Transcript Document

Electro-optical systems
Sensor Resolution
Outline
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Electro-optical vs. photographic systems
Spatial resolution
Radiometric resolution
Signal-to-noise ratio
Noise equivalent reflectance, radiance, temperature
Spectral Resolution
Temporal Resolution
Principles of Detection
• Photographic camera/film systems
• Digital electro-optical systems
Photographic Systems vs. Electro-optical Systems
• Both can be used to create images
– photography is non-scanning
– electro-optical systems can be either scanning or non-scanning
• Both record interactions with radiation
– films coated with photo-sensitive silver halide emulsions to record
an image
– electro-optical systems detect radiation through an electrical
system
• EMR detection capabilities are quite different
– film is always passive, uses reflected sunlight, only works in the
range of 0.4 - 1.0 mm
– digital systems can be active or passive, can work in all parts of
EM spectrum, high spectral resolution is possible, can be nonimaging system (e.g. laser altimeter)
Digital Number
at-sensor
radiance
imaging optics
detectors
electronics
DN
The DN that is recorded is proportional to the
radiance at the sensor
Digital Raster Imager Format
Spatial Resolution
• “A measure of the smallest angular or linear
separation between two objects that can be resolved
by the sensor”. (Jensen, 2000)
• Resolving power is the ability to perceive two
adjacent objects as being distinct
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size
distance
shape
color
contrast with background
sensor characteristics
• Instantaneous field of
view (IFOV) is the
angular field of view of
the sensor, independent
of height
• IFOV is a relative
measure because it is an
angle, not a length
• It can be measured in
radians or degrees
sensor
b
IFOV
GIFOV
• Ground-projected instantaneous field of view
(GIFOV) depends on satellite height (H) and
the IFOV
IFOV 
GIFOV  2H tan

 2 
1 kilometer
IKONOS image of Gunnison River Basin, CO
1 meter resolution
250 meter resolution
SPATIAL
RESOLUTION
Radiometric Resolution
• Number of digital values (“gray levels”) that a
sensor can use to express variability of signal
(“brightness”) within the data
• Determines the information content of the
image
• The more digital values, the more detail can
be expressed
Radiometric Resolution
• Determined by the number of bits of
within which the digital information is
encoded
21 = 2 levels (0,1)
22 = 4 levels (0,1,2,3)
28 = 256 levels (0-255)
212 = 4096 levels (0-4095)
8 bit radiometric resolution
2 bit radiometric resolution
Dynamic
Range
Saturation
Ideal
Response
(offset for
clarity)
Dark
Current
Signal
Actual
Sensor
Response
dark
Scene Brightness
bright
Signal Strength
• Need enough photons incident on the
detector to record a strong signal
• Signal strength depends on
– Energy flux from the surface
– Altitude of the sensor
– Location of the spectral bands (e.g. visible, NIR,
thermal, etc.)
– Spectral bandwidth of the detector
– IFOV
– Dwell time (more on this next week)
Signal-to-Noise Ratio (SNR)
A sensor responds to both signal strength and
electronic errors from various sensor
components (noise)
SNR = signal-to-noise ratio
signal
noise
signal = the actual energy reaching the detector
noise = random error in the measurement (all
systematic noise has been removed)
 must have high SNR
To be effective, sensor
Noise 
DN

n
i1

m
DN 
i
2
n 1
mDN is the mean value of the DNs in the sample population
n is the number of DN values in the sample population
50%
A uniform material of
known reflectance
Mean DN = 201
Noise = 1.345
SNR = 201/1.345 = 149
200
201
199
203
202
201
200
DNs from a single
detector, measured in
a laboratory (prelaunch)
Noise Equivalent Radiance
Noise Equivalent Reflectance
Noise Equivalent Temperature
• A measure of the smallest magnitude of
signal or of a change in signal that can be
detected
• Can be expressed in terms of radiance (L) or
reflectance (r) or temperature (T)
Converting SNR to NEr:
Divide the noise value by the DN value recorded
over a 100% reflectance target
Since the sensor reads a value of 201 over a 50%
reflectance target we assume that it would read 402
over a 100% reflectance target
NEr = 1.345 402 = 0.0033 = 0.33%
50%
Noise 
DN

n
i1

m
DN 
i
2
n 1
mDN is the mean value of the DNs in the sample population
n is the number of DN values in the sample population
Noise Equivalent Radiance
Noise Equivalent Reflectance
Noise Equivalent Temperature
• “Noise equivalent” is a measure of the
smallest magnitude of a real change in signal
that can be detected
• Can be expressed in terms of radiance (L) or
reflectance (r) or temperature (T)
Spectral Resolution
• The width and number of spectral intervals in
the electromagnetic spectrum to which a
remote sensing instrument is sensitive
• Allows characterization based on geophysical
parameters (chemistry, mineralogy,etc.)
Spectral Resolution
• Determined by:
– the number of spectral bands
– width of each band
• Described by the full-width at half-maximum
(FWHM)
• spectral response function (SRF) of each band
Multiple bands:
• Surface components with very distinct
spectral differences can be resolved using
broad wavelength ranges
Hyperspectral Remote Sensing
Hundreds of
bands
Temporal Resolution
• The frequency of data acquisition over
an area
• Temporal resolution depends on:
– the orbital parameters of the satellite
– latitude of the target
– swath width of the sensor
– pointing ability of the sensor
• Multi-temporal imagery is important for
– infrequent observational opportunities (e.g.,
when clouds often obscure the surface)
– short-lived phenomenon (floods, oil spills,
etc.)
– rapid-response (fires, hurricanes)
– detecting changing properties of a feature to
distinguish it from otherwise similar features
TEMPORAL
RESOLUTION
Examples of sensor temporal resolution:
SPOT - 26 days (1, 4-5 days with pointing)
Landsat - 16 days
MODIS - 16 day repeat, 1-2 day coverage
AVHRR – 9 day repeat, daily coverage
GOES - 30 minutes
More about this when we discuss orbits