Lothar storm

Introduction

The Lothar storm that swept across Europe during 24-27 December 1999 is provided as a sample case study to use with OpenIFS. This storm was one of several storms to hit Europe in December 1999 and Lothar severely affected northern France, Switzerland and Germany (for more details see: Ulbrich et al., 2001, Weather, 56, 70-80).

The storms were characterized by record-breaking windspeed observations and rapid development across Europe. There was also a band of extremely high baroclinity near the cyclone track over the N. Atlantic and partly into Europe associated with Lothar.

The ECMWF forecasting system of the time did not accurately capture the storm's intensity though the strong jet stream was predicted some 9 days earlier. The storm initiated from a small disturbance in the Atlantic. More recently, Wedi et al, 2012, ECMWF Newsletter, have shown that very high resolution (T7999; ~2.5km) is necessary to model accurately the high wind speeds observed, particularly over the mountainous regions of Europe.

A number of initial conditions are provided along with suggested exercises.

Initial conditions

Case study initial conditions for the Lothar storm are provided on the OpenIFS ftp site. The Lothar depression developed initially on 24th December off the North American east coast at 35N.

The initial conditions are available at a range of different resolutions and start dates for a 10 day forecast. The experiment ids are created at ECMWF and used for identifying the model forecasts on the ECMWF archive system (for those with access).

Note that ERA-Interim has a resolution of T255 and the operational resolution at that time was T319. Initial data has been spectrally interpolated to the model resolutions.

The ERA-Interim analysis is an improvement over the original analysis which did not have as many observations. The scientific content of the IFS operational model at that time was significantly different to the more modern OpenIFS. A rough proxy for the how the forecast at the time performed would be to run OpenIFS at T255, the resolution of the initial data.

As OpenIFS is a spectral model, the 'T' number refers to the triangular truncation is spectral space. Equivalent grid-pt resolutions are:
T159 is approximately 125km resolution, T255 - 80km, T511 - 40km, T799 - 25km, T1279 - 16km.

Resolution	Expt id	Start date	Analysis	Filename	File size
T159L60	fqar	1999/12/24/12z	ERA-Interim	T159_1999122412_fqar.tgz	22Mb
T255L60	fqak	1999/12/24/12z	ERA-Interim	T255_1999122412_fqak.tgz	54Mb
T511L60	fqaj	1999/12/24/12z	ERA-Interim	T511_1999122412_fqaj.tgz	205Mb
T1023L60	fs2y	1999/12/24/12z	ERA-Interim	T1023_1999122412_fs2y.tgz	780Mb
T1279L60	fqaf	1999/12/24/12z	ERA-Interim	T1279_1999122412_fqaf.tgz	1.2Gb

To unpack files with .tgz, either use:

tar zxf T159_1999122412_fqar.tgz

or if your tar command does not support compression:

mv T159_1999122412_fqar.tgz T159_1999122412_fqar.tar.gz gunzip T159_1999122412_fqar.tar.gz tar xf T159_1999122412_fqar.tar

Resolution	Exp id	Start dates	Analysis	Filename	File size
T255	g8oz	1999/12, 14th-25th, 12z	ERA-Interim	T255_199912_14-25_g8oz.tar.bz2	660Mb
T511	g8su	1999/12, 14th-25th, 12z	ERA-Interim	T511_199912_14-25_g8su.tar.bz2	2.3Gb
T1279	g8t3	1999/12, 14th-25th, 12z	ERA-Interim	T1279_199912_14-19_g8t3.tar.bz2 T1279_199912_20-25_g8t3.tar.bz2	6Gb

These files use the 'bzip2' command rather than 'gzip', to achieve a better compression.

Uncompressing may take a long time depending on your system.

To uncompress:

bzip2 -d T255_199912_14-25_g8oz.tar.bz2
tar xf T255_199912_14-25_g8oz.tar

Download instructions

% mkdir -p runs/lothar/t159
% cd runs
% ftp ftp.ecmwf.int
ftp> cd case_studies/lothar_storm
ftp> binary
ftp> get 1999122412_T159_fqar.tgz
ftp> quit
% tar zxf 1999122412_T159_fqar.tgz
% ls
1999122412_T159.tgz  ICMCLfqarINIT  ICMGGfqarINIT  ICMGGfqarINIUA  ICMSHfqarINIT  ecmwf
% ls ecmwf
NODE.001_01  namelistfc

The 'ecmwf' directory contains the files as used at ECMWF to run this experiment:

namelistfc : copy this file to 'fort.4' to run the experiment (modify as required)
NODE.001_01 : this is the model output file as run at ECMWF. If your run fails, it may be useful to compare with this file.

Suggested sensitivity experiments

As ERA-Interim is an improved analysis, forecasts from these starting initial conditions will not reproduce the operational forecast of the storm. Because of changes to the forecasting system, this is impossible to do with OpenIFS. A proxy is to run the model at the same resolution as the ERA-Interim data (T255) as this is close to the resolution of the operational model of the time.

The IFS is highly tuned to give the best forecast over a range of initial conditions. However, it is instructive to try some sensitivity experiments to understand the role of various physical and dynamical processes.

What's the impact of the different 'lead times' on the forecast of the storm (i.e. starting from different dates)?
What's the impact of resolution on the forecast of the storm: both for it's development and impact over areas worse hit in Europe?
Reduce the timestep of the model - does this improve or worsen the forecast?
Reduce the gravity wave drag - how does this affect the forecast in the upper and lower levels?

Edit the source code to half the gravity wave drag coefficient

File: ifs/phys_ec/sugwd.F90, change:

Line 108: !  Revised gwd parameter values
Line 109: GKDRAG =0.15_JPRB

to:

Line 108: !  Revised gwd parameter values
Line 109: GKDRAG = 0.075_JPRB   !  half GWD coefficient: 0.15_JPRB

Increase the precipitation auto conversion rate - what impact does this have?

Edit the source code to increase the auto conversion rate by 20%

File: ifs/phys_ec/sucldp.F90, change:

line 123: RKCONV=1._JPRB/6000._JPRB   ! 1/autoconversion time scale (s)

to:

line 123: ! RKCONV=1._JPRB/6000._JPRB   ! 1/autoconversion time scale (s)
line 124: RKCONV=1.2_JPRB/6000._JPRB    ! default scaled by 20%: 1/autoconversion time scale (s)

Change the surface transfer coefficient in the turbulence scheme

Reduce the coefficient by 20%.

Alter surf/module/surfexcdriver_ctl_mod.F90 from :

line 671:  DO JL=KIDIA,KFDIA
line 672:    IF (JTILE == IFRMAX(JL)) THEN 
line 673:      PKHLEV(JL)=ZKHLEV(JL)
line 674:    ENDIF
line 675:  ENDDO

to:

line 671:  DO JL=KIDIA,KFDIA
line 672:    IF (JTILE == IFRMAX(JL)) THEN 
line 673:      PKHLEV(JL)=ZKHLEV(JL)
line 674:    ENDIF
    !  reduce surface transfer coeff by 20% in turbulence scheme
    !  for stockholm MSc course experiments
    ZCFMTI(JL,JTILE)=0.8_JPRB*ZCFMTI(JL,JTILE)
line 675:  ENDDO

Reduce (halve) the asymptotic mixing length scale (K)

For this change, two files need to be edited:

 line 53: RLAM   = 75.0_jprb  !! 150._JPRB: reduce to 75m

and:

 ZKLEN     = 75.0_jprb  !! 150.0_JPRB     ! asymptotic K length scale troposphere - Reduce to 75m

Lothar storm

Introduction

Initial conditions

Download instructions

Suggested sensitivity experiments

Further reading