Ocean Break-out Summary MODIS Science Team Meeting 9 May 2012 Bryan Franz and the MODIS Ocean Science Team.

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Presentation transcript:

Ocean Break-out Summary MODIS Science Team Meeting 9 May 2012 Bryan Franz and the MODIS Ocean Science Team

R Multi-Mission Ocean Color Reprocessing Highlights: consistent algorithms and methods for all sensors** incorporated enhanced knowledge of sensor characterization** regenerated all sensor-specific tables and coefficients improved aerosol models based on AERONET additional correction for NO2, improved turbid water atmos. corr. Status: SeaWiFS completed September 2010 OCTS completed September 2010 MODIST completed January 2011 MODISA completed June 2011 CZCS completed August 2011 Scope: MODISA, MODIST, SeaWiFS, OCTS, CZCS

MODISA Rrs in good agreement with SeaWiFS Deep-Water solid line = SeaWiFS R dashed = MODISA R Rrs (str -1 ) & & & 670

MODIST Rrs in good agreement with SeaWiFS Deep-Water solid line = SeaWiFS R dashed = MODIST R Rrs (str -1 ) & & & 670

Chlorophyll spatial variation in good agreement SeaWiFS MODIS/AquaMODIS/Terra Fall 2002

Chlorophyll spatial variation in good agreement SeaWiFS MODIS/AquaMODIS/Terra Fall 2008

Chl a in Good Agreement with Global In situ SeaWiFS vs in situ MODISA vs in situ

Global Chlorophyll Timeseries Oligotrophic Subset Mesotrophic Subset SeaWiFS MODISA MODIST

Global Chlorophyll Timeseries Oligotrophic Subset Mesotrophic Subset SeaWiFS MODISA MODIST MERIS

SeaWiFS

MERIS

50% 30% 20% 10% 60% MODISA Lunar and Solar Calibration Trends More Erratic in 2011 MODIS 412nm Responsivity Changes Since Launch 0% Gain Solar 40% Lunar

MODISA R Temporal Anomalies ( ) Rrs(443)Rrs(547) Chlorophyll Deep-Water Big Trending Errors in 2011

Degraded Timeseries Quality in 2011 Oligotrophic Subset Mesotrophic Subset SeaWiFS MODISA MODIST MERIS

New Temporal Calibration Approach MCST final calibration for Collection 6 uses Earth view data lunar calibration + desert observations for 412 and 443 largely reproduces previous SeaWiFS cross-cal results (validation!) But still not quite good enough for ocean color significant residual time-trend at 412 (due to scan-edge changes) residual cross-scan and striping artifacts

C6 Calibration introduced trend in 412 fixed 50% increase in Rrs at 412nm induced downward trend

Significant Temporal Trend in Rrs(412) i ntroduced after MCST C6 desert-based calibration

New Temporal Calibration Approach MCST final calibration for Collection 6 uses Earth view data lunar calibration + desert observations for 412 and 443 largely reproduces previous SeaWiFS cross-cal results (validation!) Additional cross-scan correction developed by OBPG relative to MCST C6 desert-based calibration based on contemporaneous Aqua L3 15-day Rrs derive time-varying RVS shape per detector & mirror-side applied to all OC bands But still not quite good enough for ocean color significant residual time-trend at 412 (due to scan-edge changes) residual cross-scan and striping artifacts See talk by Gerhard Meister this afternoon

OBPG MODISA Cross-Scan Corrections at 412nm relative to MCST desert-based C6 calibration Gain Scan Pixel 412nm, Detector 5, Mirror-Side Mission Time

OBPG MODISA Cross-Scan Corrections relative to MCST desert-based C6 calibration 412nm443nm 488nm531nm Mission Time Gain

MODISA R Temporal Anomalies ( ) Rrs(443)Rrs(547) Chlorophyll Deep-Water Much Better! consistent with expectation

MODIS Reprocessing New approach for temporal calibration of MODIS-Aqua ocean color time-series is now fully independent of SeaWiFS MODIS-Aqua Reprocessing starting this week only change is to temporal calibration and vicarious adjustment level-2 processing completed Sunday (10 years in 5 days, 700x!) MODIS-Terra has similar issues relies heavily on SeaWIFS for temporal RVS and polarization waiting for "final" MCST C6 calibration cross-calibrate Terra to Aqua to resolve polarization sensitivity Both MODIS sensors are beyond design life maintaining quality is an on-going challenge, user beware

Terra MODIS SST V6 V6 Algorithm has coefficients derived for zonal intervals (Latband). This removes regional and seasonally repeating bias errors Following initial problems in first year of mission, instrument and SST retrievals are very stable. Time series of median uncertainties of Terra MODIS 4 µm night-time SSTs, relative to drifting buoys, in six latitude bands. Minnett & Evans

