overall, the double Gaussian, that is binormal, PDFs
perform better than the single Gaussian or double delta function PDFs. In cumulus
layers with low cloud fraction, the improvement occurs because typical PDFs are
highly skewed, and it is crucial to accurately represent the tail of the distribution,
which is where cloud occurs. Since the double delta function has been shown in
prior work to be the PDF underlying mass-flux schemes, the data analysis herein
hints that mass-flux simulations may be improved upon by using a parameterization
built upon a more realistic PDF.
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Golaz, J.-C., V. E. Larson, and W. R. Cotton, 2002a: A PDF based
model for boundary layer clouds. Part I: Method and model description.
J. Atmos. Sci., 59, 3540-3551.
(pdf, 195K;
doi: 10.1175/1520-0469(2002)059<3540:apbmfb>2.0.CO;2)
Abstract
A new cloudy boundary layer single-column model is presented. It is designed
to be flexible enough to represent a variety of cloudiness regimes--such as cumulus,
stratocumulus, and clear regimes--without the need for case-specific adjustments.
The methodology behind the model is the so-called assumed probability density function
(PDF) method. The parameterization differs from higher-order closure or mass-flux schemes
in that it achieves closure by the use of a relatively sophisticated joint PDF of
vertical velocity, temperature, and moisture. A family of PDFs is chosen that is
flexible enough to represent various cloudiness regimes. A double Gaussian family
proposed by previous works is used. Predictive equations for grid box means and a number
of higherorder turbulent moments are advanced in time. These moments are in turn used to
select a particular member from the family of PDFs, for each time step and grid box. Once
a PDF member has been selected, the scheme integrates over the PDF to close higher-order
moments, buoyancy terms, and diagnose cloud fraction and liquid water. Since all the
diagnosed moments for a given grid box and time step are derived from the same unique joint
PDF, they are guaranteed to be consistent with one another. A companion paper presents
simulations produced by the single-column model.
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Golaz, J.-C., V. E. Larson, and W. R. Cotton, 2002b: A PDF based
model for boundary layer clouds. Part II: Model results. J. Atmos.
Sci., 59, 3552-3571.
(pdf, 662K;
doi: 10.1175/1520-0469(2002)059<3552:apbmfb>2.0.CO;2)
Abstract
A new single-column model for the cloudy boundary layer, described in a companion
paper, is tested for a variety of regimes. To represent the subgrid-scale variability,
the model uses a joint probability density function (PDF) of vertical velocity, temperature,
and moisture content. Results from four different cases are presented and contrasted with
large eddy simulations (LES). The cases include a clear convective layer based on the
Wangara experiment, a trade wind cumulus layer from the Barbados Oceanographic and
Meteorological Experiment (BOMEX), a case of cumulus clouds over land, and a nocturnal
marine stratocumulus boundary layer. Results from the Wangara experiment show that the
model is capable of realistically predicting the diurnal growth of a dry convective
layer. Compared to the LES, the layer produced is slightly less well mixed and
entrainment is somewhat slower. The cloud cover in the cloudy cases varied widely,
ranging from a few percent cloud cover to nearly overcast. In each of the cloudy cases,
the parameterization predicted cloud fractions that agree reasonably well with the LES.
Typically, cloud fraction values tended to be somewhat smaller in the parameterization,
and cloud bases and tops were slightly underestimated. Liquid water content was generally
within 40% of the LES-predicted values for a range of values spanning almost two orders
of magnitude. This was accomplished without the use of any case-specific adjustments.
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Brown, A. R., R. T. Cederwall, A. Chlond, P. G. Duynkerke, J.-C. Golaz,
M. Khairoutdinov, D. C. Lewellen, A. P. Lock, M. K. MacVean, C.-H. Moeng,
R. A. J. Neggers, A. P. Siebesma, and B. Stevens, 2002: Large-eddy simulation
of the diurnal cycle of shallow cumulus convection over land. Quart. J.
Roy. Meteor. Soc., 128, 1075-1093.
(pdf, 601K;
doi: 10.1256/003590002320373210)
Abstract
Large-eddy simulations of the development of shallow cumulus convection over land
are presented. Many characteristics of the cumulus layer previously found in simulations
of quasi-steady convection over the sea are found to be reproduced in this more strongly
forced, unsteady case. Furthermore, the results are shown to be encouragingly robust,
with similar results obtained with eight independent models, and also across a range
of numerical resolutions. The datasets produced are already being used in the
development and evaluation of parametrizations used in numerical weather-prediction
and climate models .
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Golaz, J.-C., H. Jiang, and W. R. Cotton, 2001: A large-eddy simulation study
of cumulus clouds over land and sensitivity to soil moisture. Atmos.
Res., 59-60, 373-392.
(pdf, 275K;
doi: 10.1016/S0169-8095(01)00113-2)
Abstract
A series of large-eddy simulations (LES) of non-precipitating cumulus clouds
over land was performed. These simulations were idealized from observed conditions
at the Southern Great Plains ARM site on 21 June 1997 and were intended to investigate
the effect of initial soil moisture on the structure of the cloudy boundary layer. The
surface fluxes were either dominated by latent heat or sensible heat flux, with the
transition between one regime and the other occurring over a very narrow soil moisture
range. The effect on clouds was mixed. Cloud fraction was nearly identical throughout
all experiments. Simulations with dominant sensible heat fluxes led to more turbulent
boundary layers and higher cloud bases. Simulations dominated by latent heat flux tended
to have fewer but stronger updrafts in the cloud layer.
