NWP SAF: Deliverable 8
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Regional use of locally received ATOVS radiances in NWP
R. Randriamampianina1 and F. Rabier2
(1) Hungarian Meteorological Service, Budapest, Hungary, (2) Météo-France, Toulouse, France
Abstract We investigated the impact of locally received and pre-processed ATOVS radiances in the French global model, ARPEGE over Europe. The ARPEGE model uses stretched geometry emphasizing the European area with the finest resolution over France. Thus, the impact of locally received ATOVS data in an area where the model has fine resolution could be investigated. ARPEGE uses a four- dimensional variational assimilation system and assimilates pre-processed ATOVS radiances. In the experiments, runs with HIRS+AMSU-A and AMSU-A only were performed. The benefit of increased resolution data was investigated as well. The impacts of locally pre-processed ATOVS radiances with those of NESDIS (BUFR-120km) on different ranges forecast were compared at each assimilation time (00, 06, 12 and 18 UTC). The majority of the locally pre-processed ATOVS data from NOAA-16 became available for the assimilation within a relatively short time (short cut-off: 1h50 at 00 and 12 UTC and 3h at 06 and 18 UTC) compared to data sent by NESDIS. Positive impact on the forecast of the locally pre-processed ATOVS data compared to that of NESDIS was found in most of the cases. Assimilation of pre- processed in Lannion data with relatively finer resolution gave strong positive impact on the forecast compared to the finer resolution data, pre-processed by NESDIS.
Introduction This work was performed in the framework of NWP SAF. The NWP SAF (Satellite Application Facility) intends to improve and support the interface between satellite data/products and European activities in global and regional NWP (Numerical Weather Prediction). The NWP SAF supports scientific processes (rather than products) such as: research on observation operator (e.g. radiative transfer models), investigation of shared monitoring, development of pre-processing software (e.g. AAPP), and studies on retrieval software (e.g. ICI) (English, 2000). The objective of our study was to investigate the use and impact of locally received and pre- processed ATOVS (Advanced TIROS Operational Vertical Sounder) radiances in the French global model, ARPEGE over Europe. The impact of locally received ATOVS data was studied in an area where the model has fine resolution. ARPEGE uses a four-dimensional variational assimilation scheme and assimilates pre-processed ATOVS radiances.
System environment – the ARPEGE model The global numerical weather prediction model used operationally at Météo-France is the stretched version of the ARPEGE/IFS system developed in collaboration between Météo-France and ECMWF (European Centre for Medium-Range Weather Forecasts) (Courtier et al. 1991). ARPEGE uses a stretched geometry (stretching factor is 3.5) emphasizing the European area with the finest resolution over France around 19 km and 234 km at the Antipodes. At the time of this study, in 2001, the model had a truncation of 199 wave numbers and 31 hybrid coordinate vertical levels from the surface up to about 5 hPa. The forecast ranges were 96, 72, 42 and 36 hours at 00, 12, 6, 18 UTC, respectively. Since 20 June 2000, a four-dimensional variational (4D-Var) assimilation system has been used at Météo-France as an operational analysis system. It is similar to the ECMWF 4D-Var system (Rabier et al. 1998) with some differences linked to some operational constraints such as multi-incremental technique, weak constraint initialisation using digital filters and use of simplified physics in the minimization process (Janisková et al. 1999). The operational assimilation scheme of ARPEGE assimilates pre-processed TOVS/ATOVS radiances (BUFR-120km) from NESDIS (National Environmental Satellite Data and Information Service) globally. These data are received at 120km resolution but are used only at 250km resolution. The current analysis scheme consists of applying a one-dimensional variational (1D-Var) assimilation system to the pre-processed radiances to obtain quality control flags, vertical profiles of temperature, humidity and surface temperature. The radiances are then injected into 4D-Var together with the surface temperature and retrieved profiles above the top of the model (Rabier et al. 2001). Short cut- off times, used for the operational forecasts are as short as 1h50 after the analysis times at 0 and 12 UTC, as opposed to 3h at 6 and 18 UTC. Long cut-off used for the assimilation suite is 8h10 after the analyses times at 0 and 12 UTC and 6h15 at 6 and 18 UTC.
