An overview of recent activities at the Global Modeling and - - PowerPoint PPT Presentation

an overview of recent activities at the global modeling
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An overview of recent activities at the Global Modeling and - - PowerPoint PPT Presentation

National Aeronautics and Space Administration Global Modeling and Assimilation Office An overview of recent activities at the Global Modeling and Assimilation Office with focus on the stratosphere K. Wargan, L. Coy, S. Pawson, A. Molod, R.


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National Aeronautics and Space Administration gmao.gsfc.nasa.gov ¡

Global Modeling and Assimilation Office

An overview of recent activities at the Global Modeling and Assimilation Office with focus on the stratosphere

  • K. Wargan, L. Coy, S. Pawson, A. Molod, R. Gelaro,
  • R. Todling, L. Takacs, C. Orbe, A. El Akkraoui, G. Partyka

&

The GMAO team

¡

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National Aeronautics and Space Administration gmao.gsfc.nasa.gov ¡

Outline

  • Status of MERRA-2 validation
  • QBO ‘reboot’ in 2016
  • Towards full stratospheric chemistry
  • Replay and downscaling experiments
  • AMIP simulations
  • Transition to 4D-EnVar!!!
  • Other ongoing developments

This talk focuses on the stratosphere. There is much more going on at GMAO: weather, tropospheric chemistry, land, ocean…

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Status of MERRA-2 validation: core publications

MERRA-2 overview paper Gelaro et al. 2016: The Modern-Era Retrospective Analysis for Research and Applications, Version-2 (MERRA-2); to be submitted to J. Clim. This week MERRA-2 ozone validation paper Wargan et al., 2016: Evaluation of the Ozone Fields in NASA's MERRA-2 Reanalysis, submitted to J. Clim. MERRA-2 QBO paper Coy et al., 2016: Structure and dynamics of the quasi-biennial oscillation as seen in MERRA-2, J. Clim Tech memos Bosilovich, M. G., et al. 2015: MERRA-2: Initial evaluation of the climate, NASA Tech. Rep. series on global modeling and data assimilation, NASA/TM-2015-104606, vol. 39, 136 pp., NASA. [Available at http:// gmao.gsfc.nasa.gov/pubs/tm/docs/Bosilovich803.pdf.] McCarty et al. 2016: MERRA-2 Input Observations: Summary and Assessment, NASA/TM–2016-104606/Vol. 46 . Finished and ready for processing

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Status of MERRA-2 validation: the stratosphere & mesosphere

MERRA-2 Global Temperature Anomalies

1980 1985 1990 1995 2000 2005 2010 2015 1000 100 10 1 0.1 Pressure (hPa)

Averaging Period

  • 4.5 -4 -3.5 -3 -2.5 -2 -1.5 -1 -0.5 0.5

1 1.5 2 2.5 3 3.5 4 4.5 T (K)

Gelaro ¡et ¡al., ¡2016 ¡ AMSU-­‑A ¡ MLS ¡ Pressure ¡[hPa] ¡

Some cooling, no obvious discontinuities in the lower stratosphere El Chichon and Mt. Pinatubo signal The largest impact of the

  • bserving system changes: in the

upper stratosphere and mesosphere

  • Introduction of ATOVS AMSU-A
  • Introduction of MLS (p<5 hPa)

El ¡Chichon ¡

  • Mt. ¡Pinatubo ¡
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National Aeronautics and Space Administration gmao.gsfc.nasa.gov ¡

Status of MERRA-2 validation: the stratosphere & mesosphere

Gelaro ¡et ¡al., ¡2016 ¡

Evolution of polar temperatures during the 2005-2006 Northern Hemisphere winter

  • Disappearance of the warm polar

stratopause during the major SSW

  • Reformation at a higher altitude and

slow descent These features are captured more realistically in MERRA-2 compared to MERRA that did not use MLS

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Status of MERRA-2 validation: the stratosphere & mesosphere

Globally averaged temperature at 10 hPa MERRA-2 uses CRTM to assimilate SSU; cell pressure leaks are taken into account. The two reanalyses converge once more data become assimilated: AMSU, AIRS

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MEAN ¡30°N-­‑60°N ¡ DIFFERENCE ¡St. ¡Dev. ¡ MIPAS ¡MERRA ¡MERRA-­‑2 ¡