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Larson, V. E., R. Wood, P. R. Field, J.-C. Golaz, T. H. Vonder Haar, and
W. R. Cotton, 2001a: Systematic biases in the microphysics and thermodynamics
of numerical models that ignore subgrid-scale variability. J. Atmos.
Sci., 58, 1117-1128.
(pdf, 184K;
doi: 10.1175/1520-0469(2001)058<1117:sbitma>2.0.CO;2)
Abstract
A grid box in a numerical model that ignores subgrid variability has biases in certain
microphysical and thermodynamic quantities relative to the values that would be obtained
if subgrid-scale variability were taken into account. The biases are important because
they are systematic and hence have cumulative effects. Several types of biases are
discussed in this paper. Namely, numerical models that employ convex autoconversion
formulas underpredict (or, more precisely, never overpredict) autoconversion rates,
and numerical models that use convex functions to diagnose specific liquid water content
and temperature underpredict these latter quantities. One may call these biases the
"grid box average autoconversion bias," "grid box average liquid water content bias,
" and "grid box average temperature bias," respectively, because the biases arise when
grid box average values are substituted into formulas valid at a point, not over an extended
volume. The existence of these biases can be derived from Jensen's inequality. To assess
the magnitude of the biases, the authors analyze observations of boundary layer clouds.
Often the biases are small, but the observations demonstrate that the biases can be large
in important cases. In addition, the authors prove that the average liquid water content
and temperature of an isolated, partly cloudy, constant-pressure volume of air cannot increase,
even temporarily. The proof assumes that liquid water content can be written as a convex
function of conserved variables with equal diffusivities. The temperature decrease is due
to evaporative cooling as cloudy and clear air mix. More generally, the authors prove that
if an isolated volume of fluid contains conserved scalars with equal diffusivities, then
the average of any convex, twice-differentiable function of the conserved scalars cannot increase.
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Larson, V. E., R. Wood, P. R. Field, J.-C. Golaz, T. H. Vonder Haar, and
W. R. Cotton, 2001b: Small-scale and mesoscale variability of scalars in
cloudy boundary layers: One-dimensional probability density functions. J. Atmos. Sci., 58, 1978-1994.
(pdf, 279K;
doi: 10.1175/1520-0469(2001)058<1978:ssamvo>2.0.CO;2)
Abstract
A key to parameterization of subgrid-scale processes is the probability density function
(PDF) of conserved scalars. If the appropriate PDF is known, then grid box average cloud
fraction, liquid water content, temperature, and autoconversion can be diagnosed. Despite
the fundamental role of PDFs in parameterization, there have been few observational studies
of conserved-scalar PDFs in clouds. The present work analyzes PDFs from boundary layers
containing stratocumulus, cumulus, and cumulus-rising-into-stratocumulus clouds. Using
observational aircraft data, the authors test eight different parameterizations of PDFs,
including double delta function, gamma function, Gaussian, and double Gaussian shapes.
The Gaussian parameterization, which depends on two parameters, fits most observed PDFs
well but fails for large-scale PDFs of cumulus legs. In contrast, three-parameter
parameterizations appear to be sufficiently general to model PDFs from a variety of
cloudy boundary layers. If a numerical model ignores subgrid variability, the model has
biases in diagnoses of grid box average liquid water content, temperature, and Kessler
autoconversion, relative to the values it would obtain if subgrid variability were taken
into account. The magnitude of such biases is assessed using obser vational data. The
biases can be largely eliminated by three-parameter PDF parameterizations. Prior authors
have suggested that boundary layer PDFs from short segments are approximately Gaussian.
The present authors find that the hypothesis that PDFs of total specific water content
are Gaussian can almost always be rejected for segments as small as 1 km.
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Galli, G., F. Gygi, and J.-C. Golaz, 1998: Vibrational and electronic
properties of neutral and negatively charged C20
clusters. Physical Review B, 57, 1860-1867.
(pdf, 161K;
doi: 10.1103/PhysRevB.57.1860)
Abstract
We computed vibrational and electronic properties of the cage, bowl, and ring isomers of neutral and
negatively charged C20 , within density-functional theory, using fully optimized local-density and gradient-corrected
geometries. Vibrational and electronic spectra exhibit distinctive features, which could be used to
identify a given isomer and its charge state in molecular beams or thin films. Notable changes are observed in
both the Raman and infrared spectra when going from the neutral to the charged isomers. We also calculated
vibrational entropies from harmonic frequencies. Our results indicate that, above a critical temperature, the ring
isomer is always stabilized by entropic effects, irrespective of the theoretical model used to compute the
internal energy. In particular, gradient-corrected functionals predict both the neutral and charged ring to be the
most stable isomer at all temperatures. Molecular-dynamics simulations were performed to study the geometry
of the ring at high temperature. Furthermore, we rationalized photoelectron spectra of C2n clusters, n59 –12,
in terms of differences in the electronic structure for even and odd n.