Processing of radiances -Observation processing The Spatial Meteorological Centre (CMS) of Météo-France in Lannion produces pre-processed ATOVS radiances (level 1d) for the Western European area (45W, 30N, 40E, 70N). Since pre- processed radiances from the CMS are not treated operationally in Toulouse, we had to provide a chain of conversion of the data format from BUFR to CMA. It consisted, mainly, of the adaptation of the existing code such that we would be able to treat locally pre-processed data from NOAA (National Oceanic and Atmospheric Administration) Satellites in accordance with the following particularities of our experiments: - Choice of Satellite: Due to the failure of the AVHRR instrument on NOAA-15, those data were not pre-processed at CMS during the study period. The only data we used in this study are then those from NOAA-16. - Extraction of data according to cut-off times: Posterior extraction of data from the database was possible only according to the time of their observation. We were interested in data, received before the cut-off time. Consequently, some adjustments were done to be able to extract data according to their arrival time in the database. Due to these modifications, posterior simulation of operational runs became available. - The pre-processed NESDIS data were extracted for the “Lannion reception area” only, with the same cut-off conditions, as for data from Lannion. - When starting the experiments the amount of Lannion pixels, selected in the analyses, was found to be much less than that of NESDIS. Analysing the spatial distribution of the pixels it was shown, that it did not only come from differences in cloudy pixel distributions. We found out that besides the land-sea flag, the Lannion data contained coastline information. The pixels at the coastline could not be identified by 1D-VAR and were handled as bad ones. Coastline pixels were taken as over land to avoid this problem.
-Description of the experiments The following seven experiments were performed for the period of May 22 - June 11, 2001: 1- model run without any radiance data (reference run) – (CONV) 2- experiments with assimilation of Lannion radiance data, using: 2a: infrared + microwave (A-unit) radiances, 250 km res. – (LAN) 2b: data of microwave A-unit only, 250 km resolution – (LAN4) 2c: data of microwave A-unit at finer, 120 km resolution – (LAN3) 3- experiments with assimilation of NESDIS radiance data, using: 3a: infrared + microwave (A-unit) radiances, 250 km res. – (NES) 3b: data of microwave A-unit only, 250 km resolution – (NES4) 3c: data of microwave A-unit at finer, 120 km resolution – (NES3)
The experiments with assimilation of advanced microwave (AMSU) data only (LAN4 and NES4) were set to examine the impact of radiances independently. Experiments LAN3 and NES3 using 120 km resolution were performed to study the impact of finer resolution data. The assimilation times were 00, 06, 12 and 18 hours. Forecasts were archived at each assimilation time every 12 hours up to 96 hours for both, short and long cut-offs. The short and long cut-offs were maintained as in the operational scheme. -Bias correction The comparison of observed and modelled radiances reflect the presence of systematic errors (Eyre et al. 1993) arising mainly from errors in the radiative transfer model, instrument calibration problems or biases in the model fields. Biases related to deficiencies in the radiative equation are air-mass dependent. Bias correction coefficients for NOAA-16 data have been computed according to the method developed by Harris and Kelly (2001). It contains a dual bias correction with respect to the scan position as well as to the air-mass. Bias correction coefficients for NESDIS data were available from the operational runs, but they referred to the whole globe. We recalculated them to have bias correction coefficients specific for the study area only. The outputs of the operational runs were used as background information to compute the modelled radiances.
-Channel selection The bias of the brightness temperature specific for each channel was analysed to select the useful channels. The list of the chosen channels and the corresponding standard deviations (STDEV) are shown in Table 1. Radiances at the edge of the orbit (3 pixels from both edges) are not used in the operational assimilation scheme to avoid “strong” angular bias, so we did not use them either.
Table 1: List of chosen channels and the corresponding standard deviations
CHANNELS PIXELS HIRS AMSU-A 2 3 4 5 6 7 8 10 11 12 13 14 15 5 6 7 8 9 10 11 Clear 0.35 0.30 0.20 0.30 0.40 0.60 1.00 0.80 1.10 1.50 0.50 0.35 0.30 0.30 0.20 0.20 0.20 0.25 0.30 0.40 Cloudy 0.35 0.30 0.30 0.20 0.20 0.20 0.25 0.30 0.40
-Statistics of the Observations The statistics of observation (ATOVS radiances) minus guess (computed radiances) and observation minus analysis were calculated to control the data use efficiency (see Figures 1.a-b as an example). The efficiency of the AMSU was found to be very small in the experiments using Lannion data when setting the standard deviations for each channel as in the operational suite.