DJF ¡ MAM ¡ JJA ¡ SON ¡

MIPAS - MERRA-2

  • correlations. Bold line: 0.7

MERRA did not assimilate Aura data Seasonal cycle at 40 hPa captured by both MERRA and MERRA-2 but MERRA-2 has smaller bias Large improvement in the MERRA-2 – MIPAS st. deviations during the Aura period

Aura ¡period ¡ SBUV ¡ period ¡

Status of MERRA-2 validation: ozone

ppmv ppmv

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MERRA-2 is in better agreement with the radiosondes at 50 hPa. Note that the sonde data are assimilated in both reanalyses

Sondes ¡(gray ¡shading) ¡MERRA ¡MERRA-­‑2 ¡

Zonal wind at Singapore

Coy ¡ ¡et ¡al., ¡2016: ¡ ¡J. ¡Clim. ¡

Status of MERRA-2 validation: the QBO

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Coy ¡et ¡al., ¡2016 ¡

Nairobi ¡sondes ¡ ¡MERRA ¡ ¡MERRA-­‑2 ¡

MERRA ¡minus ¡sondes ¡ ¡ MERRA-­‑2 ¡minus ¡sondes ¡ ¡

SBUV ¡ ¡ assimilated ¡ MLS ¡ assimilated ¡

SBUV ¡period ¡ Aura ¡period ¡

In the Aura period tropical ozone is

  • Consistent with the zonal wind
  • In agreement with ozonesondes

Large vertical smoothing errors in SBUV obscure the phase propagation [Kramarova et al., 2013] In the Aura period in MERRA-2 the QBO signal in ozone shows more realistic phase propagation

Status of MERRA-2 validation: the QBO

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MERRA-2

a

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5

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5

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5 5 5 5 5 15

100 10 Pressure (hPa) 2015 2016

Composite

b

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5 5

20 25 30 35 Pressure Altitude (km)

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200 400 Days

Anomaly

c

Composite StDev x SQRT(2)

d

  • What ¡

Happened ¡ Expected ¡ EvoluIon ¡

Coy ¡et ¡al. ¡submiLed ¡to ¡

  • J. ¡Climate ¡

QBO ¡‘reboot’ ¡of ¡2016 ¡in ¡MERRA-­‑2 ¡

Out-of-phase easterlies disrupt the westerly phase in a broad layer centered around 40 hPa Unp Unprecedent nted Oddball ¡Disrupted ¡Unexpected ¡ Anomalous ¡Rebooted ¡Hiccup ¡ dip into the gravitational field of a black hole Reported by Newman et al., 2016, GRL Osprey et al., 2016, Science ¡

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20 40 60 Latitude 1000 100 10 1 Pressure (hPa)

2016

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1 1 1 1 1 1 3 3 5 7 February momentum flux

a

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20 40 60 Latitude 1000 100 10 1 Pressure (hPa)

2014

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1 1 1 1 1 1 February momentum flux

b

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20 40 60 Latitude 1000 100 10 1 Pressure (hPa)

2011

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1 1 1 1 1 1 February momentum flux

c

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20 40 60 Latitude 1000 100 10 1 Pressure (hPa)

1998

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1 1 1 1 1 1 February momentum flux

d

Horizontal Momentum Flux (February)

Normalized ¡by ¡the ¡ Standard ¡DeviaIon ¡ (mean ¡removed) ¡ Momentum ¡ Heat ¡

2016 ¡ 1998 ¡ 2014 ¡ 2011 ¡

40 ¡ ¡

Large ¡(+9) ¡40 ¡hPa ¡and ¡ Large ¡(+3) ¡upper ¡ troposphere ¡ momentum ¡flux. ¡ ¡ ¡

Coy ¡et ¡al. ¡submiLed ¡to ¡J. ¡ Climate ¡

QBO ¡‘reboot’ ¡of ¡2016 ¡in ¡MERRA-­‑2 ¡

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2015 2016 2017 2018

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5 5 5

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100 10 Pressure (hPa) 20 25 30 35 Pressure Altitude (km) 2015 2016 2017 2018

b

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5

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5 5 5

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5

100 10 Pressure (hPa) 20 25 30 35 Pressure Altitude (km)

  • 50
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5 10 15 20 25 30 35 40 45 50 U (ms-1)

