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christoph.schraff@dwd.de Status of PP KENDA COSMO General Meeting, Sibiu, 2 – 5 Sept. 2013 1 Status Report PP KENDA Christoph Schraff Deutscher Wetterdienst, Offenbach, Germany Contributions / input by: Hendrik Reich, Andreas Rhodin, Annika Schomburg, Ulrich Blahak, Yuefei Zeng, Roland Potthast Yuefei Zeng, Klaus Stephan, Africa Perianez, Michael Bender (DWD) Chiara Marsigli, Tiziana Paccagnella (ARPA-SIM) Lucio Torrisi (CNMCA) Daniel Leuenberger, Luca Weber (MeteoSwiss) Mikhail Tsyrulnikov, Igor Mamay (HMC) Amalia Iriza (NMA) general overview assimilation of SEVIRI-derived cloud top height in LETKF

Status Report PP KENDA

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Status Report PP KENDA. Christoph Schraff Deutscher Wetterdienst, Offenbach, Germany. Contributions / input by: Hendrik Reich, Andreas Rhodin, Annika Schomburg, Ulrich Blahak, Yuefei Zeng, Roland Potthast Yuefei Zeng, Klaus Stephan, Africa Perianez, Michael Bender (DWD) - PowerPoint PPT Presentation

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Page 1: Status Report  PP KENDA

[email protected] of PP KENDACOSMO General Meeting, Sibiu, 2 – 5 Sept. 2013 1

Status Report PP KENDA

Christoph SchraffDeutscher Wetterdienst, Offenbach, Germany

Contributions / input by:

Hendrik Reich, Andreas Rhodin, Annika Schomburg, Ulrich Blahak, Yuefei Zeng, Roland Potthast

Yuefei Zeng, Klaus Stephan, Africa Perianez, Michael Bender (DWD)Chiara Marsigli, Tiziana Paccagnella (ARPA-SIM)Lucio Torrisi (CNMCA)Daniel Leuenberger, Luca Weber (MeteoSwiss)Mikhail Tsyrulnikov, Igor Mamay (HMC)Amalia Iriza (NMA)

• general overview

• assimilation of SEVIRI-derived cloud top height in LETKF

Page 2: Status Report  PP KENDA

[email protected] of PP KENDACOSMO General Meeting, Sibiu, 2 – 5 Sept. 2013 2

LETKF: implementation

experiment chain in NUMEX set up

• GME LETKF experiment for June 2011

• lateral BC by direct interpolation from 60 km to 2.8 km

• KENDA:– 1-hourly cycling, radiosonde, aircraft, wind profiler, synop– 40 ensemble members, basic set-up (only adaptive cov. infl.)– assimilation only, optimally takes 1 real day for 1 day of assimilation,

but in fact: ~ 1 – 4 real months for 1 week of assimilation !

(without forecasts !!) only 3 experiments so far

Page 3: Status Report  PP KENDA

[email protected] of PP KENDACOSMO General Meeting, Sibiu, 2 – 5 Sept. 2013 3

LETKF: implementation

• other work: • adaptive estimation of observation errors in observation space• multi-step analysis implemented• compare KENDA ensemble forecasts with COSMO-DE-EPS (8 days)

• at MCH / ARPA-SIM : studies on influence of different lateral BC (resolution gap)

• at MCH: compare determinstic LETKF analysis with nudging ana. (7 days)

• Hendrik: new flexible stand-alone scripts to run LETKF experiments without using NUMEX / archive very limited disk space

1 real day for 1 day of LETKF assimilation• to do: implement evaluation / verification tools in script suite• may become very suitable tool for users outside DWD (academia)

Page 4: Status Report  PP KENDA

[email protected] of PP KENDACOSMO General Meeting, Sibiu, 2 – 5 Sept. 2013 4

Impact of lateral BC resolution

Marsigli, Paccagnella, Montani: Test impact of lateral BC resolution for convection-permitting EPS

• 8 cases from Hymex SOP: 6 Sept. – 5 Nov. 2012

• COSMO-H2-EPS set-up (‘H2-CLEPS’):• 2.8 km, 50 levels• 10 members• IC + BC COSMO-LEPS,

res. 7 km• run at 12 UTC• 36h forecast range

• exp. ‘H2-IFS’: direct nesting• IC and BC from IFS-EPS• res: 0.25 °

Page 5: Status Report  PP KENDA

[email protected] of PP KENDACOSMO General Meeting, Sibiu, 2 – 5 Sept. 2013 5

mean difference between pairs of ensemble members < spread < rmse (i.e. e.g. betw. Member 1 of H2-CLEPS and Member 1 of H2-IFS)

• 1 exceptional case

• spin-up noise dieswithin 30 min

• impact on precipscores negligible

500 hPa geopotential

Impact of lateral BC resolution

Page 6: Status Report  PP KENDA

[email protected] of PP KENDACOSMO General Meeting, Sibiu, 2 – 5 Sept. 2013 6

LETKF: implementation of verification

• production of ‘full’ NetCDF feedback files

done: make clean interfaces to observation operators in COSMO …… integrate them into 3DVAR package

to be done (this autumn !) :extend flow control (read correct Grib files etc.)