Uncertainties in MODIS SSTs Best rms uncertainties in 4µm SST is <0.3K wrt drifting buoys. But buoy accuracies are ~0.25K, so MODIS is more accurate than can be demonstrated. To improve this situation: – new generation of drifters being developed and deployed – target ~0.01K uncertainties –2 nd generation ARGO profilers, uncertainties ~0.001K –2 nd generation of M-AERIs, uncertainties <0.1K

Significant differences between SI & non- SI uncertainties ? Ship radiometer measurements Laboratory water-bath blackbody calibrator Satellite- derived SSTs and uncertainties SI-traceable thermometers Laboratory calibration Matchup analysis of non- SI collocated measurements CDR of SST SI Traceable uncertainty budget Derivation of SST from satellite measurements Multi-year satellite radiometer measurements Non-SI traceable in situ measurements Matchup analysis of SI collocated measurements SI-standard blackbody calibrator Non – SI Traceable uncertainty budget Radiometric characterization e.g. NIST TXR Y N

Balch: Many major cruises to study coccolithophores- both northern and southern hemisphere; sampled over >120,000 km… Arctic’11 SW Pacific’11 Patagonian Shelf’08 S. Ocean’11 S. Ocean’12 SOGasEx’10 AMT GNATS’98-’12

Shipboard PIC algorithm refinement continues (we have almost doubled the explained-variance globally). This plot illustrates the relative importance of PIC to total particle backscattering (b bp )… Sub-tropical gyres Temperate Polar Sub-Polar Tropical PIC-dependent backscattering total particle backscattering [Chlorophyll a] (mg m -3 )

Question from Paula Should we be organized around measurements or missions?

Question from Paula Should we be organized around measurements or missions? MODISA MERIS MODIST SeaWiFS MOS OSMI OCM OCM2 MOS OSMI OCM OCM2 PACE VIIRS

Question from Paula Should we be organized around measurements or missions? Oligotrophic Subset SeaWiFS MODISA MODIST MERIS VIIRS

Question from Paula Should we be organized around measurements or missions? a mission meeting should focus on instrument calibration, data quality, and interdisciplinary algorithms a mission meeting should focus on instrument calibration, data quality, and interdisciplinary algorithms

Current MODIS OC Standard Product Suite 1.R rs ( ) 2.Ångstrom 3.AOT 4.Chlorophyll a 5.K d (490) 6.POC 7.PIC 8.CDOM_index 9.PAR 10.iPAR 11.nFLH Level-2 OC Product Gordon and Wang 1994, Ahmad et al 2010, etc. O'Reilly et al (OC3) updated to NOMADv2 Werdell (KD2) algorithm (similar to OC3) Stramski et al Balch et al. 2005, Gordon et al Morel and Gentili 2009 Frouin et al Behrenfeld et al Algorithm Reference R rs (412) R rs (443) R rs (469) R rs (488) R rs (531) R rs (547) R rs (555) R rs (645) R rs (667) R rs (678)

Current MODIS Evaluation Products Euphotic Depth (Lee et al. and Morel et al.) Zeu_lee, Zeu_morel Spectral Diffuse Attenuation (Lee et al.) Kd_412_lee, Kd_443_lee, Kd_490_lee (using QAA) Diffuse Attenuation of PAR ( Morel et al.) Kd_PAR Inherent Optical Properties (Maritorena et al. and Lee et al.) adg_443_lee, bbp_443_lee, aph_443_lee, a_443_lee (QAA) ** adg_443_gsm, bbp_443_gsm, chl_gsm (GSM) ** ** also in support of MEASURES (Maritorena)

412 Trend Isolated to Scan Edges Scan angles (frame): lunar (22), nadir (675), Solar diffuser (989), end-of-scan (1250)

Generating SST Climate Data Records Climate Data Records (CDRs) of SST require an unbroken chain from the derived SST fields to SI standards. Drifting buoys are not traceable to SI calibration after deployment, but matchups between MODIS SSTs and drifters are numerous. Ship-board radiometers are traceable to SI standards through the NIST TXR (transfer radiometer) at a series of workshops at RSMAS. Matchups between MODIS SSTs and radiometers are less numerous. Following slides show how to generate SST CDRs using both buoys and radiometers (long version & short version).

Significant differences between SI & non-SI uncertainties ? CDR of SST SI Traceable uncertainty budget Multi-year satellite radiometer measurements of SST Non – SI Traceable uncertainty budget Y N