1 / 44

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

zarifa
Download Presentation

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

An Image/Link below is provided (as is) to download presentation Download Policy: Content on the Website is provided to you AS IS for your information and personal use and may not be sold / licensed / shared on other websites without getting consent from its author. Content is provided to you AS IS for your information and personal use only. Download presentation by click this link. While downloading, if for some reason you are not able to download a presentation, the publisher may have deleted the file from their server. During download, if you can't get a presentation, the file might be deleted by the publisher.

E N D

Presentation Transcript


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

  2. Objectives • To understand the inter-slot radiance discrepancy issue • To seek ideas/suggestions on how to approach this GOCI specific issue

  3. 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

  4. 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

  5. GOCI sensor

  6. GOCI optical layout Three Mirror Anastigmatic Telescope

  7. GOCI slots imaging sequence 1 2 3 4 8 7 6 5 9 10 11 12 16 15 14 13

  8. Imaging procedure for a GOCI slot

  9. 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??

  10. 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

  11. Inter-slot discrepancy

  12. Variability within a slot • 20110330_0h image: slot 3-6 border

  13. Variability across different slot boundaries • 20110330-3h

  14. Inter-slot discrepancy: spectral aspect(033003) • Slot #2-7 border

  15. Inter-slot discrepancy: spectral aspect(033003) • Slot #3-6 border

  16. Slot #4-5 border

  17. Slot #5-12 border

  18. Slot #6-11 border

  19. Slot #7-10 border

  20. Slot #8-9 border

  21. Slot #9-16 border

  22. Slot #10-15 border

  23. Variability with observation hour

  24. 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.

  25. How does RT code simulate the discrepancies? uslot=3,lslot=6: 3099,1584 3099,1585 lat,lon= 41.0020866 131.8832245 sunz= 54.8425102 54.0042229 suna= 121.0095673 122.2263718 senz= 47.5428658 47.5378571 sena= 185.6037445 185.6040649 • 0h: 9hr local time uslot=3,lslot=6: 3099,1592 3099,1593 lat,lon= 40.9659882 131.8822021 sunz= 37.4894829 37.5132179 suna= 180.6660614 182.7969666 senz= 47.5027428 47.4977188 sena= 185.6062317 185.6065369 • 3h: 12hr local time uslot=3,lslot=6: 3099,1597 3099,1598 lat,lon= 40.9434242 131.8815613 sunz= 65.5979691 66.5323486 suna= 252.3380127 253.3214874 senz= 47.4776611 47.4726372 sena= 185.6077881 185.6080933 • 7h: 17hr local time

  26. Simulation with AOT550=0.1

  27. Simulation with AOT550=0.5

  28. GOCI data

  29. 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 processingincluding the atmospheric correction. • Smoothing the geophysical parameters would make sense.

  30. Distance-to-border weighted average Slot i Slot j Slot i d1 wi d4 d2 wj d3 wi= min(d1,d2,d3,d4) where is number of pixels to the k-th border N’=∑(wiⅹNi)/∑wi N’: weighted average Ni: reading from the ith slot

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

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

  33. 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.

  34. Thank you!Please contact us if you have any idea on this issue.youngjepark@kordi.re.kr

More Related