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MODIS and VIIRS TEB Performance Chris Moeller, Greg Quinn University of Wisconsin MODIS/VIIRS Calibration Workshop November 18, 2019

MODIS and VIIRS TEB Performance · Ja124_2018-Nov05 2019 SNOs: N20 Avg VilRS - IASI A; All Bands M12 M13 M14 M15 M16 0.6 -0.6 200 220 VIIRS 240 260 280 (K) 300 Brightness Temp Mae,2012

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Page 1: MODIS and VIIRS TEB Performance · Ja124_2018-Nov05 2019 SNOs: N20 Avg VilRS - IASI A; All Bands M12 M13 M14 M15 M16 0.6 -0.6 200 220 VIIRS 240 260 280 (K) 300 Brightness Temp Mae,2012

MODIS and VIIRS TEB Performance

Chris Moeller, Greg Quinn

University of Wisconsin

MODIS/VIIRS Calibration Workshop

November 18, 2019

Page 2: MODIS and VIIRS TEB Performance · Ja124_2018-Nov05 2019 SNOs: N20 Avg VilRS - IASI A; All Bands M12 M13 M14 M15 M16 0.6 -0.6 200 220 VIIRS 240 260 280 (K) 300 Brightness Temp Mae,2012

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Terra MODIS (C6.1) SNOs with MetOp-A IASI

Page 3: MODIS and VIIRS TEB Performance · Ja124_2018-Nov05 2019 SNOs: N20 Avg VilRS - IASI A; All Bands M12 M13 M14 M15 M16 0.6 -0.6 200 220 VIIRS 240 260 280 (K) 300 Brightness Temp Mae,2012

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Aqua MODIS (C6.1) SNOs with MetOp-A IASI

Page 4: MODIS and VIIRS TEB Performance · Ja124_2018-Nov05 2019 SNOs: N20 Avg VilRS - IASI A; All Bands M12 M13 M14 M15 M16 0.6 -0.6 200 220 VIIRS 240 260 280 (K) 300 Brightness Temp Mae,2012

Switch to VIIRS V3 L1B

VIIRS – CrIS Comparisons

SNPP N-20

Page 5: MODIS and VIIRS TEB Performance · Ja124_2018-Nov05 2019 SNOs: N20 Avg VilRS - IASI A; All Bands M12 M13 M14 M15 M16 0.6 -0.6 200 220 VIIRS 240 260 280 (K) 300 Brightness Temp Mae,2012

VIIRS – CrIS Comparisons

SNPP N-20

A LUT correction is planned for N-20 L1B processing that will reduce scene temperature dependence.

Page 6: MODIS and VIIRS TEB Performance · Ja124_2018-Nov05 2019 SNOs: N20 Avg VilRS - IASI A; All Bands M12 M13 M14 M15 M16 0.6 -0.6 200 220 VIIRS 240 260 280 (K) 300 Brightness Temp Mae,2012

VIIRS – IASI Comparisons

SNPP N-20

A LUT correction is planned for N-20 L1B processing that will reduce scene temperature dependence.

Page 7: MODIS and VIIRS TEB Performance · Ja124_2018-Nov05 2019 SNOs: N20 Avg VilRS - IASI A; All Bands M12 M13 M14 M15 M16 0.6 -0.6 200 220 VIIRS 240 260 280 (K) 300 Brightness Temp Mae,2012

SNPP VIIRS SNOs with MetOp-A IASI

M12 M13I4

M14 M15 I5 M16

Page 8: MODIS and VIIRS TEB Performance · Ja124_2018-Nov05 2019 SNOs: N20 Avg VilRS - IASI A; All Bands M12 M13 M14 M15 M16 0.6 -0.6 200 220 VIIRS 240 260 280 (K) 300 Brightness Temp Mae,2012

N-20 VIIRS SNOs with MetOp-A IASI

M12 M13I4

M14 M15 I5 M16

Page 9: MODIS and VIIRS TEB Performance · Ja124_2018-Nov05 2019 SNOs: N20 Avg VilRS - IASI A; All Bands M12 M13 M14 M15 M16 0.6 -0.6 200 220 VIIRS 240 260 280 (K) 300 Brightness Temp Mae,2012

Summary

• Terra MODIS shows trending in PVLWIR (B27-30) that could be problematical for climate studies. Electronic Xtalk likely remains root cause.

• Aqua MODIS trends more stable but watching PVLWIR.

• SNPP VIIRS trending well.

• Some differences in biases between SNPP and N-20 VIIRS as a function of scene temperature.