Optical calibration, bathymetry, water column correction and bottom typing of shallow marine areas, using passive remote sensing imageries
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Actually, 4SM is NOT for dummies!

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4SM errors
4SM conclusions


 
1 - NO NEED for field data, nor for atmospheric correction
2 - this is demonstrated in this website, using a variety of hyper/multi spectral data
 
Requirements are
1 - homogeneous water body and atmosphere
2 - some coverage of optically deep water
3 - some coverage of dry land
 
Problems are
1 - the precision on estimated depth is found wanting, because the noise-equivalent change in radiance  of accessible data is too high for shallow water column correction work 
2 - radiance data should be preprocessed by the provider at level 1 in order to improve S/N ratio
3 - exponential decay: the deeper/darker the bottom, the poorer the performances
 
So
I keep digging
until suitable data
become available
 
 
4SM is not for dummies!
 
Deal or NoDeal?
  • It shall be seen that an acceptable calibration which yields acceptable results 
    • is a fuzzy concept in respect of the many parameters involved 
    • even though we are using a simplified radiative transfer model
  • What is important is NOT
    • that a physically exact calibration has been achieved
    • leave that for the big boys at NRL, or EOMAP, or CSIRO
  • Rather what is important to us
    • is that a coherent set of calibration parameters be assembled
    • so that an acceptable and usefull result be produced : DTM and bottom type classification
    • using only the image
  • 4SM offers an integrated set of ergonomic tools to achieve that
    • within a short time frame
Dummies please Where is the competition?
Basic equation
  • At the base of the atmosphere (BOA) the simplified equation is
 L = Lw + (LB-Lw)/exp(K*Z)
  • This equation is inverted into
LB = Lw + (L - Lw) * exp(K*Z)
  • Unlike Z, K and all L terms are wavelength specific


 
Now, suppose
 
  • we have a clean BOA spectral image,
    • after removal of glint and path radiances,
    • with wavebands of increasing wavelengths labelled  i, j, k, ...,n
  • and effective wavelengths WLi, WLj, WL..., WLn are known for each waveband
  • and BOA spectral L and Lw are estimated from the image
  • and BOA spectral LM radiances are estimated for bright bareland in the image
  • and the complete series of Ki/Kj  ratios are estimated from the image for all pairs of bands
Then the water column correction
of the shallow marine area may be performed
 
At this stage, the product is comprised of
  • Retrieved depth: a map of the water depth for the shallow marine area in arbitrary units
  • Bottom typing: a map of the BOA water column corrected spectral bottom reflectance in units of image DNs, ready for bottom type classification 
If a seed value for K is derived using Jerlov's data
then then K is specified for all visible wavelengths
  • Retrieved depth: at this stage, the above map of the water depth becomes a provisory bathymetric map in units of meters
  • Bottom typing: this does not affect the water column corrected bottom reflectances, though
When suitable field data become available
  • Final bathymetric map: then a final retrieved Z may be computed:
    • a final coefficient may be estimated and applied to all retrieved depths
    • the tide correction may be applied to retrieved depths
    • so that the provisory bathymetric map becomes the final bathymetric map
  • Habitat map: the bottom types may be given an appropriate habitat label
    • the bottom type classification becomes a habitat map


 
BOA Soil Line
  • Suppose the various ratios LBi/LBj for non-contrasted shallow bottom signatures at null depth
    • like clean bright to dark sands, muds, clean rocks and gravels, bare soils
    • are known for all pairs of wavebands i and j from some bareland areas in the image
  • Then in a bi-dimensional histogram of BOA radiances for the pair i and j, this Soil Line
    • extends as a straight line scatter
    • from a maximum=LM, the radiance of the brightest shallow bottom type
    • to     a minimum=     0, the radiance of a black body at the base of the atmosphere
Normalization of the data
arrange for all ratios  LMi / LMj = 1
(this assumes a "flat" non-contrasted bottom signature)

 
  • Normalize all BOA radiances LM, L, and Lw,
    • so that the various ratios LMi/LMj now equal 1
  • For all non-contrasted shallow pixels at depth Z=0 
    • Li = LBi
    • Lj = LBj
  • For all shallow pixels at depth Z>0
    • Li<LBi
    • Lj<LBj
    • Li>Lj because Kj>Ki

Busy? 4SM in 10 lines


 
Now compute Z and spectral LB all at once
  • for a pair of bands i and j, increase Z in the inverted model
    • until the ratio LBi/LBj reaches 1
      • because Kj>Ki, LBj increases faster than LBj
      • LBi/LBj decreases from being >1 to a value of 1 when correct Z is applied
  • for bands i, j, k, ..., n, increase Z in the inverted model
    • until the ratio average(LBi,...,LBm)/LBn equals 1
Bias on Z and spectral LB 
  • Two bands case: of course, only non-contrasted shallow bottom signatures resort to such simplification when using a pair of bands i and j
    • for a contrasted shallow bottom signature like seagrass, corals, etc, true Z may not be reached: such simplification entails a -potentially severe- bias on computed depth
    • unless the concept of the Soils Line is modified for BGRN multispectral bands, as demonstrated in this website's tutorials
  • N bands case: when using wavebands bands i, j, k, ..., n,
    • this bias can be reduced to considerable extent
    • and contrasted spectral LB signatures may be obtained for bottom typing , like if at low tide


 
    You're done 
 

Go for it! write an image for Z and a spectral image for LB
  • proceed with depth contour maping
  • proceed with bottom type classification