GPM Microwave Radiometer Vicarious Cold Calibration

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Presentation transcript:

GPM Microwave Radiometer Vicarious Cold Calibration Rachael Kroodsma UMD ESSIC / NASA GSFC rachael.a.kroodsma@nasa.gov Kroodsma GSICS meeting 2014/08/26

Kroodsma GSICS meeting 2014/08/26 Outline Motivation GPM inter-calibration Dissertation Work Inter-calibration algorithm development Vicarious cold calibration Current Work GMI calibration analysis Inter-calibration uncertainty analysis Kroodsma GSICS meeting 2014/08/26

Global Precipitation Measurement (GPM) Use multiple radiometers on individual platforms to measure global precipitation Goal: global measurements every 3 hours GPM X-Cal group is responsible for developing inter-calibration algorithms Original focus on microwave imagers More recent focus on microwave sounders Core observatory launched! February 28, 2014 3:37 JST Kroodsma GSICS meeting 2014/08/26

GPM Microwave Imager (GMI) GMI turned on March 4 Public data release June 16 Over 2 months ahead of requirement (6 months after launch) Next reprocessing on September 2 Clean up many of the anomalies seen in the current GMI data GMI calibration is looking very good Kroodsma GSICS meeting 2014/08/26

Microwave Imagers for GPM constellation Radiometer Frequency (GHz) Nominal EIA (degrees) Orbital Inclination (degrees) Local Crossing Time (asc) WindSat 10.7V 10.7H 18.7V 18.7H 23.8V 23.8H 37.0V 37.0H 49.9-55.3 98.7 6:00pm AMSR-E 10.65V 10.65H 36.5V 36.5H 89.0V 89.0H 55 98 1:30pm SSM/I   19.35V 19.35H 22.235V 85.5V 85.5H 53.1 98.8 6:00pm – 9:00pm TMI 21.3V 53.3 (post-boost) 35 -- SSMIS 91.655V 91.655H 98.9 6:00pm – 8:00pm AMSR2 MADRAS 53.5 20 GMI 36.64V 36.64H 52.8 65 Kroodsma GSICS meeting 2014/08/26

GPM X-Cal Algorithm GMI TMI X-Cal inter-calibration algorithm: Each team calculates a double difference (DD) between the target and reference radiometers Combine teams’ results into one value at the cold end and one at the warm end Assume linear dependent calibration between cold and warm TBs Algorithm ~1 year after launch Current GPM Inter-Calibration Algorithm GMI TMI SSMIS F16 GMI TMI TMI AMSR2 SSMIS F17 SSMIS F19 SSMIS F18 Kroodsma GSICS meeting 2014/08/26

University of Michigan’s Contribution: Vicarious Cold Calibration Kroodsma GSICS meeting 2014/08/26

Vicarious Cold Inter-Calibration Algorithm* GDAS inputs Freq/pol, EIA Radiative transfer model Radiometer ‘A’ TB data Simulated TB data for ‘A’ Vicarious cold calibration algorithm Observed cold cal TB Simulated cold cal TB Obs cold cal TB – Sims cold cal TB Repeat for radiometer ‘B’ ‘A’ Single difference ‘B’ Single difference ‘A’ single diff – ‘B’ single diff Double difference for ‘A’ and ‘B’ *R. A. Kroodsma, D. S. McKague, and C. S. Ruf, “Inter-calibration of microwave radiometers using the vicarious cold calibration double difference method,” J. Selected Topics Remote Sensing, vol. 5, no. 3, pp. 1006-1013, 2012. Kroodsma GSICS meeting 2014/08/26

Calculate Cold Cal TB from Histograms One month of over-ocean TB observations Each channel: Freq/pol ……….. 19H 21V 37V ……….. Hemispheres NH SH Orbits Channel and scan positions are radiometer-specific. asc des Scan Position ……….. 70 71 72 ……….. Kroodsma GSICS meeting 2014/08/26

Simulate Radiometer TBs and Calculate Cold Cal TB AMSR-E Observed 23.8V TBs Simulated 23.8V TBs GDAS SST, wind, water vapor, cloud liquid water and temp profiles Lat/Lon, scan time TB (K) EIA, freq RTM TOA TB Difference from match-up inter-calibration method: we simulate all over-ocean TBs for vicarious cold calibration, not just those in the match-up regions. Kroodsma GSICS meeting 2014/08/26

Observed (obs) and Simulated (sims) Cold Cal TB Comparison TB Histograms 23.8V NH monthly cold cal TB Sims cold cal TB matches obs seasonal cycle Warm tail in obs due to rain 10.65V SH des cold cal TB Sims cold cal TB matches obs scan position variation Cold end shape of histograms look similar Kroodsma GSICS meeting 2014/08/26

Single Difference (SD) [Obs – Sims] Cold Cal TB 23.8V NH monthly SD 10.65V SH des SD SD accounts for frequency, EIA, and geophysical variability *Considered a relative calibration* Kroodsma GSICS meeting 2014/08/26

Double Difference (DD) AMSR-E – TMI DD Average 1 year of DDs to derive the inter-calibration values Kroodsma GSICS meeting 2014/08/26

