Global Space-based Inter- Calibration System (GSICS)

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Global Space-based Inter- Calibration System (GSICS) Mitchell D. Goldberg NOAA/NESDIS Center for SaTellite Applications and Research (STAR) Satellite Meteorology and Climate Division 1

Motivation Applications are becoming more demanding Demanding applications require accurate, well calibrated & characterized measurements Reduce measurement uncertainty Growing global observing system 2

GEOSS GEOSS international coordinated effort to share Earth observations to provide a level of information about the Earth not previously achieved. 3

Nine Societal Benefits Improve Weather Forecasting Reduce Loss of Life and Property from Disasters Protect and Monitor Our Ocean Resource Understand, Assess, Predict, Mitigate and Adapt to Climate Variability and Change Support Sustainable Agriculture and Forestry and Combat Land Degradation Understand the Effect of Environmental Factors on Human Health and Well-Being Develop the Capacity to Make Ecological Forecasts Protect and Monitor Water Resources Monitor and Manage Energy Resources 4

Science Requirements for GEOSS to meet the 9 societal benefits: Satellite Intercalibration & Sensor characterization Data Fusion & Integrated Products, including CDRs Data Assimilation & Modeling 5

What is GSICS? Global Space-based Inter-Calibration System (GSICS) WMO sponsored Goal - Enhance calibration and validation of satellite observations and to intercalibrate critical components global observing system 6

GSICS formulation The GCOS Climate Monitoring Principles (GCMPs) were extended to address the problems associated with developing long-term climate data records from satellite observations Stable orbits Continuity and adequate overlap of satellite observations Improved calibration and validation CGMS tasked the WMO Space Programme to build an international consensus and consortium for a global space-based intercalibration system for the World Weather Watch (WWW)/Global Observing System (GOS). 7

Formulation Team Mitch Goldberg NOAA/NESDIS (Chair) Gerald Frazer NIST Donald Hinsman WMO (Space Program Director) Xu Jianmin (CMA) Toshiyuki Kurino (JMA) John LeMarshall - JC Sat. Data Assimilation Paul Menzel NOAA/NESDIS Tillmann Mohr WMO Hank Revercomb Univ. of Wisconsin Johannes Schmetz Eumetsat Jörg Schulz DWD, CM SAF William Smith Hampton University Steve Ungar CEOS, Chairman WG Cal/Val 8

Climate & Weather Requirements Need excellent accuracy and long-term stability Instruments must be inter-calibrated Need high precision (low noise) Measurements must be well characterized 9

Error Characteristics Accuracy (bias) y(t 2 ) p(t 2 ) Precision (standard deviation) a(t 2 ) a(t 1 ) p(t 1 ) Stability y(t 1 ) True y 10

GSICS Objectives To improve the use of space-based global observations for weather, climate and environmental applications through operational inter-calibration of satellite sensors. To provide for the ability to re-calibrate archived satellite data using the GSICS intercalibration system to enable the creation of stable long-term climate data sets To ensure that instruments meet specification, prelaunch tests are traceable to SI standards, and the onorbit satellite instrument observations are well calibrated by means of careful analysis of instrument performance, satellite intercalibration, and validation with reference sites 11

Space-based Observing Systems Operational Environmental Satellites 12

Outcome Coordinated international cal/val program Exchange of critical datasets for cal/val Best practices/requirements for monitoring observing system performance Best practices/requirements for prelaunch characterisation Establish requirements for cal/val Advocate for benchmark systems Quarterly reports of observing system performance and recommended solutions Improved sensor characterisation High quality radiances for NWP & CDRs 13

Prerequisites Extensive pre-launch characterization of all instruments traceable to SI standards Benchmark instruments in space with appropriate accuracy, spectral coverage and resolution to act as a standard for intercalibration Independent observations (calibration/validation sites ground based, aircraft) 14

Building Blocks for Satellite Intercalibration Collocation Determination and distribution of locations for simultaneous observations by different sensors (space-based and in-situ) Collocation with benchmark measurements Data collection Archive, metadata - easily accessible Coordinated operational data analyses Processing centers for assembling collocated data Expert teams Assessments communication including recommendations Vicarious coefficient updates for drifting sensors 15