Seasonal Forecasts

Zonal ¡Mean ¡ Zonal ¡Wind ¡ 10oS-­‑10oN ¡

MERRA-­‑2 ¡ 1 ¡Jul ¡Fcst ¡ 2018 ¡

100 ¡ 4 ¡

Forecast ¡calls ¡for ¡ descent ¡of ¡ verIcal ¡shear ¡ zones ¡ Forecast ¡ erroneously ¡ called ¡for ¡ descent ¡of ¡early ¡ Jan ¡verIcal ¡ shear ¡zones ¡ Normal ¡ Disrupted ¡

2015 ¡ 2016 ¡ 2017 ¡ MERRA-­‑2 ¡ 1 ¡Jan ¡Fcst ¡

(Low ¡Horizontal ¡ ResoluIon) ¡

QBO ¡‘reboot’ ¡of ¡2016 ¡in ¡MERRA-­‑2 ¡

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National Aeronautics and Space Administration gmao.gsfc.nasa.gov ¡

Adding the STRATCHEM chemistry model to GEOS-DAS; Research & Development stage

  • STRATCHEM replaces a simplified parameterized chemistry scheme

used in GMAO’s operational data assimilation experiments to date

  • 34 transported and 17 derived species
  • 124 gas-phase and 39 photolysis reactions
  • Includes a PSC scheme and heterogeneous reactions
  • Reaction rates follow the recommendations in JPL 2010

We plan to assess its viability for use in future products

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STRATCHEM: Towards ozone forecasts

Ozone ¡hole ¡area ¡ Ozone ¡hole ¡area ¡ Ozone ¡mass ¡ deficit ¡ Ozone ¡mass ¡ deficit ¡ With ¡parameterized ¡chem. ¡ With ¡STRATCHEM ¡ At ¡present, ¡the ¡model ¡is ¡ not ¡suited ¡for ¡running ¡

  • zone ¡forecasts ¡beyond ¡a ¡

few ¡hours ¡ ¡ With ¡full ¡chemistry ¡we ¡ have ¡a ¡good ¡ozone ¡hole ¡ forecast ¡skill ¡out ¡to ¡at ¡ least ¡10 ¡days ¡

Analysis 5-day forecast 10-day forecast

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Chemical tendency Sunlit fraction of the vortex Temperature at the pole Time- integrated tendency

Chemical ozone loss

  • Late December to mid-March after the vortex broke apart
  • Maxima in early and late February correspond to vortex displacements (minor

and final warmings) exposing larger portions of the vortex to sunlight

  • Maximum cumulative loss of ~2.1 at 480 K (~18-20 km)

STRATCHEM: polar processing in 2015/2016

~20 ¡km ¡

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MERRA-2 AMIP simulations

Ensemble of 10 model runs using the MERRA-2 GCM, at the same resolution, with the same boundary conditions and covering the same period. Purpose: Determine how the model climate compares with the reanalysis (and

  • ther atmospheric models), identify errors
  • For the stratosphere we will be interested in derived diagnostics, e.g. B-D circulation, age of air
  • Note that ozone and water vapor are constrained by climatologies – probably less interesting

than dynamics and transport

  • Currently in production; 5 ensemble members finished
  • The output will be made publicly available

This is work in progress. We haven’t looked at the stratosphere yet

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National Aeronautics and Space Administration gmao.gsfc.nasa.gov ¡

Replay ¡and ¡downscaling ¡

Assimilation Generate the analysis state, ANA INCREMENT = ANA-BKG Force the GCM with INCREMENT Run GCM, generate new BKG Replay Use ANA from an existing analysis INCREMENT = ANA-BKG Force the GCM with INCREMENT Run GCM, generate new BKG

  • Faster (the analysis step is already done)
  • Can be run with a different model and/or at different resolution
  • Analysis increments can be applied selectively

GMAO has produced a 12.5 km resolution replay of MERRA-2 (2000-2015)

  • Weather: tropical cyclones better resolved, differences in

precipitation

  • Stratosphere: gravity waves resolved better than in MERRA-2

Omega ¡[Pa/s] ¡ MERRA-­‑2 ¡ 12.5 ¡km ¡replay ¡

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National Aeronautics and Space Administration gmao.gsfc.nasa.gov ¡

Transport ¡in ¡the ¡model, ¡analysis ¡and ¡replay ¡

There exist systematic differences in transport between analysis, CTM, and replay: The use of instantaneous analysis fields leads to systematic errors in transport

