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Mapping Roads and other Urban Materials using Hyperspectral Data
Dar Roberts, Meg Gardner, Becky Powell, Phil Dennison, Val Noronha
What is Hyperspectral Remote Sensing?
• Airborne or Spaceborne Sensors– Airborne Visible/Infrared Imaging Spectrometer (AVIRIS)– Hyperion
• Sample large number of contiguous wavelengths– AVIRIS: 224 channels, 10 nm intervals, 20 to 4 m.– Ikonos: 4 channels (4 m), 1 panchromatic (1 m)– Thematic Mapper: 6 channels, 3 vis,3 NIR, 30 m.
• Material identification based on chemistry and physical structure– Radiance --> reflectance– Reflectance --> identification
Challenges of the Urban Environment
• Urban environments are incredibly heterogeneous– The diversity of materials is high
• Urban land-cover is typically homogeneous below the spatial resolution of most sensors– Most sensors sample 20-30 meter resolution, but surfaces are
smaller than that– Exceptions: Ikonos (1 m), aerial photography (< 1m)
• Spectral knowledge of urban environments is lacking• Algorithms for mapping urban environments are mostly
lacking– Mostly pattern matching, some classification
Objectives
• To develop a spectral library of urban materials
• To map urban features using hyperspectral data– automated road feature extraction
– roof type mapping and other urban surfaces
• To explore the potential of hyperspectral data for assessing pavement age and quality
Image Data Availability
• Santa Barbara study region• Fine resolution AVIRIS (4 m)
– 1999, 2000, 2001 (scheduled)
• Coarse resolution AVIRIS (20 m)– 1998 to 2001
• Hyperion (30 m, follows ETM)– June 12, 2001
• ETM (30 m)– June 12, 2001
• IKONOS• Extensive photographic coverage (DOQQs)
AVIRIS - Santa Barbara, CaliforniaOct 11, 1999 low-altitude data - 4 meter pixels
Red 1684 nmGreen 1106 nmBlue 675 nm
Each pixel is a spectrumPotential for library development is large
AVIRIS 991011Red = 1684 nmGreen = 1106 nmBlue = 675 nm
0
50
100
150
200
400 900 1400 1900 2400
Wavelength (nm)
Re
fle
cta
nce
(50
0=50
%)
Parking Lot
0
100
200
300
400
500
400 900 1400 1900 2400
Wavelength (nm)
Re
fle
cta
nce
(50
0=50
%)
Roof5(Vons1)
Roof6(Vons2)
0
50
100
150
200
400 900 1400 1900 2400
Wavelength (nm)
Re
fle
cta
nce
(50
0=50
%)
Road2(CalleReal)
Road7(Fairview)
Field Spectra
• Spectrometer: Analytical Spectral Devices Full range: On loan from JPL
• Late May, early June 2001 field campaign
• Measured a diversity of roads, bridges, sidewalks, roofs and other materials
• Well documented metadata including some photographs
Sample Concrete Spectra
0
0.1
0.2
0.3
0.4
0.5
350 850 1350 1850 2350
Wavelength (nm)
Re
fle
cta
nce
(0.
5=50
%) ppcsmm.001-
ppcsmm.002-
ppcsmm.003-
ppcsmm.004-
ppcsmm.005-
ppcsmm.006-
Field Spectra CollectionASD Full-Range Spectrometer
Field photos were taken & metadata recorded at each field site...
Field Spectra Summary• Over 6,500 urban field spectra were collected throughout Santa Barbara in May & June
2001
• Field spectra were averaged in sets of 5 and labeled appropriately in building the urban spectral library
• The resulting urban spectral library includes:– 499 roof spectra– 179 road spectra– 66 sidewalk spectra– 56 parking lot spectra– 40 road paint spectra– 37 vegetation spectra– 47 non-photosynthetic vegetation spectra (ie. Landscaping bark, dead wood)– 27 tennis court spectra– 88 bare soil and beach spectra– 50 miscellaneous other urban spectra
Roads and Parking Lots
Typical Roads
0
0.05
0.1
0.15
0.2
0.25
0.3
0.35
0.4
0.45
0.5
350 850 1350 1850 2350
Wavelength(um)
Ref
lect
ance
Fairview
Cathedral Oaks
Butte
Pembroke
Brandon
Parking Lots
0
0.05
0.1
0.15
0.2
0.25
350 850 1350 1850 2350
Wavelength (um)
Refl
ecta
nce
Dry oil
Parking lot1
Parking lot 2
Parking Lot 3
Sealcoat
Concretes
0
0.1
0.2
0.3
0.4
0.5
0.6
0.7
350 850 1350 1850 2350
Wavelength (um)
Ref
lect
ance
Old ConcreteNew ConcreteConcrete BridgeRed TintedConstance
Street Paints
0
0.1
0.2
0.3
0.4
0.5
0.6
0.7
0.8
350 850 1350 1850 2350
Wavelength (um)
Re
fle
cta
nc
e Old White
