Preliminary After-launch GOCI Characterization: Inter-slot radiance discrepancy issue

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Preliminary After-launch GOCI Characterization: Inter-slot radiance discrepancy issue Young-Je Park*, Hee-Jeong Han, Seongick Cho, Joo-Hyung Ryu, Jae-Hyun Ahn and Yu-Whan Ahn Korea Ocean Satellite Center, Korea Ocean Research and Development Institute Presented at IGARSS 2011, Vancouver, Canada

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Preliminary After-launch GOCI Characterization: Inter-slot radiance discrepancy issue. Young-Je Park*, Hee-Jeong Han, Seongick Cho, Joo-Hyung Ryu , Jae-Hyun Ahn and Yu- Whan Ahn Korea Ocean Satellite Center, Korea Ocean Research and Development Institute - PowerPoint PPT Presentation

Transcript of Preliminary After-launch GOCI Characterization: Inter-slot radiance discrepancy issue

Page 1: Preliminary After-launch GOCI Characterization:  Inter-slot radiance discrepancy issue

Preliminary After-launch GOCI Characterization:

Inter-slot radiance discrepancy issue

Young-Je Park*, Hee-Jeong Han, Seongick Cho, Joo-Hyung Ryu, Jae-Hyun Ahn and Yu-Whan Ahn

Korea Ocean Satellite Center, Korea Ocean Research and Development Institute

Presented at IGARSS 2011, Vancouver, Canada

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Objectives

• To understand the inter-slot radiance discrepancy issue

• To seek ideas/suggestions on how to approach this GOCI specific issue

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Sensors have specific issues

• MODIS stripe noise– detector calibration– difference in mirror side characteristics– Sensitivity to polarization state

• MERIS– SMILE effects: wavelength variation – Discontinuity at some camera interface

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Outline

• Overview of the GOCI optical system and image acquisition sequence

• Inter-slot discrepancy: – variability within a slot– variability across different slot boundaries– variability with observation hours (0, 3, 7 hours)– How RT simulations show

• Image smoothing technique• Future directions

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GOCI sensor

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GOCI optical layout

Three Mirror Anastigmatic Telescope

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GOCI slots imaging sequence

Target Area

20,00

25,00

30,00

35,00

40,00

45,00

50,00

110,00 115,00 120,00 125,00 130,00 135,00 140,00 145,00 150,00Longitude (deg)

Lat

itude

(deg

)

P1 (+Y,-Z)P2 (+Y,+Z)

P3 (-Y,+Z)

P4 (-Y,-Z)

Slot 1

Slot 16

Slot 4

Slot 5Slot 8

Slot 9 Slot 12

Slot 13

P6

P5P7

P8

1 2 3 4

56

16

9

8 7

15 14 13

121110

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Imaging procedure for a GOCI slot

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Nominal time intervals for GOCI operation

• Interval between bands = ~ 8 seconds• Interval between consecutive L1a slots = ~ 103

seconds• Duration for acquiring one GOCI image = ~ 103*16

seconds = 27 minutes• Interval between consecutive GOCI images = one hour• Interval between the adjacent slots in L1B scene = up

to ~103*7 seconds or 12 minutes => sun angle difference??

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Requirements for comparing radiances from two slots

• Accurate geometric registration• Spatially homogenous conditions for the

atmosphere and water are preferred, which is to avoid seeing different air/water mass from two different slots

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Inter-slot discrepancy

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Variability within a slot

• 20110330_0h image: slot 3-6 border

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Variability across different slot boundaries

• 20110330-3h

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Inter-slot discrepancy: spectral aspect(033003)

• Slot #2-7 border

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Inter-slot discrepancy: spectral aspect(033003)

• Slot #3-6 border

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• Slot #4-5 border

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• Slot #5-12 border

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• Slot #6-11 border

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• Slot #7-10 border

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• Slot #8-9 border

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• Slot #9-16 border

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• Slot #10-15 border

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Variability with observation hour

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Slot border reflectance change

• Within a slot border: moderately variable with consistent difference spectra

• For different slot borders: variable magnitude, moderately variable spectra

• For different observation hours: larger difference (lower reflectance for the upper slot) in the 7h image

• Bands 7 & 8 reflectance ratio changes significantly, which has a serious effect on atmospheric correction that uses those bands.

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How does RT code simulate the discrepancies?

uslot=3,lslot=6: 3099,1584 3099,1585lat,lon= 41.0020866 131.8832245sunz= 54.8425102 54.0042229suna= 121.0095673 122.2263718senz= 47.5428658 47.5378571sena= 185.6037445 185.6040649

uslot=3,lslot=6: 3099,1592 3099,1593lat,lon= 40.9659882 131.8822021sunz= 37.4894829 37.5132179suna= 180.6660614 182.7969666senz= 47.5027428 47.4977188sena= 185.6062317 185.6065369

uslot=3,lslot=6: 3099,1597 3099,1598lat,lon= 40.9434242 131.8815613sunz= 65.5979691 66.5323486suna= 252.3380127 253.3214874senz= 47.4776611 47.4726372sena= 185.6077881 185.6080933

• 0h: 9hr local time

• 3h: 12hr local time

• 7h: 17hr local time

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Simulation with AOT550=0.1

400 450 500 550 600 650 700 750 800 850 900-0.004

-0.003

-0.002

-0.001

0

0.001

0.002

0h3h7h

wavelength (nm)

TOA

refle

ctan

ce d

ifere

nce

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Simulation with AOT550=0.5

400 450 500 550 600 650 700 750 800 850 900-0.004

-0.003

-0.002

-0.001

0

0.001

0.002

0h3h7h

wavelength (nm)

TOA

refle

ctan

ce d

ifere

nce

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GOCI data

400 450 500 550 600 650 700 750 800 850 900-0.008

-0.006

-0.004

-0.002

0

0.002

0.004

0.006

0h3h7h

wavelength (nm)

TOA

refle

ctan

ce d

ifere

nce

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An image smoothing technique

• Distance-to-border weighted average– Applied to overlapped area– Simple and good for image generation– Smoothing the TOA reflectance data will not be

good for downstream data processing including the atmospheric correction.

– Smoothing the geophysical parameters would make sense.

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Distance-to-border weighted average

d1

Slot i

d2

d3

d4

Slot i

wi

wi = min(d1,d2,d3,d4) where is number of pixels to the k-th border

Slot j

wj

N’=∑(wi Nⅹ i)/∑wi

N’: weighted averageNi: reading from the ith slot

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Example 1 (original)GOCI 20110412-07h, South Japan

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Example 1 (weighted average)GOCI 20110412-07h, South Japan

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Future work

• Clarify questions of – Is it an issue of the GOCI radiometric calibration?– Is it an issue of the band filter properties?– Is it an issue of the ghost image?

• Develop a scientifically based model to correct the inter-slot discrepancy. Bands6,7,8 are critical for atmospheric correction.

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Thank you!

Please contact us if you have any idea on this issue.

[email protected]