Atmospheric Motion Vectors from Kalpana-1: An ISRO status

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Atmospheric Motion Vectors from Kalpana-1: An ISRO status Sanjib Kr. Deb, Inderpreet Kaur, C. M. Kishtawal and P. K. Pal Atmospheric and Oceanic Sciences Group Space Applications Centre Indian Space Research Organization, Ahmedabad, India E-mail: sanjib_deb@sac.isro.gov.in 20-24 February 2012 Eleventh International Winds Workshop, Auckland, New Zealand

Contents: Current and future Indian Geostationary/LEO satellites. ISRO AMV retrieval algorithm. Improvement in Height assignment. Recent improvement in retrieval algorithm. Validation statistics with radiosonde. Spatial error analysis NCEP GFS. Conclusion Future directions. Few slides with latest status of OSCAT winds

ISRO missions and geophysical parameter retrieval & cal-val ongoing activities Kalpana-1 2002 INSAT-2E/3A (1999/2003) INSAT-3D (2012) INSAT-3D R Geo-HR( ~2013) G E O VHRR VHRR, CCD 6-Ch VHRR IR Sounder F o l l o w - u p (~2015) CMV, OLR, Rainfall, AMV AMV, OLR, Rainfall Aerosol SST, AMV, OLR, Rainfall, T, h Profile L E O OCEANSAT 1/2 (1999/2009) Vector Winds Aerosol, T & h Profille MSMR, OCM, Scatterometer ROSA SARAL (2012) SSH, Waves, Winds Altimeter MEGHA-TROPIQUES (20) MW Imager, WV Sounder, ScaRaB GPS-RO SS Wind, TWV, Rainfall T, h Profile, Radiation Budget

Current Indian Geostationary Meteorological Satellites Satellites INSAT-3A (2003) KALPANA-1 (2002) Location 93.5E 74E Payloads VHRR & CCD VHRR VHRR bands (µm): Visible 0.55-0.75 (2 km x 2 km) WV 5.70-7. (8 km x 8 km) TIR.5-12.5 (8 km x 8 km) Visible 0.55-0.75 (2 km x 2 km) WV 5.70-7. (8 km x 8 km) TIR.5-12.5 (8 km x 8 km) CCD Camera (µm): Visible 0.62-0.68 (1 km x 1 km) NIR 0.77-0.68 (1 km x 1 km) SIR 1.55 1.69 (1 km x 1 km) VHRR= Very High Resolution Radiometer CCD = Charged Couple device (for agriculture related studies)

INSAT 3D (Launch schedule: July/2012) 6 Channel IMAGER 19 Channel SOUNDER Spectral Bands (µm) Visible : 0.55-0.75 Short Wave Infra Red : 1.55-1.70 Mid Wave Infra Red : 3.80 4.00 Water Vapour : 6.50-7. Thermal Infra Red 1 :.30 -.30 Thermal Infra Red 2 :.50-12.50 Resolution : 1 km for VIS, SWIR 4 km for MIR, TIR 8 km for WV Spectral Bands (µm) Short Wave Infra Red : Six bands Mid Wave Infra Red : Five Bands Long Wave Infra Red : Seven Bands Visible : One Band Resolution (km) : X for all bands No of simultaneous : Four sounding per band

INSAT Meteorological Data Processing System (IMDPS) Ongoing: (Using Kalpana-1 & INSAT-3A data) - Rainfall - Atmospheric Mo.on Vectors (AMV). - Outgoing Long-wave Radiation (OLR) - Upper Tropospheric Humidity (UTH) - Sea Surface Temperature (SST). - Cyclone Track, Intensity - Monsoon Monitoring - Now-casting (Activities: Retrievals and Applications) - NWP impact through assimilation. - Assimilation of WV radiances (NWP) Future: (Using INSAT 3D data) - Rainfall, - SST, AMV, UTH, OLR - Fire & Smoke, - Fog, - Aerosol Optical Depth, - Snow - Temp & Humidity profile, - Total Ozone. - Merged rainfall product (Polar & Geo) - Cyclone track and intensity. - Now-casting - NWP impact through assimilation - Assimilation of WV radiances

ISRO AMV winds retrieval activities Started in 2006/2007 time frame with the initiation of IMDPS project Image Triplet (IR and WV) Tracer selection (Local variance / anomaly) Tracking ( Nash- Sutcliffe model efficiency) Height Assignment using Genetic Algorithm Quality Control (EUMETSAT- QI) Calculate winds from two pairs of images Winds were generated only at 00 & 12 UTC, when 30-min. full disc image triplet were available. Final winds with height and QI Other time image frequency was 1-hour. References: 1. S. K. Deb, C. M. Kishtawal, P. K. Pal and P. C. Joshi, A modified tracers selection and tracking procedure to derive winds using water vapor imagers, 2008, Jour. Appl. Meteor. Clim, 47 (12), 3252-3263. 2. C. M. Kishtawal, S. K. Deb, P. K. Pal and P. C. Joshi, Estimation of atmospheric motion vectors from Kalpana-1 imagers, 2009, Jour. Appl. Meteor. Clim. 48 () 24-2421.

