71
The Arctic region is warming more rapidly than the global
average (AMAP 2017) and it is well established that this
warming is at least partially responsible for the Greenland
ice sheet losing mass at an accelerating rate, raising concern
worldwide (e.g. Kahn et al. 2015; Rahmstorf et al. 2015).
It is essential to monitor the changes of the Greenland ice
sheet to be able to assess the potential environmental, social
and economic implications around the globe, and to provide
decision-makers with reliable data. The annual mass-budget
deficit of the Greenland ice sheet has grown over the past two
decades due to increases in surface melting (Van den Broeke
et al. 2017) and ice-f low acceleration (Kahn et al. 2015).
Currently, and for the last two decades, the Greenland ice
sheet is the single largest Arctic cryospheric contributor to
global sea-level rise and the Greenland ice-surface melt rates
are projected to increase as the Arctic continues to warm
(AMAP 2017).
The snowline is here defined as the maximum elevation
during the melt season at which snow remains from the pre-
vious accumulation season (Cogley et al. 2011). The snow-
line is a valuable climate indicator as its position integrates
the competing effects of melt (increasing snowline elevation)
and snow accumulation (decreasing snowline elevation).
Thus the snowline provides a key holistic variable indicating
climate change.
We have developed a methodology that determines snow-
line elevation utilising the moderate resolution imaging spec-
troradiometer (MODIS) sensor on the Terra satellite. The
MODIS sensor produces a global dataset on a daily basis,
with a resolution varying between 250 m and 1 km, in 36
bands covering the visible to thermal wavelengths. Using
MODIS, we derived the maximum snowline altitude for the
Greenland ice sheet for the years 2000–2017. We are pro-
ducing a freely available, consistent dataset that provides an
important tool for the monitoring of the long-term impact of
climate change on the Greenland ice sheet. Direct compari-
son with field observations from automatic weather stations
(AWSs) from the Programme for Monitoring of the Green-
The Greenland ice sheet – snowline elevations at the
end of the melt seasons from 2000 to 2017
Robert S. Fausto and the PROMICE team*
* Signe B. Andersen, Andreas P. Ahlstrøm, Dirk van As, Jason E. Box, Daniel Binder, Michele Citterio, William Colgan, Konstanze Haubner,
Karina Hansen, Nanna B. Karlsson, Kenneth D. Mankoff, Allan Ø. Pedersen, Anne Solgaard and Baptiste Vandecrux
500 km
THU
UPE
KPC
TAS
KAN
NUK
SCO
QAS
EGP
Land
185.3
370.6
555.9
741.2
926.5
1112
1297
1482
1668
1853
2038
2224
2409
2594
2779
2965
3150
Snowline 2016
PROMICE
GIMP DEM
Fig. 1. Greenland map showing the location of PROMICE automatic
weather stations and the 2016 snowline as derived from Terra satellite data
using the moderate resolution imaging spectro- radiometer (MODIS)
sensor. The locations of the ground-control automatic weather stations
(PROMICE) are indicated. EGP: East GRIP. K AN: Kangerlussuaq.
KPC. Kronprins Christian Land. NUK: Nuuk. QAS: Qassimiut. SCO:
Scoresby Sund. TAS: Tasiilaq. THU: Thule. UPE: Upernavik. DEM:
Digital elevation model. GIMP: Greenland ice mapping project.
© 2018 GEUS. Geological Survey of Denmark and Greenland Bulletin 41, 71–74. Open access: www.geus.dk/bulletin
http://www.geus.dk/bulletin
7272
land Ice Sheet (PROMICE) network validates the snowline
dataset derived from MODIS. We use the services of the
CryoClim internet portal, providing an operational and per-
manent service for long-term systematic climate monitoring
of the cryosphere, to distribute our snowline product. More
specifically, end-of-melt season, 1 km2 resolution raster grids
illustrating snow and bare-ice surfaces, and snowline shape
files can be downloaded via CryoClim. Here, we describe the
snowline classification algorithm, its validation and its inter-
annual variations for 18 years spanning 2000–2017.
