Strategies for Cumulus Parameterization for CESM3 and Beyond€¦ · parameterization development...

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Strategies for Cumulus Parameterization for CESM3 and Beyond Leo Donner GFDL/NOAA, Princeton University AMWG, 27 February 2017

Transcript of Strategies for Cumulus Parameterization for CESM3 and Beyond€¦ · parameterization development...

Page 1: Strategies for Cumulus Parameterization for CESM3 and Beyond€¦ · parameterization development process • Compensating errors easily introduced • Since many aspects of the parameterizations

Strategies for Cumulus Parameterization for CESM3 and

Beyond

Leo DonnerGFDL/NOAA, Princeton University

AMWG, 27 February 2017

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Introduction

• Cumulus parameterization has evolved very slowly through successive generations of CCSM and CESM

• Cumulus convection and related cloud processes likely play key roles in climate forcing and sensitivity

• With CESM2 completion, parameterization of deep convection stands out as major atmospheric physical process without major advances

• Likelihood of breakthroughs on decades-old questions in climate science limited by uncertainties in modeling deep convection in climate models

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From Forster et al. in Journal of Geophysical Research: AtmospheresVolume 118, Issue 3, pages 1139-1150, 6 FEB 2013 DOI: 10.1002/jgrd.50174http://onlinelibrary.wiley.com/doi/10.1002/jgrd.50174/full#jgrd50174-fig-0007

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Convection-deep and shallow-is a highly uncertain player in climate

forcing by aerosol-cloud interactions. Droplet and ice activation depend on updraft velocities, not even a part of

CESM2’s current deep parameterization.

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from Donner et al. (2016, ACP)

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Aerosol SensitivityIn order to study the sensitivity of ice number density (Ni) resulting from

homogeneous freezing to aerosol concentration (Na), an aerosol sensitivity parameter (ηα) was defined, following Kay and Wood 2008.

Ni (cm-3) contoured as a function of updraft velocity (V) and aerosol

concentration (Na).Colors indicate the aerosol sensitivity parameter (ηα).

Kay and Wood (2008, Geophys. Res. Lett.)

ra_dry= 0.2 μm (mono-disperse) αi (deposition coefficient)=0.1;

T0= -50oC, P0=250 hPa;

Slide courtesy of Xiaohong Liu, U. Wyoming

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Entrainment and microphysics in convection are major controls on sensitivity in climate models.

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Change in Cloud-Radiative Effect, Normalized by Energy-Balance Change

Dependence of Climate Sensitivity on Convective Entrainment (Zhao, 2014, J. Climate)

Climate SensitivityIncreasing Entrainment for

fixed precipitation threshold, except for Exp. 2

Climate sensitivity dependence on entrainment also shown by Stainforth et al. (2005, Nature), Sanderson et al. (2010, Clim. Dyn.), and for shallow but not deep convection, Klocke et al. (2011, J. Climate).

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Multi-Scale Convection: ISS over Libya, 8 September 2014, photo by Alex Gerst

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Should We Consider a New Strategy for Cumulus Parameterization in CESM3?

• “Individual-centric” efforts have dominated, e.g., Zhang and McFarlane (1995, Atmos.-Ocean), Wu et al. (2007, J. Atmos. Sci.)-CCSM4, Park (2014, J. Atmos. Sci.)-CESM2

• Efforts with new perspectives and major research commitment but parameterizations ultimately not adopted

• High-stakes, “winner-take-all” aspect despite efforts by modeling leadership, frustrating and discouraging to developers and potential developers

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Should We Consider a New Strategy for Cumulus Parameterization in CESM3?

• “Individual-centric” parameterizations have almost inevitably necessitated a limited view as to which aspects of the problem are most critical

• Commitments to these choices required very early in parameterization development process

• Compensating errors easily introduced• Since many aspects of the parameterizations are not

robustly tied to physical understanding or process-level models or observations, cumulus parameterizations are tuning targets to compensate for problematic formulations elsewhere in the model.

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A “Community” Approach to Cumulus Parameterizaton

• “Team” approach, with strong emphasis on physical robustness, based on process models and observations

• Foundational problems, including stochastic aspects, convective microphysics, convective vertical velocities, convective organization, scale awareness, closures (likely prognostic), addressed at outset.

• Draw on broad community to address foundational problems, including those outside of model development per se

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A “Community” Approach to Cumulus Parameterization

• When robust solutions are identified, concerted effort to “lock them in”

• When multiple approaches available, attempt to discern among them at early stage

• CESM a process integrator to be used as frequent tool in development process

• Flexibility essential, development process not likely to follow smooth linear path, with issues likely to be revisited

• Multiple approaches could be advantageous, e.g., MMFs or early-stage global “CRMs”

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Next Steps?

• Consider a workshop to refine strategy• Explore prospects for support across communities

representing microscale, mesoscale, and earth-system modeling communities

• Probe obvious early questions, e.g., based on single-column and process models, is a vertically local (assumed distribution, higher-order closure) like CLUBB more suitable than an approach based on vertically integrating plume structures?