Height Assignment (Empirical Algorithm) Verification in heights Randomly choose large number of Meteosat7 images and corresponding EUMETSAT winds Training using GA Generate an independent relationship for tracer height for MET7 images using BT of coldest, warmest pixels and latitude information A mapping is defined between Meteosat7 and kalpana-1 using SRF Calculate final optimized function for tracer height in Kalpana images Main drawbacks An ad-hoc method. Tries to re-produce operational height assignment of Meteosat7, with its own limitations. Needs further training for other satellites, since the mapping is sensitive to satellite SRF. Don t use NWP forecast as background. This is where ISRO-CIMSS collaboration has come up in 20/20.

Improvement in Height assignment - Collaboration with CIMSS/SSEC - (Chris Velden & his group) Implemented following height assignment techniques in ISRO Algorithm Infrared window technique (WIN). H 2 O Intercept Method. (Nieman et. al 1993) Cloud Base Method (BASE). (LeMarshall et. al 1993) Few gross error checks. RMSVD 9.5 8.5 7.5 6.5 5.5 4.5 IR Winds TRIP_GA TRIP_NEW MET7_CIMSS Jan- Feb- Mar- Apr- May- Jun- HIGH-Level 14 12 8 6 4 IR Winds TRIP_GA TRIP_NEW MET7_CIMSS Jan- Feb- Mar- Apr- May- Jun- MID-Level IR Winds LOW-Level WV Winds HIGH-Level 9 8 7 6 5 4 3 TRIP_GA TRIP_NEW MET7_CIMSS Jan- Feb- Mar- Apr- May- Jun- 9.5 8.5 7.5 6.5 5.5 4.5 TRIP_GA TRIP_NEW MET7_CIMSS Jan- Feb- Mar- Apr- May- Jun- All the above validation is with radiosonde in region [ 30E -130E; 50S 50N] Reference: S. K. Deb, Steve Wanzong, C. S. Velden, Inderpreet Kaur, C. M. Kishtawal, P. K. Pal and W. P. Menzel, Height Assignment improvement in Kalpana-1 Atmospheric Motion Vectors, 20, submitted to Remote Sensing Lett.

Improvement in retrieval algorithm Use of full disc image is replaced with sector generated image with improved registration and fixed lat/lon co-ordinate. Take advantage of using multiple 30-min images, rather than traditional 3 images. The study (Kaur et al. 20) for finding the temporal scales of satellite derived atmospheric winds over Asian Monsoon region has shown that Minimum Decorrelation time scale in AMV is ~ 4 hours. Based on the above study we take winds retrieved from previous 8-images (i.e. 7 sets of winds using 2-image at a time) as support for current time retrieval. Details in the Session-2 presentation References: Inderpreet Kaur, C. M. Kishtawal, S. K. Deb and Raj Kumar, Temporal Scales of Satellite Derived Atmospheric Winds over the Asian Monsoon Region., 20, Published online 26 October 20: DOI:.19/LGRS.20.2167494 IEEE. Trans. Remote Sens. Letters

Validation statistics with radiosonde RMSVD IR Winds HIGH-Level IR Winds MID-Level 9.5 8.5 7.5 TRIP_GA TRIP_NEW M ULP_NEW M ET7_CIM SS 14 12 TRIP_GA TRIP_NEW M ULT_NEW M ET7_CIM SS 6.5 8 5.5 6 4.5 Jan- Feb- Mar- Apr- May- Jun- 4 Jan- Feb- Mar- Apr- May- Jun- IR Winds LOW-Level WV Winds HIGH-Level TRIP_GA TRIP_NEW M ULT_NEW M ET7_CIM SS 9.5 TRIP_GA TRIP_NEW M ULT_NEW M ET7_CIM SS 9 8 7 8.5 7.5 6 6.5 5 4 3 Jan- Feb- Mar- Apr- May- Jun- 5.5 4.5 Jan- Feb- Mar- Apr- May- Jun- Note: Retrieval algorithm and resolution of Kalpana-1 & Meteosat7 are different.