These issues are being investigated ¡

Replay minus analysis N2O at 480 K, 1 March 2015 % ¡

Realistic age of air in MERA-2 driven CTM Too young in replay Improved with time-averaged analysis forcing Replay produces faster descent inside the polar vortex leading to lower N2O mixing ratio

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Transition to 4D-EnVar

  • A version of 4D data assimilation in which

– Ensemble forecasts are used to estimate background error covariances – The ensemble eliminates the need for a tangent linear and adjoint model integration

  • In this implementation the background error

covariance matrix is a combination of a static and an ensemble component

  • 32 ensemble members
  • Incremental analysis update
  • Now run in parallel to the operational forward

processing; it will become the next operational stream

Pressure ¡[hPa] ¡ StaIc ¡B ¡ Ensemble ¡B ¡

Ensemble & static component weights

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Other ongoing developments

  • Vertical resolution: 72 layers à 132 layers; ~0.5 km in the stratosphere
  • Seasonal forecasts (contributing to the North American Multi-Model

Ensemble): upgrade to a more recent model configuration in progress

  • Tropospheric chemistry: inclusion of a new tropospheric chemistry model

(GEOS-Chem), carbon data assimilation, work towards multispecies data assimilation

Plans for new reanalyses

  • MERRA-2 based full chemistry reanalysis (in replay mode)
  • Coupled atmosphere-ocean-land-ice 1980 onwards
  • High resolution atmospheric reanalysis 2000s
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Summary of GMAO developments

  • GMAO validation of MERRA-2 and research

– Stratosphere: a section in Gelaro et al., QBO paper (Coy et al. 2016a); anomalous 2016 QBO: Newman et al., 2016, Coy et al. 2016b; polar TIL and SSWs (Wargan & Coy 2016) – Ozone: Wargan et al., ozone validation paper submitted to J. Clim.

  • Introduction of full stratospheric chemistry
  • MERRA-2 AMIP and downscaling experiments
  • Ongoing research on stratospheric transport in analyses, models

and replay

  • Transition to 4D-EnVAR
  • Lots and lots of work on the troposphere, land and ocean…

Note: production of MERRA was discontinued; final date: 29 February 2016

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Technical note: Incremental Analysis Update; ‘ANA’ vs. ‘ASM’ output

Each predictor step, e.g. 15 min: xi+1 = xi+Δx(xi) In the corrector step: xi+1 = xi+Δx(xi)+ΔANA

Nonlinearity sits here: the tendency depends on state, which depends

  • n the analysis increment

‘ANA’ = background state + analysis increment ‘ANA’ : the analyzed states, the closest to the observations, 6-hourly, only assimilated fields ‘ASM’: the IAU state, consistency between fields and tendencies (dynamical, radiative,…), 3-hourly, larger set of fields (e.g. EPV). Use ‘ASM’ for most applications

Diagram by Bill Putman

ASM ¡

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backup ¡

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Wargan ¡ ¡et ¡al., ¡2016 ¡

Tropopause – 50 hPa MERRA ¡ MERRA-­‑2 ¡

Difference ¡St. ¡Dev. ¡

  • Improvement. ¡

Correla[ons ¡ Lower stratospheric ozone between 30°N and 60°N in ozonesondes, MERRA and MERRA-2

  • Error standard deviation 11.2% (8.1 % in the

Aura period)

  • Very high correlation

MERRA-2 performs significantly better than MERRA when Aura data are assimilated

Status of MERRA-2 validation: ozone

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20 40 60 80 100 120 140

Analysis times

0.5 1 1.5 2 2.5 3

MLS global statistics for March 2016

MERRA-2 O-F STRATCHEM O-F MERRA-2 O-A STRATCHEM O-A

Penalty ¡func[on ¡

STRATCHEM: Impact on the GEOS-DAS performance

Large reduction in the MLS ozone term of the penalty function indicates much better agreement between the model and MLS and a healthier data assimilation system.

MERRA-2 GEOS- STRATCHEM

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Note ¡on ¡MLS ¡ozone ¡data ¡versions ¡ ¡

We replaced MLS v2.2 with v4.2 on 1 June 2015 We turned off the 261 hPa level on 1 May 2016 because of high bias

Pressure ¡[hPa] ¡ Pressure ¡[hPa] ¡ Version ¡2.2 ¡ Version ¡4.2 ¡

V 2.2 Oct 2004-May 2015 V4.4 w/ 261 hPa level June 2015 – May 2016 V4.4, 261 hPa turned off Since June 2016