Contribution to GPM X-Cal: AMSR2 – TMI UM results show good agreement Kroodsma GSICS meeting 2014/08/26

Current Work: GMI Calibration Analysis Kroodsma GSICS meeting 2014/08/26

GMI Calibration Analysis Use the vicarious cold calibration single difference (SD) to analyze GMI calibration [Obs – Sims] cold cal TB Relative calibration Time dependent SD Calibration stability over time Scan dependent SD Identify scan biases Kroodsma GSICS meeting 2014/08/26

Kroodsma GSICS meeting 2014/08/26 GMI Time Dependent SD Cold cal TB calculated using 7 days of data. Only scan positions 50-150. All channels show a relatively stable calibration w.r.t. time Kroodsma GSICS meeting 2014/08/26

GMI Time Dependent SD: Asc/Des splits Splitting into asc/des orbits shows a very apparent yaw dependent calibration at some channels (10.65V/H and 36.5V) Kroodsma GSICS meeting 2014/08/26

GMI Asc SD – Des SD by Yaw Nonzero value indicates an asc/des calibration dependency. 10.65V/H and 36.5V show the largest deviations from zero. Note that 10.65H is opposite from 10.65V and 36.5V. Kroodsma GSICS meeting 2014/08/26

GMI Scan Dependent SD by Yaw 10.65 and 36.5 channels show some yaw dependent scan biases. Significant scan dependent biases in 10.65H. Kroodsma GSICS meeting 2014/08/26

Wentz et al. 2001: TMI scan biases Initial TMI calibration showed some significant scan biases. Except for the 10.65H channel, GMI scan biases look very good by comparison. Plus, we have been able to identify the source of many of the scan anomalies seen in GMI data and can remove them. Kroodsma GSICS meeting 2014/08/26

X-Cal Consensus Inter-Cal: GMI – TMI 10v 10h 18v 18h 23v 36v 36h 89v 89h Cold DD 3.9 3.0 2.8 2.2 1.1 2.0 0.8 0.9 @Temp 160 85 180 100 190 200 130 250 Warm DD 5.2 5.0 4.1 2.6 1.5 1.3 -- 285 283 288 286 282 281 Notes: Using GMI 1C V03A and TMI 1B11 v7 89 GHz channel is a constant offset at all temperatures These numbers may change with the next reprocessing (GMI V03B) Kroodsma GSICS meeting 2014/08/26

Current Work: Inter-Calibration Uncertainty Kroodsma GSICS meeting 2014/08/26

Vicarious Cold Inter-Calibration Algorithm* Sources of Error GDAS inputs Freq/pol, EIA Radiative transfer model Radiometer ‘A’ TB data Simulated TB data for ‘A’ Vicarious cold calibration algorithm Observed cold cal TB Simulated cold cal TB Obs cold cal TB – Sims cold cal TB Repeat for radiometer ‘B’ ‘A’ Single difference ‘B’ Single difference ‘A’ single diff – ‘B’ single diff Double difference for ‘A’ and ‘B’ *R. A. Kroodsma, D. S. McKague, and C. S. Ruf, “Inter-calibration of microwave radiometers using the vicarious cold calibration double difference method,” J. Selected Topics Remote Sensing, vol. 5, no. 3, pp. 1006-1013, 2012. Kroodsma GSICS meeting 2014/08/26

Double Difference Sensitivity to RTM Surface emissivity models: Elsaessar (current) and RSS Atmospheric absorption: Rosenkranz (current) and MonoRTM Ancillary data: GDAS (current) and ERA-I DDs are found for the following 5 cases using 2013 data for SSMIS F17 and AMSR2 compared with TMI. Case 1: GDAS inputs, Elsaessar surface model, Rosenkranz atmosphere Case 2: GDAS inputs, RSS surface model, Rosenkranz atmosphere Case 3: GDAS inputs, Elsaessar surface model, MonoRTM atmosphere Case 4: ERA-I inputs, Elsaessar surface model, Rosenkranz atmosphere Case 5: ERA-I inputs, Elsaessar surface model, MonoRTM atmosphere Kroodsma GSICS meeting 2014/08/26

Double Differences for 5 Cases DD spread (K) of 5 cases Channel A2-TMI F17-TMI 10v 0.08 -- 10h 0.04 19v 0.11 0.10 19h 0.12 21v 0.69 0.57 37v 0.16 0.07 37h 0.06 85v 0.34 0.32 85h 0.70 0.67 Kroodsma GSICS meeting 2014/08/26

Kroodsma GSICS meeting 2014/08/26 Summary Initial check-out of GMI looks good Vicarious cold calibration shown to be a useful tool for analyzing calibration GMI will be ready to be used as the reference radiometer for GPM 1 year of data is desired before adding it to the constellation X-Cal has recently started to focus on calculating uncertainties for inter-calibration Preliminary analysis has shown sensitivity of water vapor and high frequency channels to water vapor profile assumptions and atmospheric absorption models Kroodsma GSICS meeting 2014/08/26