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Pickup et al. (1995) indicated that a single equation, based on
view angle, can be used for scene-brightness normalisation.
Their findings show that this produces results better than the
commonly used band-ratio techniques. This method was tried
with data collected at another minesite but to date the results
have not been thoroughly analysed.
The mining industry is vital to the Australian economy, but
mining activity inevitably causes environmental impacts.
Usually the miner must rehabilitate areas of disturbance to a
condition satisfactory to the relevant government legislation. In
Comalco’s bauxite mines at Weipa and Andoom, North
Queensland, Australia, DMSV data were collected by
SpecTerra Systems (STS) in November, 1994. This system was
chosen because it gives a non-invasive, high-resolution, timely
and cost-effective method of quantitatively monitoring a large-
scale rehabilitation operations.
À total of 196 frames of DMSV data, each being approximately
1x1.5 kilometre. with 2 metre spatial resolution, were collected
over the Weipa and Andoom minesites on the 12th, 13th and
14th of November, 1994. The objective was to produce digital
and photographic mosaics for quantitative measurement of the
vegetation status. Before this could be achieved, it was
necessary to remove ‘artefacts’ inherent in the DMSV data, of
which shading is the most significant.
For this work spaceborne data, acquired at about the same time
(10th November, 1994) as the DMSV image, were used as
uniformly illuminated ‘flat’ image to derive a shading surface
for correcting the DMSV data. Landsat TM bands 1, 2, 3, and
4 have band-centres close to the band-centres of the DMSV
(Table 1). The correction method exploits this similarity by
correlating the DMSV data with the near-simultaneously
acquired TM imagery. The wavebands of the field radiometer,
used for the calibration of the DMSV images, are also included
in Table 1.
Methods
Table 1: Wavelengths of Landsat TM, DMSV and Exotech Radiometer bands
| Sensor band 1 band 2 band 3 band 4
Landsat TM 450 - 520 (nm) 520 - 600 (nm) 600 - 690 (nm) 760 - 900 (nm)
DMSV 438 - 462 (nm) 538 - 562 (nm) 638 - 762 (nm) 758 - 782 (nm)
Exotech | -..450 - 480 (nm) 500 - 600 (nm) 600 - 700 (nm) 700 - 800 (nm)
All solar-illuminated remotely sensed data exhibit some amount
of differential shading. However, it is assumed for this
correction method, that the shading variation is insignificant in
the portion of the Landsat TM image used for correcting the
DMSV dataset. Figure 2 illustrates a hypothetical illumination
curve across a Landsat TM image. Although this differential
Grey
Level
i
shading would be significant were the whole of this image used
in the analysis, for a small portion of it the shading can be
assumed negligible. Figure 3 compares the Landsat TM subset
used with a DMSV frame. As illustrated, the area used for the
correction is small and the shading is negligible therefore the
shading curve across this subset is assumed to be “flat”.
Sun
Hot
Spot
i
Distance across track
7
Figure 2. Shading across a Landsat TM frame, for a given sun elevation angle 6°.
283
International Archives of Photogrammetry and Remote Sensing. Vol. XXXI, Part B2. Vienna 1996