- 545 -
± 200 m, and normally only accuracies in the order of ± 300 -
600 m.
[ties is
given
nited
il
, the
Bologi-
lic in-
Lderably
BO 000
^graphs
I be-
Techno-
area of
This accuracy can be met or even exceeded by ERTS-1
imagery. According to BÂHR & SCHUHR (1974) the mean positional
error of system corrected ERTS-1 MSS images is ± 171 m, and the
maximum error amounts to ± 400 m. COLVOCORESSES & McEWEN (1974)
and KRATKY (1974) report similar values.
Interpretation of aerial photographs at a scale of
1 : 50 000 and plotting on a third order stereoplotter results
in a positional accuracy of ± 25 m, under the condition that
the control points used are sufficiently accurate.
Taking into account that the precision of drafting on
an ERTS-1 enlargement image is in the order of ± 0.5 mm
(corresponding to ± 100 m in the field at 1 : 200 000), it
es give
or field
follows that in such a case the geological interpretation of
the satellite image will produce equal or higher positional
accuracy than field mapping, and that by using aerial photogra
phic interpretation an even préciser positioning of geological
of the
al.
1 photo-
STOCK
K 1972;
s, a
ese
details can be expected.
For instance, a regionally important lineament in the
northeastern Tibesti is represented on the existing "Carte géo
logique provisoire" (WACRENIER 1958) with more than 1 km devi
ation from its position as shown on the ERTS-1 image. Other
details are sometimes up to 5 km off their real positions accor
ding to ERTS-1.
luated
Resolution, Detectability, Recognizability
trans-
•gements
The resolution of the ERTS-1 MSS images is in the or
der of 224 - 316 m, depending on the band used (COLVOCORESSES
1972). These values refer to photographic resolution and do not
give the minimum size of objects we can really see on the ima
ges (ROSENBERG 1971). The detection limits for the smallest ob
)00.
)00.
jects visible on the MSS images of the Tibesti are in the or
der of 75 m (LIST, HELMCKE & ROLAND 1974) under optimum condi
tions (contrast, outlines of object, light object on dark
background).
;al pro-
i repre-
which
; least
In theory, when mapping on suitable enlargements from
satellite images, we come close to the accuracy obtainable by
geological field work, as far as detection and representation
of small details under favorable conditions is concerned, since
areas smaller than 50 m in diameter can also not be shown on a
map of 1 : 50 000 or smaller.
But the limit of about 75 m refers only to detectabi
: avail-
Bologist
r than
lity, and not to recognizability. In this respect the satellite
image is far inferior to the larger scale aerial photograph.
The low detection limit of the ERTS-1 image can only be fully
utilized for geological mapping if we are sure what kind of
geological feature there is, like sand-filled valley floors or