Radiometric Calibration,
Spatial Characterization, and Spectral Evaluation of the Advanced Land
Imager and Hyperion Sensors
Principal Investigator
Dr. Stuart
Biggar, Remote Sensing
Group, Optical Sciences Center,
U.
Arizona
Co-Investigators
Spatial Performance Analysis
1.0 Calibration/validation of ALI spatial response
and MTF and comparison to ETM+
We propose to measure the ALI spatial response to validate the pre-launch
predicted performance and to monitor any on-orbit changes over time.
1.1 Background
Previous experience with Landsat-4 and -5 TM indicate that the spatial
response of that design extends over about 40-45m, rather than the 30m
pixel often assumed.
Because of the whiskbroom design of TM, the spatial response is notably
asymmetric in-track and cross-track (Schowengerdt, 1997), with a wider
response cross-track due to an electronic low-pass filter in the data stream.
The spatial response characteristics of ALI are expected to be substantially
different from TM and ETM+ since ALI is a pushbroom array imager. For example,
if time integration is used in-track to increase SNR, then a broader spatial
response will be expected in-track than cross-track. At this time, we do
not have the sensor engineering details necessary to make such a conclusion,
and will need relevant engineering design and test data for ALI to support
our on-orbit tests.
1.2 Approach
The ALI, Hyperion and ETM+ spatial response functions will be measured
with three techniques:
1) Analysis of linear targets such as bridges over
water
This technique has advantages of high signal contrast and subpixel sampling
dependent on the angle of the target to the in-track and cross-track directions
(Schowengerdt et al, 1996). However, it requires imagery of specific targets
and only permits 1-D measurements orthogonal to the target. Possible targets
are the San Mateo Bridge over San Francisco Bay (18.3m wide at 31.1°
to cross-track), which we've used previously to evaluate TM (Schowengerdt
et al, 1985), and the causeway over Lake Pontchartrain, Louisiana (two
10m spans, separated by 12m, at <1° to in-track ). The latter target
has several unique characteristics, including a straight 26 mile length
and alignment to the TM path within 1° (see Fig. ?). These features,
combined with the 12-bit quantization of ALI and Hyperion data, allow high
precision cross-track subpixel sampling (the incremental subpixel phase
from line-to-line is about 1/70 pixel for TM) for alias-free MTF analysis
and precise unmixing tests (described below). Furthermore, the nearly in-track
orientation of the Causeway means that we will be using only a few adjacent
detectors in the pushbroom array, minimizing any required relative calibration
effort.
Both of these targets are near the center of the Landsat path. To acquire
them with ALI and Hyperion will require "rolling" of the spacecraft so
both sensors view nadir, which we understand can be done by special request.
The radiometric profile across a bridge over water will vary with solar
angle due to shadows (see Fig. ?). We will calculate the size of these
shadows for given image acquisitions based on the bridge geometry and height
above water. Spectroradiometric ground measurements will also be used to
determine the relative reflectances of the bridge and water. The MTF analysis
then requires a correction for the radiance profile of the bridge as described
by Schowengerdt (1985).
2) Comparison of relative spatial frequency content
of ALI to ETM+ images
This technique can be used on any near-coincident pair of ALI and ETM+
images. Temporal changes are not of concern because of their one minute
separation. The spatial response of ALI relative to that of ETM+ will be
measured in terms of a relative MTF (Schowengerdt et al, 1985) and can
be obtained for bands ALI-2 (TM-1), -3 (TM-2), -4 (TM-3), -8 (TM-5), and
-9 (TM-7). The other ALI bands do not match those in ETM and a relative
image comparison is therefore not valid. Information on relative SNR may
also be obtained from this analysis. A drawback is that the scene must
have high spatial detail and radiance contrast in order to obtain reliable
MTF measurements.
3) Comparison of relative spatial frequency content
of ALI-pan and ALI-2, -3 and -4 bands
Any ALI image set that includes data from these four channels can be used
for this technique. The MTF of the 30m bands (in the visible) relative
to the 15m panchromatic band will be obtained. This information will be
useful in fusion of ALI-pan and ALI-MS bands. The same advantages and drawbacks
as in (2) above apply to this technique as well.
