in the region and the water levels on some parts of
the chotts are dominated by this runoff. These areas
do not, however, have spring mound or aioun fields.
As spring mounds are formed by upward groundwater
seepage they are frequently associated with specific
underlying lithologies and structures, particularly
well developed faulting and jointing Reeves (1968).
The overall structure in this area consists of a
series of sedimentary horizons, with known aquifers,
dipping to the north. This structure itself is not
conducive to groundwater upwellings despite the
fact that groundwater is present. The Alpine folding
and faulting of the Atlas Mountains affects the
sedimentary strata on the northern margin of the
Saharan Platform. Folding of these sediments on
the Saharan Platform led to the formation of the
Chott el Fedjadj anticline. The Djebel Tebaga is
the prominent southern limb of this anticline and
it plunges westward under the Chott el Djerid. The
area still suffers from infrequent tectonic activity.
It can be hypothesised that the occurrence of spring
mounds are related to faulting and jointing
associated with this folding. This can be tested to
examining the directions of the alignments of these
isolated features on Landsat TM imagery by lineament
analysis.
In addition the distribution of aioun can also be
examined and related to the structural trends. This
should enable the origins of aioun to ascribe to
either deep or shallow groundwater sources.
3. IDENTIFICATION OF SPRING MOUNDS AND AIOUN ON
SATELLITE IMAGERY
Difficulties exist in attempting to identify and map
spring mounds and aioun by ground survey
Geomorphological problems are encountered during the
identification and mapping of aioun because of their
lack of relief and the difficulty in mapping subtle
variations in salt concentrations on flat playa
surfaces. Spring mounds are far easier to identify
in the field because of their relief and the presence
of vegetation. Vegetation is commonly found on the
less saline margins of playas. It mainly takes the
form of halophytic shrubs and grasses and the centre
of the spring mounds are also vegetated, often with
less salt tolerant species, in response to spring-
flow. The logistical problems of field work on playas
are immense; they mainly concern difficulties of
access, heat, salt glare and the location of ground
control points. As a consequence most topographic
maps mark playas as featureless voids!
Remotely sensed imagery is therefore an extremely
important tool in the identification and mapping of
playa features such as spring mounds and aioun.
The advantages of remotely sensed imagery in such
studies not only lie in their ability to overcome
the geomorphological and logistical problems but
also because of the shape and spectral characteristics
of the features themselves.
A very important identification criterion for
spring mounds and aioun is their circular shape;
this makes them readily identifiable on remotely
sensed imagery (Figs, 2 and 3). However it can be
seen on Fig. 3 that the spring mounds develop long
tails to the SW. These tails are deposits of
gypsiferous sands deposited in the lee of the spring
mounds in the prevailing wind directions.
In addition there are significant variations in
spectral responses between the features and the
adjacent playa surfaces, Table 1. Spring mounds
are often vegetated with either a natural vegetation
community of tamarisk and date palms or, more
commonly in this area, they form the nucleus of
irrigated oases with date palms and an understory
of smaller trees and ground crops. As they are
Figure 2. Band 3,4,5, false colour composite of the
Chotts el Djerid and el Fedjadj showing the playa
facies (from Mitchell, 1982), the aioun and spring
mound fields and the Chott el Fedjadj plunging
anticline.
Figure 3. Band 3 image of Seftimi showing spring
mounds with sand tails. The resistant limestone
beds forming the southern limb of the Chott el
Fedjadj anticline can be seen at the bottom of the
image.
located in marginal playa facies they can be
surrounded by unvegetated surfaces or halophytic
plant communities. Where they are surrounded by
bare surfaces identification is easy because of the
differences in absorption between vegetation and
bare soils; particularly in TM Bands 3 (0.63-
0.69ym) and 4 (O. 79-0.90y.m) . It is also relatively
easy to spectrally separate spring mound vegetation
from the surrounding halophytic vegetation. As
spring mounds have adequate water supplies all the
year around their vegetation is rarely under stress
and maintains a low reflectance in TM Bands 3 and 4
throughout the year. Halophytic vegetation does
however exhibit some seasonality and partially dies
back in the summer; stressed halophytic vegetation
is seen on TM imagery in this area. In addition the
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