Snowline classification algorithm
We processed all MODIS MOD12KM and MOD03 scenes
covering Greenland from late July to the beginning of Sep-
tember 2000–2017. We used the surface-type detection algo-
rithm of Fausto et al. (2015) that distinguishes between bare-
ice and snow surfaces. Fausto et al. (2015) uses normalised
thresholds (Th) from calibrated radiances (MOD021KM)
between the near-infrared band 5 (1230–1250 nm) and the
visible band 10 (483–493 nm) with surface-type thresholds
Th
dry snow
≤0.86, 0.86
265–2.1×LAT, where LAT is latitude. Th
bare ice
is defined as:
T h
b a r e i c e
= c 0 + c 1 × b 1+ c 2 × b 2 + c 3 × b 3 + c 5 × b 5 + c 7 × b 7
where c0=–0.0015, c1=0.160, c2=0.291, c3=0.243, c5=
0.112, c7=0.081 and b1 to b 7 designate band 1 to band 7.
Cloud-covered regions are removed using the MOD35_L2
dataset. Subsequently pixels are classified for every MODIS
scene as either snow or bare ice for the whole Greenland ice
sheet.
Daily classification scenes are aggregated to yield a maxi-
mum extent of bare ice to define an end-of-melt-season
snowline. Snowlines from peripheral glaciers are generally
excluded, and the snowline products are based on an algo-
rithm success rate of over 95% classified pixels.
Validation
To help validate the MODIS data we make use of the PROM-
ICE automatic weather station network that currently con-
sists of two or three stations primarily in the ablation area
in eight ice sheet regions. Each automatic weather station
records a suite of meteorological and glaciological measure-
ments, supplemented by e.g. surface-height changes due to
accumulation or ablation (Fig. 1; Van As et al. 2016).
To validate the classified snowline elevation at the end
of the melt season, we use the mass-budget values from the
PROMICE weather stations (Fig. 2; e.g. Fausto et al. 2012) at
different elevations to calculate the vertical surface mass-bal-
ance gradient for all eight PROMICE transects to determine
the equilibrium line altitude (ELA, zero mass budget), for di-
rect comparison with MODIS estimated snowline elevation
(Fig. 1). AWS balance profiles from the Upernavik region,
and those indicating an ELA above 2000 m are excluded as
we find them unrealistic. The location of the upper AWS
should be close to the actual ELA to get the best balance pro-
files. In total, we exclude 25% or 17 out of 67 balance profiles.
Fig. 2. South Greenland PROMICE automatic
weather station at the end of the 2013 melt
season. From the stakes to the left of the weather
station, the amount of melt (c. 4 m) is directly
visible. The melt is also measured with a pres-
sure transducer system drilled into the ice.
73
Figure 3 illustrates the performance of the MODIS end-of-
melt-season snowline algorithm for all PROMICE regions in
Greenland. The correlation (r=90%, p=0.0001, n=50) and
the root-mean-square error (RMSE=200 m) are reasonable
as the ELA and snowline elevation can be different due to
superimposed ice formation (Cogley 2011). The mean differ-
ence between snowline altitude and ELA is −104 m.
Results and discussion
Figure 1 illustrates the location of remotely sensed snowline
plotted on top of the digital elevation model (DEM) from
the Greenland Ice Mapping Project (GIMP, Howat et al.
2014). The snowline is easily visible in the southern, western,
and northern parts of Greenland due to the relatively even
terrain, while the snowline shows a more complicated pat-
tern in the mountainous terrain in East Greenland (Fig. 1).
The snowline separates bare ice from snow areas and can
therefore be used to document the change in bare-ice areas.
We find the extent of bare-ice exposure to be increasing in
the period 2000–2017 at an average rate of c. 500 km2 per
year (Fig. 4), which roughly corresponds to the size of the
Danish island of Bornholm. This increase in the bare-ice
area is insignificant, but it demonstrates a small average gain
of melt over accumulation since 2000. The increasing trend
in the bare-ice area is consistent with increasing Greenland
mass loss due to surface processes (Van den Broeke et al.
2017). Both independent, in situ observations (Machguth et
al. 2016) and remotely sensed observations (Hall et al. 2012;
Tedesco et al. 2017) show that the Greenland melt area is ex-
panding to higher elevations. Further, the increase in bare ice
enhances the positive feedback mechanism of a darkening ice
sheet surface (ice is darker than snow), which affects the sur-
face mass and energy balance of the Greenland ice sheet (Box
et al. 2012). Figure 4 also illustrates the inter-annual variabil-
ity of the 2000–2017 snowlines, which is highly dependent
on the complicated seasonal weather systems around Green-
land. For instance, the below average snowline of the snowy
year of 2016/2017 is consistent with positive albedo anoma-
lies that reduced melting in 2017 (Tedesco et al. 2017).
