1 Center for S a t ellite A pplications and R esearch (STAR) Applicability of GOES-R AWG Cloud Algorithms for JPSS/VIIRS AMS Annual Meeting Future Operational.

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Presentation transcript:

1 Center for S a t ellite A pplications and R esearch (STAR) Applicability of GOES-R AWG Cloud Algorithms for JPSS/VIIRS AMS Annual Meeting Future Operational Environmental Satellite Systems 25 January 2011 PRESENTED BY: Dr. Andrew Heidinger GOES-R Cloud Application Team Chair NOAA/NESDIS/STAR Advanced Satellite Products Branch

Motivation GOES-R AWG has developed algorithms for the same cloud properties slated for VIIRS. To date, many NPOESS cloud algorithms have not been tested and validated on global data. To date, the Government Team(s) have run into technical problems implementing NPOESS code. Based the above, the performance of some of the NPOESS algorithms remains unknown – this is a risk. It is therefore natural to ask: “Are the GOES-R AWG Cloud Algorithms Applicable to VIIRS?” We might need them to: – Serve as an alternative set of algorithms. – Serve as an additional source of data to help verify NPOESS data when available. 2

AWG Algorithm Strategy We propose to – use the existing NPOESS VIIRS Cloud Mask (VCM) which also provides cloud phase. – Implement the AWG Cloud Height Algorithm (ACHA) – Implement the Daytime Cloud Optical and Microphysical Properties (DCOMP) – Explore implementation of AWG cloud typing (M. Pavolonis/NOAA) – Explore implementation of nighttime cloud optical properties (NCOMP). 3

AWG Algorithm Description (1) DCOMP – Daytime Cloud Optical and Microphysical Products. – Products: Cloud Optical Depth, Cloud Particle Size and Cloud Water Path – Based on traditional method of retrieving cloud optical depth and particle size from non-absorbing and absorbing solar reflectance channels. – AWG code implemented using Optimal Estimation (OE) and provides pixel-level uncertainties. – Algorithm accounts for surface reflectance, molecular scattering and gaseous absorption. – Ice scattering tables provided by Professor Ping Yang. – Lead developer is Dr. Andi Walther – Currently implemented for AVHRR and GOES processing at NOAA. 4

DCOMP Spectral Considerations 5 Minimal spectral differences in channels available for DCOMP between VIIRS and ABI Baseline channel set for GOES-R AWG is 0.63 and 2.2  m (same as MYD06) DCOMP can operate on 1.6, 2.2 and 3.75  m channels. ABI VIIRS

AWG Algorithm Description ACHA – AWG Cloud Height Algorithm – Products: Cloud-top height, temperature and pressure. Cloud emissivity and IR microphysical index. – GOES-R ABI provides multiple IR windows with a H 2 O and CO 2 IR absorption bands. – The MODIS approach of CO 2 slicing is therefore not possible on VIIRS. – The ACHA code was been developed to handle multiple IR channel sets that includes those from AVHRR, GOES, VIIRS, ABI and MODIS. – On GOES-R, ACHA uses 11, 12, and 13  m channels. – On VIIRS, ACHA uses 8.5, 11 and 12  m channels – As with DCOMP, ACHA uses optimal estimation and provides pixel- level uncertainties. – Algorithm uses fast IR models (SSEC/PFAAST) and high resolution surface emissivity data bases (SEEBOR). – ACHA also provides cloud emissivity and IR microphysical estimates. – Currently implemented for AVHRR and GOES processing at NOAA NESDIS 6

ACHA Spectral Considerations 7 VIIRS lacks IR H 2 0 or CO 2 absorption channels. Notably, the ABI 13.3  m channel is missing ACHA on VIIRS uses all VIIRS longwave IR channels (except the 9.7  m O 3 channel) Heidinger et al (JGR,2010) explores the negative impact on cloud heights. ABI VIIRS

How Do We Test the Viability of GOES-R AWG Algorithms for VIIRS ? Test on MODIS as a VIIRS-proxy. Validate against – NASA MODIS cloud products provide a set of well-used data from state-of-the-art algorithms that provide a meaningful basis for comparison. – Active sensors (CALIPSO/CloudSat) provide direct measures of cloud profiles that provide more quantitative performance metrics for cloud-top height. 8

Prelaunch Processing Strategy 9 GRAVITE PEATE NPOESS VCM VIIRS SDR AWG VIIRS Cloud EDRs PEATE AWG VCM MODIS SDR AWG VIIRS Cloud EDRs Planned … Employed for this Work … PEATE = UW SSEC NPP Processing Infrastructure for NPP funded by NASA NGAS = Northrop Grumman Aerospace Systems (NPOESS Prime Contractor) Caveats: AWG VCM is not tuned for the VIIRS applications in contrasts to the NGAS VCM MODIS observations are used, not simulated VIIRS. AWG uses physical retrievals that account for spectral response of channels. This should not be an issue for this analysis.

COMPARISON TO NASA MODIS MYD06 CLOUD OPTICAL AND MICROPHYSICAL PROPERTIES 10

11 DCOMP Comparison to NASA MODIS MYD06 Products (One Granule 22:40 UTC on August 1, 2009) N A S A M O D I S P R O D U C T S ( M Y D 0 6 ) WATER PATH (g/m 2 ) EFFECTIVE RADIUS (  m) OPTICAL DEPTH A W G P R O D U C T S (D C O M P )

12 DCOMP Comparison to NASA MODIS MYD06 Products (Full Day – August 1, 2009)

13 DCOMP Comparison to NASA MODIS MYD06 Products (Full Day – August 1, 2009: Water Phase Clouds) Each circle provides the accuracy (mean bias) for this granule plotted at the center of the granule. Size of the circle indicate magnitude of the bias Color indicates sign of the bias Global distribution of all accuracy values for each granule. Granules with differences exceeding 2  m are rare.

COMPARISON TO NASA CALIPSO/CALIOP MYD06 CLOUD-TOP HEIGHTS 14

15 ACHA Comparison to NASA CALIPSO/CALIOP Products (One Granule 18:00 UTC on August 1, 2009)

16 ACHA Comparison to NASA CALIPSO/CALIOP Products (Full Day – August 1, 2009: All Clouds) Each circle provides the accuracy (mean bias) for this granule plotted at the center of the granule. Size of the circle indicate magnitude of the bias Color indicates sign of the bias Tropical errors due to multi-layer clouds. Global distribution of all accuracy values for each granule. Granules with errors larger than 2 km are rare.

Conclusions The VIIRS products based on GOES-R AWG algorithms are consistent with – NASA MODIS MYD06 cloud optical properties – NASA CALIPSO/CALIOP Lidar cloud-top heights. We will implement these two algorithms (DCOMP and ACHA) on VIIRS proxy data flowing from GRAVITE and on real VIIRS data when available. The algorithms will run concurrently during NPP. Data shown here is available for the asking. 17