TY - JOUR
T1 - Extent of low accumulation 'wind glaze' areas on the East Antarctic plateau: implications for continental ice mass balance
AU - Scambos, T.
AU - Frezzotti, M.
AU - Lenaerts, J.T.M.
AU - van den Broeke, M.R.
AU - Winther, J.G.
PY - 2012
Y1 - 2012
N2 - Persistent katabatic winds form widely distributed localized areas of near-zero net surface
accumulation on the East Antarctic ice sheet (EAIS) plateau. These areas have been called ‘glaze’
surfaces due to their polished appearance. They are typically 2–200km2 in area and are found on
leeward slopes of ice-sheet undulations and megadunes. Adjacent, leeward high-accumulation regions
(isolated dunes) are generally smaller and do not compensate for the local low in surface mass balance
(SMB). We use a combination of satellite remote sensing and field-gathered datasets to map the extent
of wind glaze in the EAIS above 1500m elevation. Mapping criteria are derived from distinctive surface
and subsurface characteristics of glaze areas resulting from many years of intense annual temperature
cycling without significant burial. Our results show that 11.2 1.7%, or 950 143 103 km2, of the
EAIS above 1500m is wind glaze. Studies of SMB interpolate values across glaze regions, leading to
overestimates of net mass input. Using our derived wind-glaze extent, we estimate this excess in three
recent models of Antarctic SMB at 46–82 Gt. The lowest-input model appears to best match the mean in
regions of extensive wind glaze.
AB - Persistent katabatic winds form widely distributed localized areas of near-zero net surface
accumulation on the East Antarctic ice sheet (EAIS) plateau. These areas have been called ‘glaze’
surfaces due to their polished appearance. They are typically 2–200km2 in area and are found on
leeward slopes of ice-sheet undulations and megadunes. Adjacent, leeward high-accumulation regions
(isolated dunes) are generally smaller and do not compensate for the local low in surface mass balance
(SMB). We use a combination of satellite remote sensing and field-gathered datasets to map the extent
of wind glaze in the EAIS above 1500m elevation. Mapping criteria are derived from distinctive surface
and subsurface characteristics of glaze areas resulting from many years of intense annual temperature
cycling without significant burial. Our results show that 11.2 1.7%, or 950 143 103 km2, of the
EAIS above 1500m is wind glaze. Studies of SMB interpolate values across glaze regions, leading to
overestimates of net mass input. Using our derived wind-glaze extent, we estimate this excess in three
recent models of Antarctic SMB at 46–82 Gt. The lowest-input model appears to best match the mean in
regions of extensive wind glaze.
U2 - 10.3189/2012JoG11J232
DO - 10.3189/2012JoG11J232
M3 - Article
SN - 0022-1430
VL - 58
SP - 633
EP - 647
JO - Journal of Glaciology
JF - Journal of Glaciology
IS - 210
ER -