GSICS Organizational Chart 16

GSICS Components GSICS Executive Panel reps from each operational satellite agency Priorities, objectives and agreements GSICS Coordination Center (GCC) - NESDIS Transmit intercalibration opportunities to GPRCs Collect data from the GPRCs and provide access Quarterly reports on performance GSICS Processing and Research Centers (GPRCs) Operational satellite agencies Activities: Pre-launch calibration Intersatellite calibration Supporting research 17

Calibration Support Segments (CSS) Pre-launch Instrument Characterization Earth-based Reference Sites and Natural Calibration Sources Extraterrestrial Calibration Sources Model Simulations Benchmark Measurements (space-based, aircraft, groundbased) 18

Web Interface to the Integrated Cal/Val System 19

Simultaneous Nadir Overpass (SNO) Method -a core component in the Integrated Cal/Val System POES intercalibration Unique capabilities developed at NESDIS Has been applied to microwave, vis/nir, and infrared radiometers for on-orbit performance trending and climate calibration support Capabilities of 0.1 K for sounders and 1% for vis/nir have been demonstrated in pilot studies Method has been adopted by other agencies Useful for remote sensing scientists, climatologists, as well as calibration and instrument scientists Support new initiatives (GEOSS and GSICS) Significant progress are expected in GOES/POES intercal in the near future GOES vs. POES20

Integrated Cal/Val System Architecture Calibration Opportunity Prediction Data Acquisition Scheduler Calibration Opportunity Register (CORE) Raw Data Acquisition for Calibration Analyses Stored Raw Data for Calibration Analyses SNO/ SCO Rad. Bias and Spectral Analysis Calibration Parameter Noise/ Stability Monitoring RTM Model Rad. at Calibration Reference Sites Intersensor Bias and Spectral Analysis Earth & Lunar Calibration Geolocation Assessment (Coastlines, etc.) Assessment Reports and Calibration Updates 21

Currently about 4 out of the 12 longwave channels meet the specification, including the important water vapor channel (ch12). NOAA18/HIRS is extremely sensitive to vibrations, due to a possible loose part in the aft optics, and the sensitive design with a 10 km resolution 22

AVHRR VIS/NIR Vicarious Calibration using the Libyan Desert Target NOAA 16 AVHRR Albedo NOAA 17 AVHRR Albedo CH1 CH2 CH3 Courtesy of X. Wu 23

AVHRR 0.86um channel (with vicarious calibration) N-16 coeff. update N-17 coeff. update 24

SNO Events Between Concurrently Operating AMSU-A Instruments Time Period: May 21, 2005 to July 31, 2006 Locations: Mainly Around 80 0 North and South SNO Time Threshold: 30 Seconds Number of SNOs: Aqua/ N15 Aqua/ N16 Aqua/ N18 N15/ N16 N15/ N18 N16/ N18 NH 63 57 58 57 60 54 SH 65 53 55 55 57 54 Globe 128 110 113 112 117 108 25

POES and Aqua AMSU-A SNO-ensemble Mean Biases and 99% Confidence Intervals GL SNO-ens. Mean Bias (K) 0.7 0.35 0-0.35 A) Aqua-N15 3 4 5 6 7 8 9 10 11 12 13 14 AMSU-A Channel GL SNO-ens. Mean Bias (K) 0.7 0.35 0-0.35 B) Aqua-N16 3 4 5 6 7 8 9 10 11 12 13 14 AMSU-A Channel GL SNO-ens Mean Bias (K) 0.7 0.35 0-0.35 C) Aqua-N18 3 4 5 6 7 8 9 10 11 12 13 14 AMSU-A Channel 26

Observed and Predicted AMSU-A SNO biases using Aqua/AMSU-A as a Calibration Transfer Radiometer Tb Bias (K) 0.75 0.5 0.25 0-0.25-0.5 3 4 5 6 7 8 9 10 11 12 13 14 AMSU-A Channel Avg N15-N18 Avg (Aqua-N18)- (Aqua-N15) Tb Bias (K) Tb Bias (K) 0.75 0.5 0.25 0-0.25-0.5 0.75 0.5 0.25 0-0.25-0.5 3 4 5 6 7 8 9 10 11 12 13 14 AMSU-A Channel 3 4 5 6 7 8 9 10 11 12 13 14 AMSU-A Channel Avg N15-N16 Avg (Aqua-N16)- (Aqua-N15) Avg N16-N18 Avg (Aqua-N18)- (Aqua-N16) 27

