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5.1. Glacier change assessment
The successful DEM co-registration allowed glacier change
measurements to be made. Figure 5 shows an elevation profile
along the glacier front of Leonardo glacier. Substantial surface
lowering can be observed while the glacier front remains
relatively stable. The lowering is higher near the front and
reduces further upstream. Maximum elevation changes of up to
50 m are observable which translates into an annual lowering of
~1.5 m/yr over the period of 33 years (1968-2001). Similar
results were found for Nemo glacier where a lowering of up to
30 m (~0.8 m/yr) at the glacier front was observed (1969-2005).
While the front of Leonardo glacier remains relatively stable
over the observed period (see Figure 6), the front of Nemo
glaciers shows significant retreat of ~165 m between 1969 and
2005 (not shown here). The frontal retreat was measured
perpendicular to the glacier front in the ortho-imagery for both
epochs.
300 s
w 1968
—— 2001
A
200 = Upstream
9
®
>
0
! 190 -
Front
0 i 1 A — T.
0 500 1000 1500 2000 2500
Distance [m]
Figure 5: Surface elevation profiles (dotted line in Figure 6) for
Leonardo glacier, western AP (61.91* W, 64.68* S) for 1968
and 2001
Leonardo Glacier 1968 - 2001
——- Frontline 1968
^ Frontline 2001
~ Profile
"Volume sampling area
Figure 6: Satellite image of Leonardo glacier front in 2001
(dotted line represents profile in Figure 5)
DEM differencing also allowed the measurement of volumetric
changes using ArcGIS. À glacier wide mass balance assessment
was not possible because both glaciers were not completely
covered by the imagery. However, it was possible to derive a
specific surface mass balance, assuming an ice density of
0.917 kg/m’, for an area along the front of Leonardo and Nemo
glacier. For Leonardo glacier (Figure 6) a mass loss of 25.1 =
3.5 million m? w.e. over an area of 3.6 km? (1968-2001) was
determined. The respective mass loss for Nemo glacier was 5.6
+ 0.6 million m? over an area of 1.5 km? (1969-2005). It should
be noted, that higher elevation mass gains, due to increased
accumulation of snow (Pritchard and Vaughan, 2007) might
outbalance the observed loss. However, this aspect is yet to be
examined. The overall trend from the results presented here is a
mass loss along the glacier fronts.
6. DISCUSSION
The observed lowering is in agreement with observations of
regional warming and glacier retreat in the AP over the last
decades (Cook et al., 2005). The frontal lowering at Leonardo
glacier (-64.7°S) is higher than at Nemo glacier (~67.7°S). If
the observed glacier surface lowering is caused by atmospheric
warming these differences could be explained by changes in the
mean air and sea surface temperatures across the western AP
(Meredith and King, 2005; Cook and Vaughan, 2010). The
recently observed acceleration of glaciers in the AP (Pritchard
and Vaughan, 2007) is likely to be connected to frontal thinning,
as observed here.
Although, this study allowed the measurement of multi-decadal
glacier change since the 1960s, the temporal resolution is too
low for the assessment of changes between the decades till now.
The glaciers studied here only represent a small section of the
roughly 400 glaciers in the western AP. A better spatial and
temporal resolution across the whole region is needed to answer
the following questions:
e When did the surface lowering begin to be significant?
e Is the lowering constant over time or has it changed at
different rates?
e Is the lowering evident for all glaciers in the AP and
up to what altitude does the lowering occur?
e — What is the spatial pattern of change across the AP
and how does it fit with climatic observations?
These questions could be answered with further exploration of
the USGS and BAS image archives. It should be noted, that
parts of these archive images are not directly suitable for DEM
extraction e.g. due to extensive cloud cover or high image
brightness caused by reflection of ice and snow. Currently,
within this research, more image frames are being processed
and analysed, with further results to be reported in due course.
ASTER provides a suitable source of reference data for the
comparison with the historic datasets if higher resolution data is
not directly available. However, attention should be paid to
upcoming data sources with higher resolution such as TanDEM-
X, which could further extend the time series. Glacier wide