• Implications well beyond CESM

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Supplemental Slides-The Example of Convective

Vertical Velocities

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ConvectiveVertical

Velocities from GFDL

AM3 (Donner et al., 2011) and TWP ICE dual-Doppler

(Collis et al., 2013, J.

Appl. Meteor.

Climatol.)

Shading shows ranges of radar observations

with lower cut-off from 0.5 to

2.0 m s-1 over 5-km layer. 95th

percentile by extrapolating

AM3 ensembles ~ 1 m s-1 for

GATE, 1.5 m s-1

for TWP ICE 1/19-22, and 2.0

m s-1 for TWP ICE 1.23.

Analysis by Will Cooke, GFDL; GATE observations provided by Ian Glenn, U. Utah.

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TWP-ICE PDFs of Cumulus Vertical Velocity in GFDL AM3 and Radar Observations: Prospects for Sub-Grid Parameterization

PDFs of cumulus vertical velocities at TWP-ICE from GFDL AM3 (Donner et al. (2011, J. Climate) and dual-Doppler radar (Collis et

al., 2013, J. Appl. Meteor. Climatol.) show AM3 vertical velocity values often, but not always, larger than observed. Analysis by

Will Cooke, GFDL.

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MC3E PDFs of Cumulus Vertical Velocity in GFDL AM3 and Radar Observations

PDFs of cumulus vertical velocities at MC3E from GFDL AM3 (Donner et al. (2011, J. Climate) and dual-Doppler radar (Collis et

al., 2013, J. Appl. Meteor. Climatol.) show AM3 vertical velocity values often, but not always, larger than observed. Analysis by

Will Cooke, GFDL.

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Figure 9: Median profiles of maximum vertical velocity (a,c) and radar reflectivity (b,d) for three-dimensionally definedconvective updrafts beginning below 1 km and ending above 15 km for the period of 1310Z to 1750Z on 23 January 2006.

CRM statistics are shown in (a-b) and LAM statistics are shown in (c-d). Gray lines with symbols and the dashed black linesrepresent simulations. Observations are represented by solid black lines.

©2014 American Geophysical Union. All rights reserved.

Observed (Solid Black) & CRM Vertical Velocities (Varble et al., 2014, JGR)

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Improving representation of convective transport for scale‐aware parameterization: 1. Convection and cloud properties simulated with spectral bin and bulk microphysics

Journal of Geophysical Research: Atmospheres2014JD022142, 29 APR 2015 DOI: 10.1002/2014JD022142

http://onlinelibrary.wiley.com/doi/10.1002/2014JD022142/full#jgrd52099-fig-0009

TWP-ICE, 22 Jan 2006 SBM: spectral microphysics

MOR, MY2: bulk microphysics (from Fan

et al., 2015, JGR-Atmos.)

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Improving representation of convective transport for scale‐aware parameterization: 1. Convection and cloud properties simulated with spectral bin and bulk microphysics

Journal of Geophysical Research: Atmospheres2014JD022142, 29 APR 2015 DOI: 10.1002/2014JD022142

http://onlinelibrary.wiley.com/doi/10.1002/2014JD022142/full#jgrd52099-fig-0008

MC3E, 20 May 2011SBM: spectral

microphysics; MOR, MY2: bulk

microphysics (from Fan et al., 2015,

JGR-Atmos.)

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Improving representation of convective transport for scale‐aware parameterization: 1. Convection and cloud properties simulated with spectral bin and bulk microphysics

Journal of Geophysical Research: Atmospheres2014JD022142, 29 APR 2015 DOI: 10.1002/2014JD022142

http://onlinelibrary.wiley.com/doi/10.1002/2014JD022142/full#jgrd52099-fig-0007

MC3E, 23 May 2011, SBM: spectral bin

microphysics; MOR and MY2: bulk

microphysics, from Fan et al. (2015, JGR-

Atmos.)

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A simplified PDF parameterization of subgrid‐scale clouds and turbulence for cloud‐resolving models (horizontal resolution 3.2 km)

Journal of Advances in Modeling Earth SystemsVolume 5, Issue 2, pages 195-211, 18 APR 2013 DOI: 10.1002/jame.20018

http://onlinelibrary.wiley.com/doi/10.1002/jame.20018/full#jame20018-fig-0003 Bogenschutz and Krueger (2013)

Local turbulence

unsuccessful even at 40m

vertical resolution.

Higher-order, assumed

distribution turbulence

approaches LES even at 200m

vertical resolution.

BOMEXLES

Horizontal resolution: 100mVertical resolution: 40m

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Supplemental Slides on Convective Entrainment and

Climate Sensitivity

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From Stainforth et al. (2005, Nature)

Parameteric Control on Simulations without Cloud-Aerosol Interactions

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from Stainforth et al. (2005, Nature) Blue: No Entrainment VariationRed: No Autoconversion Variation

Global-mean temperature increase due to CO2 doubling

Entrainment is strong control on climate sensitivity. Vertical velocities depend strongly on entrainment.

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Source: Sanderson et al. (2010, Climate Dynamics, pp. 1219-1236)