Fresh White
Blue
Fresh Red
Yellow
Fresh Yellow
Tennis Courts & Other Surfaces
0
0.1
0.2
0.3
0.4
0.5
0.6
0.7
0.8
350 850 1350 1850 2350
Wavelength (um)
Ref
lect
ance
Tennis Court (dg)
Tennis Court (g)
Tennis Court (t)
Gravel 1
Gravel 2
Bare Soil
Plant Materials
0
0.1
0.2
0.3
0.4
0.5
0.6
0.7
0.8
350 850 1350 1850 2350
Wavelength (um)
Ref
lect
ance
Old Bark
New Bark
Pine Needles
Grass
English Ivy
Star Jasmine
Composite Shingles
Dark Composite Shingle
0
0.05
0.1
0.15
0.2
0.25
350 850 1350 1850 2350Wavelength (um)
Ref
lect
ance
Dark Grey
Tan
Very Black
Dark Orange
Green
Light Composite Shingle
0
0.05
0.1
0.15
0.2
0.25
0.3
0.35
0.4
0.45
0.5
350 850 1350 1850 2350
Wavelength (um)
Ref
lect
ance
Red 10 years
Red
Light Grey
Light Brown
Very Light Green
Grey (4)
Represents less than half the spectra measured, all distinct
Other Roof Materials
Bright Roofs
0
0.1
0.2
0.3
0.4
0.5
0.6
0.7
0.8
350 850 1350 1850 2350
Wavelength(um)
Refle
ctan
ce
Wood 1
bRed Tile
dRed Tile
Calshake
Green Metal
Wood 2
Dark Roofs
0
0.1
0.2
0.3
0.4
0.5
350 850 1350 1850 2350
Wavelength (um)
Ref
lect
ance
Uncoated Tile
Tar (1)
Gravel 2
Red Gravel
Cedarlite
Mapping road quality and age
• What do roads look like when they are modified?
• What do roads look like as they age?
• Can road quality be mapped?
• What materials are confused with roads?
Road Surface Modification
0
0.05
0.1
0.15
0.2
0.25
350 850 1350 1850 2350
Wavelength (um)
Re
fle
cta
nc
e
Dry Oil
Wet Oil
Tar Patch
Sealcoat
Road Aging
0
0.05
0.1
0.15
0.2
0.25
0.3
0.35
0.4
350 850 1350 1850 2350
Wavelength (um)
Ref
lect
ance
Calle Real
Cathedral Oaks
Evergreen
Brandon
Butte
Delnorte-avg
Old
New
Road Quality
Good roads and bad roads can be spectrally similarCracking & patching occur at the wrong scale
0
0.05
0.1
0.15
0.2
0.25
350 850 1350 1850 2350
Wavelength (um)
Re
fle
cta
nc
e
Butte
Berkeleyg
Berkeleyb
Roads and Roofs
Roof Materials
0
0.1
0.2
0.3
0.4
350 850 1350 1850 2350
Wavelength(um)
Ref
lect
ance
Uncoated Tile
Tar Roof(1)
Cedarlite
dg Composite
10yr Red Composite
vblk Composite
All but the darkest are spectrally distinct in some portion of the spectrumIllumination differences and mixed pixels will reduce separability
Roads and Parking Lots
0
0.1
0.2
0.3
0.4
350 850 1350 1850 2350
Wavelength (um)
Ref
lect
ance
Tar Patch Parking Lot1
Parking Lot3 Fairview
Butte Pembroke
Approaches for Spectral Feature Extraction
• Matched filters and derivatives
• Cluster matched filter
• Spectral Angle Mapper
• Tetracorder
• Multiple Endmember Spectral Mixture Analysis (MESMA)
• Simple Spectral Mixture Analysis– One suite of spectra used to decompose full scene
– Typical spectra: Soil, Shade, Green Vegetation, Non-photosynthetic Vegetation
– Inappropriate for many urban areas
• MESMA– Multiple suites of spectra
• number and type vary per pixel– Select by fit and fractions
• ideal for the complex urban environment
• Models can be prioritized
Multiple Endmember Spectral Mixture Analysis
MESMA: Initial Results
Road and Roof Confusion
AVIRIS Color Composite Road MappingUsing Adobe Photoshop™ Paintbucket Tool
Masked MESMA
Summary
• Most urban materials sampled are spectrally distinct– Dark surfaces were the least distinct
• Spectra change with aging– Road surfaces and composite shingle brighten
– Paints and red tile darken
• Road quality did not impact spectra– Cracks and patches occur at a different scale
• Roads and certain roof types are confused– Tar roofs, dark composite shingles
• A combination of spatial pattern matching and spectral matching is promising
Future Directions• Improve upon current techniques:
– Publish results
• Address three critical questions:– How many bands do you need, and which bands are best?
– What is the minimum spatial resolution required?
– Which sensors meet these requirements and if none, what could be designed?
– Santa Barbara test site• Test bed of techniques and sensors• Competing techniques for centerline mapping (ie, GPS) and road quality
• Scale up:– Rural roads and global road databases