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AP IOP 10 South Foehn Event in the Wipp Valley: Verification of High-Resolution Numerical Simulations with Observations A. Gohm*, G. Zängl**, G. J. Mayr* * University of Innsbruck, Austria ** University of Munich, Germany CAM/MAP 2003 Brig, Switzerland, May 19 to 23, 200 Gohm, A., G. Zängl, G. J. Mayr, 2003, submitted to Mon. Wea. Rev.

MAP IOP 10 South Foehn Event in the Wipp Valley: Verification of High-Resolution Numerical

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ICAM/MAP 2003 Brig, Switzerland, May 19 to 23, 2003. MAP IOP 10 South Foehn Event in the Wipp Valley: Verification of High-Resolution Numerical Simulations with Observations A. Gohm*, G. Zängl**, G. J. Mayr* * University of Innsbruck, Austria ** University of Munich, Germany. - PowerPoint PPT Presentation

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Page 1: MAP IOP 10 South Foehn Event in the Wipp Valley: Verification of High-Resolution Numerical

MAP IOP 10 South Foehn Event in the Wipp Valley:

Verification of High-Resolution Numerical

Simulations with Observations

A. Gohm*, G. Zängl**, G. J. Mayr*

* University of Innsbruck, Austria

** University of Munich, Germany

ICAM/MAP 2003 Brig, Switzerland, May 19 to 23, 2003

Gohm, A., G. Zängl, G. J. Mayr, 2003, submitted to Mon. Wea. Rev.

Page 2: MAP IOP 10 South Foehn Event in the Wipp Valley: Verification of High-Resolution Numerical

The scientific objective:

To assess to what extent the temporal evolution and spatial structure of small-scale orographic flows can be simulatedwith a state-of-the-art mesoscale model run in a very high-resolution mode.

The phenomenon:

Deep south foehn in the Wipp Valley on 24-25 October 1999

The scientific tools:

• Penn State/NCAR mesoscale model MM5• NOAA/ETL ground-based scanning Doppler lidar (TEACO2)• NCAR airborne aerosol backscatter lidar (SABL)• ZAMG Doppler sodar• radiosoundings and weather stations

Page 3: MAP IOP 10 South Foehn Event in the Wipp Valley: Verification of High-Resolution Numerical

MM5 basic setup:

• 6 domains with x = 64.8 – 0.267 km

• 39 full-sigma levels

• initialized with operational ECMWF analysis at 23 Oct 18 UTC and 24 Oct 00 UTC

Wipp Valley Innsbruck

Brenner Pass

Page 4: MAP IOP 10 South Foehn Event in the Wipp Valley: Verification of High-Resolution Numerical

Backscatter intensityversus potentialtemperature,15 UTC 24 Oct 1999:

P1

P2

MM5 00 UTC run

AML top heights &isentropes indicateregions of flow descentand jump-like features

indications forunderestimation offlow descent

SABL lidar on NCAR Electra

InnsbruckBrenner

flow

Page 5: MAP IOP 10 South Foehn Event in the Wipp Valley: Verification of High-Resolution Numerical

Wind profile at Brenner Pass, 24 Oct 1999:

ZAMG PA2 sodar MM5 00 UTC run, D6 simulated windspeed 15 % too high

lower gap area30% too large in D6

simulated massflux 50% too high

00 (18) UTC run: RMSE = 5.6 (6.2) m/sME = +1.5 (+1.6) m/s

Alpine crest line

lower gap

upper gap

Page 6: MAP IOP 10 South Foehn Event in the Wipp Valley: Verification of High-Resolution Numerical

Wind speed, 24 Oct 1999:

too strong winds

Page 7: MAP IOP 10 South Foehn Event in the Wipp Valley: Verification of High-Resolution Numerical

Potential temperature, 24 Oct 1999:

-2 K bias

Page 8: MAP IOP 10 South Foehn Event in the Wipp Valley: Verification of High-Resolution Numerical

Radial windvelocity,24 Oct 1999:

lidar Doppler lidar

09 UTC

MM5 (00 UTC run)

-1.6-3.1ME

5.36.9RMSE

15Z09ZTime

abs(radial velocity)00 UTC run – lidar

15 UTC

Doppler lidar

MM5 (00 UTC run)

Page 9: MAP IOP 10 South Foehn Event in the Wipp Valley: Verification of High-Resolution Numerical

Inversion upstreamof the pass,09 UTC 24 Oct 1999:

upstream inversion1 km too low early inthe event (~09 UTC)

southerly flow tooshallow

MM5 (00 UTC run): domain 4

Page 10: MAP IOP 10 South Foehn Event in the Wipp Valley: Verification of High-Resolution Numerical

Conclusions:

The model captured several striking features:

• foehn break-through in the Inn Valley

• magnitude of surface wind speed at several weather stations

• regions of strong descent

• jump-like features related to deep amplified gravity waves

Discrepancies were found between simulations and observations:

• overestimation of the mass flux through lower Brenner gap (+50%)

• underestimation of the descent of potentially warm air through upper gap

• bias of surface pot. temperature in the northern Wipp Valley (-2 K)

• wrong inversion height upstream of the pass early in the event

Page 11: MAP IOP 10 South Foehn Event in the Wipp Valley: Verification of High-Resolution Numerical

ECMWF analysis12 UTC 24 Oct 1999:

500 hPa geopot. height:

Sea level pressure:

L

H

Page 12: MAP IOP 10 South Foehn Event in the Wipp Valley: Verification of High-Resolution Numerical

MM5 flow structure,15 UTC 24 Oct 1999,00 UTC run:

surface wind speed:wind speed &

pot. temperature:

Brenner Innsbruck

Page 13: MAP IOP 10 South Foehn Event in the Wipp Valley: Verification of High-Resolution Numerical

Pressure gradient, 24 Oct 1999:

as function of time

as function of wind speed

Page 14: MAP IOP 10 South Foehn Event in the Wipp Valley: Verification of High-Resolution Numerical

Doppler lidar rad. vel.

09 UTCRadial windvelocity,24 Oct 1999:

15 UTC

lidar

MM5 (00 UTC run) rad.vel.

MM5 (00 UTC run) + wspd-1.6-3.1ME

5.36.9RMSE

15Z09ZTime

abs(radial velocity)00 UTC run – lidar