jim marquis, yvette richardson, paul markowski , david dowell,

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Our experiences with EnKF assimilation of high-res radar observations collected in the 5 June 2009 Vortex 2 tornadic supercell. Jim Marquis, Yvette Richardson, Paul Markowski, David Dowell, Josh Wurman, Karen Kosiba, Paul Robinson Photo by Sean Waugh

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Our experiences with EnKF assimilation of high-res radar observations collected in the 5 June 2009 Vortex 2 t ornadic supercell . Jim Marquis, Yvette Richardson, Paul Markowski , David Dowell, Josh Wurman , Karen Kosiba , Paul Robinson. Photo by Sean Waugh. Goals of EnKF analysis. - PowerPoint PPT Presentation

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Page 1: Jim Marquis, Yvette Richardson, Paul  Markowski , David Dowell,

Our experiences with EnKF assimilation of high-res radar observations collected

in the 5 June 2009 Vortex 2 tornadic supercell.

Jim Marquis,Yvette Richardson, Paul Markowski, David Dowell,

Josh Wurman, Karen Kosiba, Paul RobinsonPhoto by Sean Waugh

Page 2: Jim Marquis, Yvette Richardson, Paul  Markowski , David Dowell,

Goals of EnKF analysis• Increase availability of 3-D kinematic and

thermodynamic data (dual-Doppler and in situ obs are spatially/temporally limited).

Courtesy of Paul Markowski

Page 3: Jim Marquis, Yvette Richardson, Paul  Markowski , David Dowell,

Goals of EnKF analysis• We want a set of smoothly evolving EnKF analyses

(i.e., We are not using EnKF to initialize a forecast).

• Analyze roles that mesocyclone-scale processes play in tornadogenesis, maintenance, and decay:

- trajectory analysis,- circulation/vorticity budgets,

- mid-upper level features.

Page 4: Jim Marquis, Yvette Richardson, Paul  Markowski , David Dowell,

Model Specifics• WRF-ARW 3.2.1:

-Δx,y = 500 m, 80m < Δz < 2km, [120 x 80 x 20] km3 -LFO microphysics,-open lateral BCs,-no surface fluxes, no radiation, flat terrain.

Homogeneous environment:

Page 5: Jim Marquis, Yvette Richardson, Paul  Markowski , David Dowell,

DA Specifics• DART:

– Ensemble adjustment filter,

– 50 members,– Localization:• Gaspari-Cohn, W = 0 @ r = 6 km

– Ensemble initiation:• 10 randomly placed warm bubbles at model t0 for each member

– Ensemble spread maintained with:• Additive noise added to T, Td, U, V every 5 min where radar

reflectivity is > 25 dBZ, (Dowell and Wicker 2009) • Perturbations smoothed to 4 km (horiz), 2 km (vert) scales

Page 6: Jim Marquis, Yvette Richardson, Paul  Markowski , David Dowell,

Courtesy www.vortex2.org

σ2obs = (2 m/s)2

• Radar velocities assimilated every 2 minutes

• OBAN: Cressman weighting

500 m horizontal grid spacing (for 500m-model grid experiment)

data along conical slices

Experiment timeline

“synthetic Data”

Page 7: Jim Marquis, Yvette Richardson, Paul  Markowski , David Dowell,

Thinning the amount of observations assimilated:

Unthinned 50% assim’ed 25% assim’ed

Model gridRadar vel. ob.

Y

X

No thinning done in vertical direction shown today; though, experiments show poor storm structure when low-level elevation angles are neglected.

Page 8: Jim Marquis, Yvette Richardson, Paul  Markowski , David Dowell,

θρdBZ ζW > 0

Z = 0.5 km AGL

(Note: these experiments conducted with 2-km model grid)

(K)

X

Y

50%

ass

imila

ted

25%

ass

imila

ted

u

nthi

nned

Y

Page 9: Jim Marquis, Yvette Richardson, Paul  Markowski , David Dowell,

ζradarsDu

al-D

oppl

erEn

KF

Wm/s

Z = 400 m AGL

Dual-Doppler – EnKF (ensemble mean) kinematics comparison(DOW6 & DOW7)

X (km)

Y (k

m)

Page 10: Jim Marquis, Yvette Richardson, Paul  Markowski , David Dowell,

Model errors/idealized conditions require DA for a good storm.

Storm structure with/without radar assimilation:

Top row: Series of EnKF (Ens. Mean) analyses.

