T. Prinz, MULTISPECTRAL REMOTE-SENSING OF THE GOSSES BLUFF IMPACT CRATER, CENTRAL AUSTRALIA (NT) BY USING LANDSAT-TM AND ERS-1 DATA, ISPRS journal of photogrammetry and remote sensing, 51(3), 1996, pp. 137-149
Remote sensing techniques offer a unique chance to analyse and to map
planetary impact craters in a relatively short time and at low cost. I
n the past, studies were mainly restricted to the search for possible
impact sites (e.g. Earth) or for age determinations (crater statistics
). On the basis of Landsat-TM 5 and ERS-1 data the lithological and st
ructural characteristics of the complex Gosses Bluff impact crater (Au
stralia) has been analysed in order to obtain reasonable lithological
classification approaches. The fundamental statistical selection rule
for pure colour composites of original TM-data was the calculation of
the optimum index factor (OIF), or for hybrid colour composites (e.g.
a combination of a original TM-band with a principal component and a r
atio) using the widest statistical variance for each dataset. Addition
al spectral measurements were carried out for each representative rock
unit of the crater specific zones in order to estimate the quality of
supervised maximum-likelihood computer classifications for geological
mapping. Complementary ERS-1 altimetric data were utilized to study t
he resulting crater morphology as an expression of the displacement ef
fects and some structural features of the target caused by the crateri
ng process (e.g. diameter, fracture pattern, ejecta displacement, etc.
).