Hyperspectral%20Environmental%20Monitoring%20of%20Waste%20Disposal%20Areas - PowerPoint PPT Presentation

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Hyperspectral%20Environmental%20Monitoring%20of%20Waste%20Disposal%20Areas

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Chlorophyll concentration (mm/cm2) Equivalent water thickness (cm) Generated spectra. Healthy leaf (high chlorophyll and water) Stressed leaf (low chlorophyll and ... – PowerPoint PPT presentation

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Title: Hyperspectral%20Environmental%20Monitoring%20of%20Waste%20Disposal%20Areas


1
Hyperspectral Environmental Monitoring of Waste
Disposal Areas
  • Jason Hamel
  • Advisor Rolando Raqueño
  • Digital Imaging and Remote Sensing Laboratory
  • Chester F. Carlson Center for Imaging Science
  • Rochester Institute of Technology
  • Rochester, NY

2
Overview
  • Background
  • Procedure/Results
  • Spectra
  • Classification
  • Conclusions

3
What are Landfills?
  • Very common waste management technique
  • They do not separate toxic wastes from the
    environment
  • A water resistant clay cap is placed over the
    landfill slows the spread of chemicals

4
Clay Caps
Diagram of the material layers in the 2 major
clay cap technologies BGC.pdf for DOEs SRS
site
5
Clay Cap Technology
  • Caps are designed to last 40 years
  • Replace with new technology that actually deals
    with the waste
  • This lack of solution has given chemicals time to
    leach into the environment
  • These problem areas must be found

6
Why Look at Landfills?
  • Currently, possible dangerous sites are manually
    sampled and processed in a lab
  • This can be time and money consuming for larger
    sites or a large number of sites
  • Chemicals are often dangerous even at very low
    concentrations
  • Remote sensing with new hyperspectral detectors
    may provide and economic alternative

7
Example of Expected Imagery
Hyperspectral AVIRIS scene with 224 bands SRS
site
8
Purpose of this Research
  • Low concentrations make it very difficult to
    directly detect a chemicals spectral signature
  • Determine if new hyperspectral sensors collect
    enough information to identify materials
  • Determine the detectability of specific secondary
    spectral effects of leachates (e.g.)
  • Vegetation health
  • Soil water moisture
  • Determine if atmospheric correction is necessary

9
General Procedure
PROSPECT
Real Soil
Material Classification
OSP
SAM
SSM
Unmixing
Spectra
VEG S/U
Spectral Matching Algorithms
VEG/ Soil
Wavelength
Soil/ Soil
Atmosphere, Detectors, and Noise
Mix Spectra
10
Vegetation Spectra
  • PROSPECT leaf model and software
  • Two varied inputs
  • Chlorophyll concentration (mm/cm2)
  • Equivalent water thickness (cm)
  • Generated spectra
  • Healthy leaf (high chlorophyll and water)
  • Stressed leaf (low chlorophyll and water)

11
Vegetation Spectra
Reflectance Spectra of Vegetation Green
Healthy Red Stressed
12
Soil Spectra
  • Ground measurements taken with spectrometer as
    soil dried
  • Moisture in soil was not measured while spectra
    was taken
  • Relative labels given to various spectra
  • Wet Soil
  • Moist Soil
  • Dry Soil

13
Soil Spectra
  • Reflectance
  • Spectra of Soil
  • Brown Dry
  • Orange Moist
  • Black Wet

14
Reflectance Data Set
  • The 5 basic vegetation and soil spectra are mixed
    by
  • This creates 10 additional mixed spectra
  • 15 spectra in final data set

where R1 and R2 are 2 basic spectra
15
Atmosphere and Detector Effects
  • Light reflecting off material propagates through
    atmosphere
  • Detector measures the radiance reaching the
    detector at various narrow wavelength regions
    called channels
  • Detector electronics record input signal in
    digital counts (DC)
  • The hyperspectral AVIRIS detector has 224
    channels from 400nm to 2500 nm

16
Digital Count Spectral Data Set
  • Radiance reaching the sensor, Lsen, calculated
    from the Big Equation
  • Radiance variables supplied by MODTRAN

ES
Lu
LD
T1
T2
R
17
Detector Effects
  • All spectra converted to AVIRIS wavelength
    regions
  • Lsen was multiplied at each wavelength by an
    AVIRIS gain factor to calculate AVIRIS DCs

18
AVIRIS Basic DC Spectra
19
Realistic Data Set
  • All detectors measure noise as well as signal
  • Standard gaussian noise with standard deviation
    of 1 added to DC spectra (not representative
    AVIRIS noise value)
  • Noisy sensor radiance determined
  • Noisy reflectance spectra calculated by removing
    atmosphere effects

20
Noisy Basic Reflectance Spectra
21
Classification
  • 6 classification algorithms used
  • Linear Spectral Unmixing (ENVI)
  • Orthogonal Subspace Projection (Coded)
  • Spectral Angle Mapper (ENVI)
  • Minimum Distance (ENVI)
  • Binary Encoding (ENVI)
  • Spectral Signature Matching (Coded)
  • The 5 basic vegetation and soil spectra were used
    as endmembers
  • Reflectance endmembers converted to DC before
    classifying DC spectra

22
Classification Algorithms
  • Linear Spectral Unmixing (LSU)
  • Generates maps of the fraction of each endmember
    in a pixel
  • Orthogonal Subspace Projection (OSP)
  • Suppresses background signatures and generates
    fraction maps like the LSU algorithm
  • Spectral Angle Mapper (SAM)
  • Treats a spectrum like a vector Finds angle
    between spectra
  • Minimum Distance (MD)
  • A simple Gaussian Maximum Likelihood algorithm
    that does not use class probabilities
  • Binary Encoding (BE) and Spectral Signature
    Matching (SSM)
  • Bit compare simple binary codes calculated from
    spectra

23
Classification Results
  • The LSU and OSP fraction maps allow for the
    calculation of sum of squared error

i endmember j wavelength
Sum of Square Errors Classifier Ground
Sensor DC Retrieved
Reflectance with Atmosphere Reflectance
LSU 4.81e-11 0.239
0.032 OSP 2.32e-6
0.237 0.038
24
Classification Results
  • The SAM, MD, BE, and SSM algorithms were not
    designed to classify mixed pixels
  • Accuracy is the correct identification of one of
    the fractions in a pixel

Percent Accuracy Classifier Ground Sensor
DC Retrieved
Reflectance with Atmosphere Reflectance
SAM 66.67 40.00
66.67 MD 66.67
80.00 66.67 BE
86.67 66.67 86.67
SSM 93.33 80.00
93.33
25
Conclusions
  • Atmosphere degrades performance of most of the
    classification algorithms studied
  • Removal of the atmosphere is recommended
  • The LSU and OSP fraction maps are more useful
  • Provide very accurate material identification
    without a large spectral library
  • Detects not just the material, but the amount of
    material in a given pixel

26
Follow Up Work
  • There are many areas to expand on this research
  • More realistic sensor noise
  • Additional levels of vegetation health
  • Broader range of atmospheres
  • Incorporate background cloud effects
  • Create a greater variety of mixed pixels
  • Different percentages
  • More than 2 materials
  • Identification of actual secondary spectral
    effects of leachates
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