a) b)
AMSU-A RMS (Clear pixels) HIRS RMS (Clear pixels) Short cut-off Short cut-off ch 8 ch 9 ch10 ch11 ch 1 ch 2 ch 3 ch 4 ch 5 ch 6 ch 7 ch 8 ch 9 ch10 ch11 ch12 ch13 ch14 ch15 ch 5 487 ch 6 487 ch 7 487 1730 1730 1730 1730 0 1356 1356 1338 1338 1338 481 481 0 481 1338 1336 481 481 481 ch 5 ch 6 ch 7 ch 8 ch 9 ch10 ch11 ch 1 ch 2 ch 3 ch 4 ch 5 ch 6 ch 7 ch 8 ch 9 ch10 ch11 ch12 ch13 ch14 ch15 1584 1584 1584 1967 1967 1967 1967 0 1649 1649 1649 1649 1647 1520 1520 0 1520 1647 1641 1520 1520 1520 0.50 3.00 2.50 0.40 2.00 K
. K 0.30 1.50 . g g e e d
d 0.20 1.00 0.10 0.50 O-B_NES4 O-A_NES4 O-B_LAN4 O-A_LAN4 0.00 0.00 O-B_NES O-A_NES O-B_LAN O-A_LAN -0.50 Channels number and pixels amount Channels number and pixels amount (upper Lannion, lower NESDIS) (upper Lannion, lower NESDIS) Figure 1: Example of the statistics of the observation minus guess (O-B) (solid line) and observation minus analyses (O-A) (dashed line) for AMSU-A (left) and for HIRS (right). Thick lines represent results of data from Lannion while thin lines that of NESDIS (BUFR-120km).
The computed mean square error is the sum of the observation and background mean square errors, so it should be bigger than the theoretical one, but was found to be much smaller in case of AMSU-A (Advanced Microwave Sounding Unit-A) pre-processed in Lannion. Based on this experience we reduced the theoretical STDEV values of the Lannion AMSU-A channels, dividing them by 1.5, for their more efficient use. The main difference between the pre-processing of ATOVS data is the antenna correction, applied for data form Lannion but not for the BUFR-120km from NESDIS (T. Reale, personal communication). Impact study -Amount of pixels used in the experiments The mean amount of pixels, used in the experiments with the advanced microwave (AMSU) channels for different assimilation and cut-off times is presented in Figure 2. Satellite ID was used to get pixel amount information.
A: Short cut-off B: Long cut-off 160 250 AMSU-A Lannion AMSU-A Lannion 140 AMSU-A NESDIS AMSU-A NESDIS s s l 200 l
e 120 e x x i i p
100 p
f 150 f o o
80 r r e e
b 100 60 b m m u
40 u N N 50 20 0 0 00 06 12 18 00 06 12 18 assimilation time in hours assimilation time in hours (45W, 40E, 70N, 30N) Figure 2: Number of AMSU-A pixels used in the Lannion reception area; average on 21 days
In the short cut-off the amount of available pixels was the largest at 06h for both Lannion and NESDIS, and there were many pixels at 12h as well. Very few Lannion data were available at 00h and 18h, while there were no NESDIS data at 00h at all. Twice as many Lannion and NESDIS pixels were available at 12h in the long cut-off than in the short one. The amount of Lannion pixels remained the same at 06h and 18h, and increased almost 3 times at 00h. The amount of NESDIS pixels was much bigger in the long cut-off at 00h, 06h and 12h, than that of the short cut-off, and did not change for the 18h assimilation time. The periodical absence of Lannion data at 00 and 18 hours could be explained by the fact that these orbits are at the edge of Lannion reception area and either not detected or relatively small and not processed. On the other hand NESDIS uses full orbits that we cut at the "Lannion window", so these data are available at the edges as well.
-Forecast verification The verification of the forecasts was performed by comparing them with their own analyses as well as independent information – radiosonde profiles (TEMP). The main observation time of the TEMP profiles is 00h and 12h. Consequently, relatively small amount of TEMP profiles was available at 06 and 18 hours. The root mean square error (RMSE) values were calculated to compare the impact of pre-processed ATOVS data on the forecast. For example, "NES-LAN" means the difference between the RMSE values, calculated from the NES and LAN experiments. After checking the general tendencies we moved towards more and more detailed investigations: 1, Impact study using analysis as a reference (layer by layer and horizontal distribution) 2, Impact study using radiosonde (TEMP) profiles as a reference (vertical and temporal distributions) Scores were computed for the studied area only – Europe and Eastern Atlantic.