• ensemble-related diagnostic + verification tool, using feedback files :(Iriza, NMA)

– ensemble scores implemented, further testing required

Page 7: Status Report  PP KENDA

[email protected] of PP KENDACOSMO General Meeting, Sibiu, 2 – 5 Sept. 2013 7

testing KENDA at MCH, ARPA-SIM

• OSSE

–temperature inversion in Po Valley: assimilate synthetic TEMP

–(semi-)idealised: horizontally homogeneous case; daily cycle of Alpine pumping

develop OSSE capability

COSMO reading feedback files implemented

• no PhD project on idealised OSSE to investigate convective-scale issues

Page 8: Status Report  PP KENDA

[email protected] of PP KENDACOSMO General Meeting, Sibiu, 2 – 5 Sept. 2013 8

accounting for model error

• stochastic perturbation of physics tendencies (SPPT)(Torrisi)

–perturbation of moist turbulence tendencies implemented

–implemented in (private) V4_26

–tests (LETKF for COSMO-ME): drying effect on precip

–further tests in MCH / ARPA-SIM

• Pattern Generator (for random fields with prescribed correlation scales)(Tsyrulnikov et al.)

Page 9: Status Report  PP KENDA

[email protected] of PP KENDACOSMO General Meeting, Sibiu, 2 – 5 Sept. 2013 9

high-resolution obs

• radar

–obs operators finished

–radial winds vr in LETKF: Yuefei Zeng (DWD, until summer 2014)

monitoring of 3d volumn data (statistics of observation increments) :large scatter, data quality problems

need to test thinning / superobbing strategies 3-hour assimilation with 1-hrly cycle done (different localization radii)

–vr + reflectivity Z in LETKF: Theresa Bick (HErZ-I Bonn, until end 2014 at least)

• GPS slant path delay

–obs operator (incl. TL / adjoint) implemented in 3DVar, approximations tested

–implementation in COSMO should start soon

Page 10: Status Report  PP KENDA

[email protected] of PP KENDACOSMO General Meeting, Sibiu, 2 – 5 Sept. 2013 10

high-resolution obs

• (SEVIRI-based, radiosonde-corrected) cloud top height : see next slides(Schomburg)

• new task: Raman lidar and microwave radiometer T- , q- profiles(Haefele, MCH)

• direct assimilation of SEVIRI radiances (window channels for cloud info)(Perianez)

–technically implemented (obs operator (RTTOV), reading / writing)

–work on monitoring / assimilation start in Nov.

Page 11: Status Report  PP KENDA

[email protected] of PP KENDACOSMO General Meeting, Sibiu, 2 – 5 Sept. 2013 11

• avoid too strong penalizing of members with high humiditybut no cloud

• avoid strong penalizing of members which are dry at CTHobs but have a cloud or even only high humidity close to CTHobs

search in a vertical range hmax around CTHobs fora ‘best fitting’ model level k, i.e. with minimum ‘distance’ d:

Z [km]

Cloud top

RH [%]

CTHobs

2

max

2 )(1))()((min obskobskkCTHh

hRHfRHfd

function of relative humidity

height ofmodel level

k

= 1

• use f (RHobs=1) – f (RHk)and CTHobs – hk as 2 separate obs increments in LETKF

if cloud observed with cloud top height CTHobs ,what is the appropriate type of obs increment ?

(if above a layer with cloud fraction > 70 %, then choose top of that layer)

use of (SEVIRI-based) cloud top height (CTH) ‘observations’ in LETKF: method

Page 12: Status Report  PP KENDA

[email protected] of PP KENDACOSMO General Meeting, Sibiu, 2 – 5 Sept. 2013 12

3

6

9

12

Z [km]

„no cloud“

„no cloud“

„no cloud“

CLC

• assimilate cloud fraction CLC = 0 separatelyfor high, medium, low clouds

• model equivalent: maximum CLC within vertical range

type of obs increment , if no cloud observed ?