Understanding Global Biases and Developing Calibration Algorithms for Bias Correction SSMIS (54.4 GHz) SSMIS is the first conical microwave sounding instrument, precursor of NPOESS CMIS. Shown are the differences between observed and simulated measurements. Biases are caused by 1) antenna emission, 2) direct solar heating to warm load and 3) stray light contamination to its calibration targets. 28

AIRS Noise Monitoring 29

Fantastic AIRS - MODIS Agreement for Band 22 (4.0μm)! AIRS Tb (K) AIRS minus MODIS (K) CIMSS AIRS Histogram MODIS Uniform Scenes Selected 30

MODIS Band 22 (4.0μm) AIRS-MODIS mean = -0.05 K Little Dependence on Scene Temperature Little Dependence on X-track View Angle Little Dependence on Solar Zenith Angle 31

Shifting MODIS Band 35 (13.9 μm) by 0.8 cm -1 Works to Remove Mean bias and Scene Tb Dependence No Shift MODIS shifted Tb diff (K) AIRS-MODIS: un-shifted, shifted (ce (0.21K) not included here) 32

8 AIRS FOVs and SHIS Data w/in them (448 fovs) used in the following comparisons 33 1 Degree

comparison 3 AIRSobs SHISobs (AIRSobs-AIRScalc) (SHISobs-SHIScalc) (AIRSobs-AIRScalc)- (SHISobs-SHIScalc) wavenumber 34

TWP versus ECMWF (ECMWF averaged over ~10-40 deg. Latitude) (Strow, UMBC) 35

Frost-Point Observations Show Significant Deviations Frost-Point Observations by H. Voelmer: NOAA Boulder Represents far fewer observations than RS- 90 s and inconsistencies day vs night. ν (cm -1 ) ν (cm -1 ) Diamonds are CO 2 Biases for channels with similar peaking weighting functions. 36

Summary GSICS - coordinated effort to better characterise and improve the fundamental measurements of the Global Observing System Improve radiance quality >>>reduce uncertainties in forecasts and climate data records 37

WMO has approved the development of an Implementation Plan Co-ordination Group of Meteorological Satellites (CGMS) XXXIII WMO- WP-21 presented a draft concept and strategy for a Global Space-based Inter-calibration System (GSICS) Action 33.15: CGMS Members to establish a Task Force lead by NESDIS (Mitch Goldberg) with participation by EUMETSAT (Johannes Schmetz), JMA (Toshiyuki Kurino), CMA (Xu Jianmin) and assisted by the WMO Space Programme to prepare a draft Implementation Plan for GSICS by 1 July 2006 for review by CGMS Members by 1 August 2006 and approval at CGMS XXXIV. 38

ORA Satellite Cal/Val Program Road Map (2005-2012) Science Advance By 2012, Global Environmental Observation System of Systems (GEOSS) data will be calibrated with a high quality for uses in the environmental data stewardship Resources: OK Deficiency Integrate DMSP, GOES and EOS into sensor performance monitoring Develop FY-3 series, METOP-A IASI and GOME2 calibration algorithms which are part of cal/val system Integrate validation efforts to form prototype cal/val system Integrated cal/val enterprise system that delivers to WMO and other users SNO data. Develop NPP, NPOESS and GOES-R calibration algorithms which are part of Cal/Val New cal/val sites deployed for GEOSS and GHG products More product validation using existing validation sites will lead to robust products in NOAA operational products such as temp/water profiles in storm conditions DMSP microwave sounding instrument bias and anomaly correction algorithms are incorporated. GOES and EOS An inter-sensor calibration system for monitoring sensor performance NOAA POES instrument on-board performance can be monitored with intersensor and intra-sensor calibration, radiative transfer simulations. The anomaly can be captured in near-real time and the instrument biases can be corrected Individual POES/GOES sensor calibration Establish a basic infrastructure for operational POES instrument calibrations through onboard calibrators and vicarious technique for quantifying instrument noise and linear and non-linear calibration. 2005 2007 2009 2010 2011 2008 2006 39 2012

Global Ocean, Day and Night, BIAS 40

International TOVS Study Conference, 15 th, ITSC-15, Maratea,Italy, 4-10 October 2006 Madison, WI, University of Wisconsin-Madison, Space Science and Engineering Center, Cooperative Institute for Meteorological Satellite Studies, 2006.