Results In general, positive impact of both, Lannion and NESDIS data against CONV data on forecasts of geopotential was found. Further analyses concerned comparisons of the impacts of Lannion and NESDIS data on the forecast. - Impact study using TEMP profiles as a reference Impact according to the cut-off time
Slight positive impact of Lannion data was observed until 48-60h forecast range (Figure 7b) when using all available data (long cut-off) (quality different). A positive impact of the LAN and LAN4 data on the forecast in the short cut-off (quality and quantity different) case could be observed (Figure 7a) for almost the entire forecast range. Note that in operative practice data, arrived within the short cut- off time are used in the forecast while data, received during the long cut-off are applied for background field computation. Furthermore, at 06UTC, there are less TEMP data and their geographical distribution is less uniform than that of analyses. Thus, these results are less representative. a) RMSE (NESDIS-Lannion)
-100 -100
-200 -200
-300 ) -300 ) a a P P h h ( ( ) ) -400 -400 1 1 - - * * ( (
s s l
l -500 -500 e e v v e e l l
s l -600 l -600 e e d d o o M -700 M -700
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-1000 -1000 0 24 48 72 96 0 24 48 72 96 Forecast ranges (hours) Forecast ranges (hours) b) RMSE (NESDIS-Lannion) Figure 7: Impact of the Lannion data compared to the NESDIS ones in short (a) and long
-100 -100
-200 -200
) -300 -300 a ) a P P h ( h
(
) -400 ) -400 1 1 - - * * ( (
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-1000 -1000 0 24 48 72 96 0 24 48 72 96 Forecast ranges (hours) Forecast ranges (hours) (b) cut-offs at 06UTC assimilation time with HIRS and AMSU-A (left) and AMSU-A only (right). Patterns with positive values are coloured. Impact of other parameters on the forecast Slight (mostly positive) impact of LAN and LAN4 data on the temperature, humidity and wind forecasts was found. - Impact study using analysis as a reference The pre-processed in Lannion HIRS (High resolution Infrared Sounder) and AMSU-A (LAN) data and AMSU-A data only (LAN4) had a strong positive impact on geopotential above 200 hPa against the NESDIS data. In general, slight positive impact on geopotential was found below 200 hPa. The positive impact could be seen from the 48h forecast range in case of LAN (Figure 3) and from 24h range in case of LAN4 (Figure 4). The impact was slightly reduced in case of long cut-offs. Neither positive, nor negative valuable impact on other parameters was detected.
32 RMSE (m) 500 hPa 27 AMSU-A Nes AMSU-A Lan 22
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12 Forecast ranges (h) 7 12 24 36 48 60 72 84 96 Figure 3: Comparison of the forecasts RMSE (m) for the geopotential height of the run with HIRS and AMSU-A in short cut-off at 06UTC assimilation time. (dashed- run with data from Lannion, solid line- run with data from NESDIS) The forecasts were compared with their own analyses.
32 RMSE (m) 500 hPa 27 HIRS+AMSU-A Nes HIRS+AMSU-A Lan 22
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12 Forecast ranges (h) 7 12 24 36 48 60 72 84 96
Figure 4: Comparison of the forecasts RMSE (m) for the geopotential height of the run with AMSU-A in short cut-off at 06UTC assimilation time. (dashed- run with data from Lannion, solid line- run with data from NESDIS) The forecasts were compared with their own analyses
The horizontal distribution of the impact of Lannion data against NESDIS ones over the studied area is demonstrated in Figure 5. The LAN4 data have positive impact on larger territories than that of NES4 data; there are more patterns with positive than negative impacts. The same conclusions can be drawn comparing the impacts of LAN and NES data over sea, but quite mixed picture was observed over land. Figure 5: Horizontal distribution of the impact of the Lannion data against NESDIS data. NES4-LAN4 on the left: run with AMSU-A for 48h forecast range in short cut-off at 06UTC assimilation time. NES-LAN on the right: run with HIRS and AMSU-A for 72h forecast range in short cut-off at 06UTC assimilation time. The forecasts were compared with their own analyses. Patterns with positive values are coloured
Impact on data with finer resolution Figure 6. shows the impact of finer (120 km) resolution Lannion and NESDIS data on the forecast, in terms of RMSE. The Lannion data at finer resolution (LAN3) was found to give more positive impact on the forecast against the 250 km resolution Lannion data (LAN4), than the "finer" NESDIS data (NES3) against the 250 km NESDIS data (NES4). In case of data, pre-processed in Lannion strong positive impact, compared to NESDIS data, could be observed below 100 hPa level at all forecast ranges.