Bottom row: Single member forecasted forward from 2157 (no DA).

ζ

Z = 150 m

X (km)

Y (k

m)

Page 11: Jim Marquis, Yvette Richardson, Paul  Markowski , David Dowell,

ζ

Ensemble mean analyses – temperature fields

Z = 50 m

(Note: these experiments conducted with 1-km model grid)

Page 12: Jim Marquis, Yvette Richardson, Paul  Markowski , David Dowell,

ζZ = 50 m

Mob. Mesonets

Page 13: Jim Marquis, Yvette Richardson, Paul  Markowski , David Dowell,

ζZ = 50 m

Mob. Mesonets

Page 14: Jim Marquis, Yvette Richardson, Paul  Markowski , David Dowell,

MM obs – EnKF outflow comparison

θ’(K)

ζ

Low-level wmax trace:dBZ MM obs:

Not great,particularly in farleft FF

Better overall, but still disagreement in FF

Decent, but stilldisagreement in FF

Warmth (lasts 1-2analysis times) - Seems to disagree With few available MM obs

Pretty good decent ok

MM’s only just getting into storm, but so far - not good

My < 1 sentence impression of the agreement of MM obs and eachEnKF analysis

Z = 50 m

• Sequence of EnKF analyses of theta’ and MM obs (valid +/- 1 min from EnKF analysis) overlayed:

ζZ = 50 m

Page 15: Jim Marquis, Yvette Richardson, Paul  Markowski , David Dowell,

Mesocyclone buoyancy (function of height & time)

Circulation and radial motion(function of radius & time)

Periods of tornado lifecycle

Pre-tornadic

T-genesisIntensification

MaturityWeakening

Time (UTC)

Inbound0 m/sOutbound

Positively buoyantNegatively buoyant

Page 16: Jim Marquis, Yvette Richardson, Paul  Markowski , David Dowell,

Trajectories (storm-rel.) calculated from ens. mean analyses

W (z = 200m)

Ring (radius = 1 km) of 20 parcels centered on peak ζ at z = 200 m; integrated forward in time from 4 times

θρ‘

(K)Most parcels rising into updraft

Some parcels rising into updraft

Few/no parcels rising into updraft

No parcels rising into updraft

Page 17: Jim Marquis, Yvette Richardson, Paul  Markowski , David Dowell,

θρ‘

(K)

Pre-tornadic T-genesis Intensification Maturity Weakening

Comparison across model grid resolutions

Page 18: Jim Marquis, Yvette Richardson, Paul  Markowski , David Dowell,

RMSI

Tota

l Sp

read

Cons

isten

cy

Rati

o

Page 19: Jim Marquis, Yvette Richardson, Paul  Markowski , David Dowell,

θ’(K)

Low-level wmax trace: MM obs:

ζ

Page 20: Jim Marquis, Yvette Richardson, Paul  Markowski , David Dowell,

Summary• EnKF Kinematic Analyses:

-Compare well with dual-Doppler fields of similar scale.-Storm-scale structure robust with different model scale.

More details come with finer model grid res.

• EnKF Thermo Analyses: - Mixed success with comparisons to MM in situ obs (where

available).- 500-m model grid seems verify with MM obs best in mesocyclone

area (partially due to more details captured?)- Seemingly random, possibly unphysical(?) anomalies appear more

prominently with finer model resolution.

Page 21: Jim Marquis, Yvette Richardson, Paul  Markowski , David Dowell,

Questions

1) Different way to maintain ensemble spread (adaptive methods)?

2) How else can we determine plausibility of analyses (kinematic and thermodynamic)?- Forcing terms along parcel trajectories?

3) More rigorous methods for optimizing scales/amounts of observations (compared to model resolution)?

Page 22: Jim Marquis, Yvette Richardson, Paul  Markowski , David Dowell,

Acknowledgements• The EnKF experiments were performed using NCAR CISL

supercomputing facilities with the Data Assimilation Research Testbed (DART) and WRF-ARW software.

• Thank you to Glen Romine, Lou Wicker, Dan Dawson, Chris Snyder, and Nancy Collins for advice/help.

• Thanks to all VORTEX2 crew for their dedication while collecting data on 5 June 2009.

• This research is funded by NSF grants: NSF-AGS-0801035, NSF-AGS-0801041. The DOW radars are NSF Lower Atmospheric Observing Facilities supported by NSF-AGS-0734001.