Uncertainties associated with the different surface-type
detection are assessed with the ELAs derived from the AWS
surface mass-budget observations. Figure 3 shows a signifi-
cant correlation between the MODIS snowline and ELAs
derived independently from PROMICE AWSs. A reason for
the difference between the two can be that the MODIS data
have a spatial resolution of 1 km2, pan-ice sheet coverage and
quasi-daily temporal coverage, while the footprints of the in
situ measurements are small (5–50 m2), and surface patchi-
ness is clear in aerial photography (Stroeve et al. 2006).
Fausto et al. (2015) discuss an August anomaly in their
monthly surface-type data set during the 2010–2014 peri-
od, illustrated by a noisy melting-snow classification in the
northern ice sheet, which was most likely due to false clas-
sification. However, with the updated bare-ice threshold,
we improve the detection of snow and ice surfaces (Fig. 1),
visualised by a less noisy snow classification of snow in the
northern part of the ice sheet, resulting in a more reliable cli-
mate indicator for Greenland.
Conclusions
Remotely sensed MODIS data can yield daily, automated
classification of the Greenland ice sheet surface type (snow
and ice). Validation indicates a high correlation (0.9) be-
tween MODIS-derived snowline altitudes and ELAs esti-
mated from in situ measurements. The end-of-melt-season
1000 1500
1700
1500
1300
1100
900
700
500
Automatic weather station ELA (m a.s.l.)
KPC
SCO
TAS
QAS
NUK
KAN
UPE
THUSn
ow
lin
e
el
ev
at
io
n
(m
a
.s.
l.)
500
2004 2009 2014
190 000
170 000
150 000
130 000
110 000
90 000
70 000
Year
A
re
a
(k
m
)
1999
2
Bare-ice area y = 504x – 879029
Fig. 3. The end-of-melt-season snowline elevation for 2000 to 2017 from
MODIS vs. the PROMICE AWS-derived equiblibrium line altitude
(ELA). The blue line gives the 1:1 relation. The locations of the PRO-
MICE automatic weather stations are shown in Fig. 1.
Fig. 4. End-of-melt-season bare-ice area for the Greenland ice sheet for the
years 2000–2017.
7474
snowline is useful as an ice-sheet climate indicator for the
competing processes of surface accumulation and ablation,
quantified by an average annual increase of c. 500 km2 of the
bare-ice area for the 2000–2017 period.
Acknowledgements
The Programme for Monitoring of the Greenland Ice Sheet (PROMICE)
is funded by the Geological Survey of Denmark and Greenland (GEUS)
and the Danish Ministry of Energ y, Utilities and Climate under the
Danish Cooperation for Environment in the Arctic (DANCEA), and is
conducted in collaboration with DTU Space, Denmark’s National Space
Institute, and Asiaq (Greenland Survey). The NUK and K AN stations
were/are (co-)funded by the Greenland Climate Research Centre (GCRC)
and the Greenland Analogue Project (GAP), respectively. This study was
funded by DK ESA-PRODEX under the CryoClim project.
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Authors’ address
Geological Survey of Denmark and Greenland, Øster Voldgade 10, DK-1350 Copenhagen K, Denmark. E-mail: rsf@geus.dk.
http://dx.doi.org/10.5194/tc-8-1509-2014
http://dx.doi.org/10.5194/tc-8-1509-2014
http://dx.doi.org/10.1088/0034-4885/78/4/046801
http://dx.doi.org/10.1088/0034-4885/78/4/046801
http://dx.doi.org/10.1038/nclimate2899
http://dx.doi.org/10.1038/nclimate2899
http://dx.doi.org/10.1038/nclimate2554
http://dx.doi.org/10.1016/j.rse.2006.06.009
http://dx.doi.org/10.1016/j.rse.2006.06.009
http://dx.doi.org/10.1007/s40641-017-0084-8
mailto:rsf@geus.dk
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