37 RMSE (m) 500 hPa 32 AMSU-A Nes (thin. 120km) 27 AMSU-A Lan (thin. 120km)
22
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12 Forecast range (h) 7 12 24 36 48 60 72 84 96 Figure 6: Comparison of the forecasts RMSE (m) for the geopotential height of the run with AMSU-A assimilated in finer resolution (thinning distance 120km) (dashed- run with data from Lannion, solid line- run with data from NESDIS) in short cut-off at 06UTC assimilation time. The forecasts were compared with their own analyses.
Conclusions 1, The AMSU-A data pre-processed in Lannion seem to have better quality than that of NESDIS. It possibly comes from the antenna correction, applied for data from Lannion but not for those from NESDIS. 2, The majority of the locally pre-processed ATOVS data from NOAA-16 became available for the assimilation within a relatively short time (short cut-off: 1h50) compared to those sent by NESDIS. Thus, comparing the impact on the forecast of data pre-processed by NESDIS with that of Lannion, the positive impact of the latter was larger in the short cut-off than in the long cut- off, because we received data from Lannion more quickly. 3, Using TEMP profiles as a reference the impact of data pre-processed in Lannion was positive, compared to that of NESDIS data in most of the cases; the positive impact of AMSU-A Lannion data compared to AMSU-A NESDIS data was more evident than that of HIRS + AMSU-A data, due to differences in calibration techniques for HIRS data. 4, Comparing the impact of data with and without radiances on the forecast and using their analyses as a reference we found, that data pre-processed in Lannion had a slight but clear positive impact compared to the ones, pre-processed by NESDIS. The impact was well defined above 200 hPa level and for the geopotential height and less clear for the other (wind, temperature and humidity) parameters. These conclusions are for both, system with valid HIRS+AMSU-A and with AMSU- A only. 5, Positive impact on the forecast of Lannion data compared to that of NESDIS was only clear at 06UTC in general, probably because relatively small amount of data and from the NOAA-16 only was used. Moreover, 06UTC was the only synoptic time when a large amount of data was located upstream of Europe. We would expect more positive impact if data of two satellites would be used. 6, Assimilation of data with relatively finer, 120 km resolution gave strong positive impact on the forecast of data, pre-processed in Lannion compared to the ones, pre-processed in NESDIS.
Perspective At the Hungarian Meteorological Service, we started the implementation of ATOVS radiances in the 3D-Var assimilation system of the limited area model ALADIN.
References English S. 2000: The NWP SAF. A satellite application facility for numerical weather prediction. Proceedings of the HMS – Eumetsat Training Course, 4-9 December, 2000, Budapest, Hungary. CD available Eyre J. R., 1993: A bias correction scheme for simulated TOVS brightness temperatures. ECMWF Technical Memorandum, 186. Available from ECMWF. Courtier P., Freydier C., Geleyn J.-F., Rabier F. and Rochas M., 1991: The ARPEGE project at Météo- France. Proceedings of the ECMWF seminar on “Numerical Methods in Atmospheric Models”, 193-232. Reading, 9-13 September 1991. Available from ECMWF. Harris B. A. and Kelly G., 2001: Satellite radiance bias correction scheme for radiance assimilation, Q.J.R. Meteorol. Soc., 127,1453-1468. M. Janisková, J-N. Thépaut and J-F. Geleyn, 1999: Simplified and regular physical paramterizations for incremental four-dimensional variational assimilation. Monthly Weather Review, Vol. 127., 26-45. Rabier, F., Thépaut, J.-N. and Courtier, P., 1998: Extended assimilation and forecast experiments with a four-dimensional variational assimilation system. Q. J. R. Meteorol. Soc., 124, 1861- 1887. Rabier F., Puech D. and Benichou H., 2001: Monitoring and assimilation of ATOVS data at Météo- France. Proceedings of the Eleventh International TOVS Study Conference, Budapest, Hungary. 20-26 Sep. 2000
Acknowledgments The authors want to thank the SAF NWP project and the EUMETSAT for the support of this study. We are very grateful to the Météo-France for hosting this work. This work was partially supported by the Hungarian National Research Foundation (OTKA- T 032466) as well. The help of the colleagues from CNRM/GMAP and CNRM/COMPAS is highly acknowledged. In particular, we would like to thank J. Barckicke for the preparation of the 4D-var scripts; P. Caille for the contribution in data processing; F. Pouponneau and Z. Liu for their help in quick graphical comparison of the results. The fruitful discussions with J. Pailleux, P. Moll, E. Gérard, P. Brunel, L. Lavanant, T. Reale and M. Dahoui are very much appreciated.