Statistics: Average of all 17 months Filters: Hor. Dist. < 1 Km Vert. Dist. < 25 hpa Speed Diff. < 30 m/s Dir Diff. < 60 deg AMV Speed > 2.5 m/s Approx. 7-9% of total collocations are affected due to these filters.

Examples Kalpana-1/ISRO Infrared winds valid at 26 May 20 12 UTC Meteosat-7/CIMSS - Thanks to CIMSS for Met7 winds

Kalpana-1/ISRO Water vapor winds valid at 26 May 20 12 UTC Meteosat-7/CIMSS - Thanks to CIMSS for Met7 winds

- Thanks to UKMO website Spatial error analysis with NCEP GFS analysis HIGH Level IR winds comparisons Period: September 20 Kalpana-1 Meteosat-7 Kalpana-1 Meteosat-7 Bias MVD RMSVD (Normalized) Collocations

- Thanks to UKMO website MID Level IR winds comparisons Period: SEPT20 Kalpana-1 Bias MVD Meteosat-7 Kalpana-1 Meteosat-7 RMSVD (Normalized) Collocations

LOW Level IR winds comparisons Period: SEP20 Bias MVD Kalpana-1 Meteosat-7 Kalpana-1 Meteosat-7 RMSVD (Normalized) Collocations - Thanks to UKMO website

HIGH Level WV winds comparisons Period: SEPT20 Bias MVD Kalpana-1 Meteosat-7 Kalpana-1 Meteosat-7 RMSVD (Normalized) Collocations - Thanks to UKMO website

Conclusions: Statistical analysis shows significant improvement after implementation of new height assignment and some positive impact for new retrieval algorithm. However more improvement is required to match with accuracies of other operational agencies. Spatial error analysis resembles well with UKMO error analysis for Met7. Future directions: Expect some more improvement with incorporation of auto editor. Optimization in tracer selection. To retrieve winds from visible and 3.9 µm channel. Wish to collaborate with other operational agency for further improvement.

OSCAT: ISRO Status

OSCAT Valida,on: Latest version released on 15 th December 20 OSCAT with Sta,s,cs of OSCAT comparison with Buoys, Model and ASCAT for 4-24 m/s Temporal Difference No. of collocated data Wind speed Wind direction Bias RMSE Bias RMSE Buoy 30 min 539 0.091 1.393-0.447 21.261 ASCAT 3 hr 9,78,455 0.19 1.14 0.49 18.39 ECMWF 6 hr 29290996 0.018 1.439-0.69 17.16 NCEP 6 hr 33951459-0.076 1.754-0.46 18.83 Source: OSCAT ISRO validation team

Parameters Analysed Wind Products 1. Wind Speed Magnitude (m/s) 2. U-component of Wind (m/s) 3. V-component of Wind (m/s) 4. Wind stress (Pa) 5. Zonal wind stress (Pa) 6. Meridional wind stress (Pa) 7. Wind Divergence (s^-1) 8. Curl of wind stress (Pa/m) Total 3 Files for each Product -Source: Rajkumar & Abhishek Chakraborty (rksharma@sac.isro.gov.in) Daily 3 Products: 50 Km resolu,on 2 Products of 12 Hourly Analysed Winds for 0-12 and 12-24 UTC 1 Product of Daily Analysed Winds 1) Binary File O2SCT_25MAY20_DAILY_L04_AWV50.grd (~8MB) for Daily 2) Log File O2SCT_25MAY20_DAILY_L04_AWV50.Log (~1KB) 3) Wind GIF File O2SCT_25MAY20_DAILY_L04_AWV50.gif (~39KB) For 12 Hourly and O2SCT_25MAY20_0600_L04_AWV50.grd for 00-12 UTC O2SCT_25MAY20_1800_L04_AWV50.grd for 12-24 UTC

Analysed winds Daily using OSCAT ; 12 Hrly using OSCAT & ASCAT

Daily Analysed wind Products using OSCAT (Stress, Curl, Div.)

Fine features resolved by High Resolu,on OSCAT winds during Cyclone MERBOK - Source: B. S. Gohil & Rajesh Sikhakolli (bsgohil@yahoo.com)

L2B Winds High Res winds

Acknowledgement EUMETSAT for financial support for attending IWW SSEC/CIMSS for scientific collaboration. IWW organizing committee for all support. Director and Associate Director SAC/ISRO for all support. EUMETSAT/CIMSS/UKMO for using their AMV products and analysis report.