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