3

6

9

12

Z [km]

- no data -

„no cloud“

Cloud top

model profile

use of (SEVIRI-based) cloud top height (CTH) ‘observations’ in LETKF: method

Page 13: Status Report  PP KENDA

[email protected] of PP KENDACOSMO General Meeting, Sibiu, 2 – 5 Sept. 2013 13

relative humiditycloud covercloud water

cloud iceobserved cloud top

3 lines on one colour indicate ensemble mean and mean +/- spread

• 1 analysis step , 17 Nov. 2011, 6 UTC (wintertime low stratus)

vertical profiles

• example: missed cloud event

CTH single-observation experiments

Page 14: Status Report  PP KENDA

[email protected] of PP KENDACOSMO General Meeting, Sibiu, 2 – 5 Sept. 2013 14

observed cloud top

observation location

• example: missed cloud event

specific water content [g/kg]

relative humidity [%]

cross section of analysis increments for ensemble mean

CTH single-observation experiments

Page 15: Status Report  PP KENDA

[email protected] of PP KENDACOSMO General Meeting, Sibiu, 2 – 5 Sept. 2013 15

CTH single-observation experiments

temperature profile (mean +/- spread)

• example: missed cloud event

first guess analysis

1000 m

2000 m

3000 m

observed cloud top

LETKF introduces inversion due to RH(CTH) T cross correlations in first guess ensemble perturbations

270 K 280 K 290 K 270 K 280 K 290 K

Page 16: Status Report  PP KENDA

[email protected] of PP KENDACOSMO General Meeting, Sibiu, 2 – 5 Sept. 2013 16

relative humiditycloud covercloud water

cloud iceobserved cloud top

3 lines on one colour indicate ensemble mean and mean +/- spread

vertical profiles

• example: false alarm cloud assimilated quantity: cloud fraction (= 0)

CTH single-observation experiments

Page 17: Status Report  PP KENDA

[email protected] of PP KENDACOSMO General Meeting, Sibiu, 2 – 5 Sept. 2013 17

high cloud cover [octas]

FG

ANA

LETKF decreases erroneous cloud cover despitevery non-Gaussian distributions

mid-level cloud cover [octas]

FG

ANA

• example: false alarm cloud assimilated quantity: cloud fraction (= 0)

FG

ANA

low cloud cover [octas]

cover

CTH single-observation experiments

observation increments - histogram over ensemble members

Page 18: Status Report  PP KENDA

[email protected] of PP KENDACOSMO General Meeting, Sibiu, 2 – 5 Sept. 2013 18

• example: false alarm cloud assimilated quantity: cloud fraction (= 0)

FG

ANA

low cloud cover [octas] mid-level cloud cover [octas] high cloud cover [octas]

cover

CTH single-observation experiments

observation increments - histogram over ensemble members

FG

ANA

FG

ANA

LETKF decreases erroneous cloud cover despitevery non-Gaussian distributions

Page 19: Status Report  PP KENDA

[email protected] of PP KENDACOSMO General Meeting, Sibiu, 2 – 5 Sept. 2013 19

0:00 UTC 6:00 UTC 12:00 UTC 17:00 UTC

cycled assimilation of dense CTH obs

observed cloud top height (CTH)

1-hourly cycle over 21 hours, 13 Nov., 21 UTC – 14 Nov. 2011, 18 UTC(wintertime low stratus)

Page 20: Status Report  PP KENDA

[email protected] of PP KENDACOSMO General Meeting, Sibiu, 2 – 5 Sept. 2013 20

20

0:00 UTC 6:00 UTC 12:00 UTC 17:00 UTC

cycled assimilation of dense CTH obs :LETKF setup

• thinning: use obs at every 5th grid pt.• adaptive covariance inflation, adaptive localisation scale ( ~ 35 km)• Observation error variances : relative humidity = 10 %

cloud cover = 3.2 octacloud top height [m] :

Page 21: Status Report  PP KENDA

[email protected] of PP KENDACOSMO General Meeting, Sibiu, 2 – 5 Sept. 2013 21

cycled assimilation of dense CTH obs

FGANA

RMSE

bias

analysis error smaller than first guess (FG) errors

time series of errors for deterministic run, averaged over cloudy obs locations

‘CTH’ CTHobs heightk ‘RH’ 1 - RHk (k : ‘best fitting model level’)

‘RH at obslev’(i.e. at observed CTH)

Page 22: Status Report  PP KENDA

[email protected] of PP KENDACOSMO General Meeting, Sibiu, 2 – 5 Sept. 2013 22

22

cycled assimilation of dense CTH obs

RMSE

spread

time series of errors of ensemble mean / spread of ensemble

averagedover

cloudy obs

locations

averagedover

cloud-free obs

locations

underdispersive,but no trend for reductionof spread

Page 23: Status Report  PP KENDA

[email protected] of PP KENDACOSMO General Meeting, Sibiu, 2 – 5 Sept. 2013 23

RMSE

bias

time series of first guess errors (det. run), averaged over cloudy obs locations

cycled assimilation of dense CTH obs

no assimilationwith cloud assimilation

CTH assimilation : hardly reduces height error of selected level k

reduces RH (1-hour forecast) errors

‘RH at obslev’

Page 24: Status Report  PP KENDA

[email protected] of PP KENDACOSMO General Meeting, Sibiu, 2 – 5 Sept. 2013 24

cycled assimilation of dense CTH obs

RH at obslev

RMSE

bias

no assimilationwith cloud assimilation

CTH assimilation : reduces RH errors related to low + mid-level cloud

time series of first guess errors, averaged over cloudy obs locations

Page 25: Status Report  PP KENDA

[email protected] of PP KENDACOSMO General Meeting, Sibiu, 2 – 5 Sept. 2013 25

cycled assimilation of dense CTH obs

time series of first guess errors, averaged over cloud-free obs locations(errors are due to false alarm cloud)

mean square error of cloud fraction [octas]

Page 26: Status Report  PP KENDA

[email protected] of PP KENDACOSMO General Meeting, Sibiu, 2 – 5 Sept. 2013 26

low clouds mid-level clouds high clouds

cycled assimilation of dense CTH obs

‘false alarm’ cloud cover

(after 6 hrs cycling)

with cloud assimilation

no assimilation

Page 27: Status Report  PP KENDA

[email protected] of PP KENDACOSMO General Meeting, Sibiu, 2 – 5 Sept. 2013 27

time series of first guess errors, averaged over cloudy obs locations

cycled assimilation of dense CTH obs

assimilation of conventional obs only assimilation of conventional + cloud obs

localization scale: adaptive / 20 km

RMSE

bias

CTH assimilation : reduces RH (1-hour forecast) errorseven slightly reduces height error of selected level k

Page 28: Status Report  PP KENDA

[email protected] of PP KENDACOSMO General Meeting, Sibiu, 2 – 5 Sept. 2013 28

no assimilation

RH at obslev

cycled assimilation of dense CTH obs

first guess fields after 20 hours of cycling (cloudy obs locations)

CTH obs

cloud assimilation

conventional only conventional + cloud

Page 29: Status Report  PP KENDA

[email protected] of PP KENDACOSMO General Meeting, Sibiu, 2 – 5 Sept. 2013 29PBPV – 03/2013

29

No assim

no assimilation cloud assimilation

conventional only conventional + cloud

total cloud coverof first guessfields after

20 hours of cycling

CTH obs

satellite obs

cycled assimilation of dense CTH obs

Page 30: Status Report  PP KENDA

[email protected] of PP KENDACOSMO General Meeting, Sibiu, 2 – 5 Sept. 2013 30

cycled assimilation of dense CTH obs

time series of first guess errors, averaged over cloud-free obs locations(errors are due to false alarm cloud)

mean square error of cloud fraction [octas]

error reduced(almost) everywhere

Page 31: Status Report  PP KENDA

[email protected] of PP KENDACOSMO General Meeting, Sibiu, 2 – 5 Sept. 2013 31

low clouds mid-level clouds high clouds

cycled assimilation of dense CTH obs

‘false alarm’ cloud cover

(after 20 hrs cycling)

conventional+ cloud

conventionalobs only

Page 32: Status Report  PP KENDA

[email protected] of PP KENDACOSMO General Meeting, Sibiu, 2 – 5 Sept. 2013 32

Summary

•assimilation of CTH by LETKF reduces errors of first guess (1-h forecast)

tends to introduce humidity / cloud where it should (+ temperature inversion)

tends to reduce ‘false-alarm’ clouds

despite non-Gaussian pdf’s

•no sign of filter collapse (decrease of spread)

•next: evaluate forecast impact

use of (SEVIRI-based) cloud top height (CTH) ‘observations’ in LETKF

Page 33: Status Report  PP KENDA

[email protected] of PP KENDACOSMO General Meeting, Sibiu, 2 – 5 Sept. 2013 33

Page 34: Status Report  PP KENDA

[email protected] of PP KENDACOSMO General Meeting, Sibiu, 2 – 5 Sept. 2013 34

with cloud

assimilation

no assimilation‘CTH‘ OBS-FG RH RH at obslev

cycled assimilation of dense CTH obs

first guess fields after 20 hours of cycling (cloudy obs locations)

CTH obs

Page 35: Status Report  PP KENDA

[email protected] of PP KENDACOSMO General Meeting, Sibiu, 2 – 5 Sept. 2013 35

Low cloud cover (COSMO)

PBPV – 03/201335

17:00 UTCCloud assim

conv Cloud +conv

No assim

Page 36: Status Report  PP KENDA

[email protected] of PP KENDACOSMO General Meeting, Sibiu, 2 – 5 Sept. 2013 36

RMSE and bias for different heights separately: Cloud assim. vs. no assim.

RH@oblsev

Page 37: Status Report  PP KENDA

[email protected] of PP KENDACOSMO General Meeting, Sibiu, 2 – 5 Sept. 2013 37

LETKF: validation of forecasts from KENDA

COSMO-DE EPS

EPS on KENDA

intermediate

combined