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On the Radiation Characteristics of
Antarctic Sea Ice
Gerd Wendler1, Blake
Moore2, Dorte Dissing2 and John
Kelley2
1 Dept. of Geography, University of
Canterbury, Christchurch, New Zealand
2 Geophysical Institute, University of Alaska, Fairbanks,
Alaska, USA
Abstract
Radiative measurements were carried out continuously
during a cruise from Australia to Antarctica during
austral summer 1995/96. Both short-wave and long-wave
radiative fluxes were measured. Some of the results
are:
- The incoming solar radiation had a mean value of 217
Wm-2; this was a relatively weak value due to the large
amount of fractional cloud cover observed. The sun was
for a large part of the trip, above the horizon for 24
hours a day.
- The reflectivity varied widely, not only as function
of sea ice concentration, but also as function of ice
type.
- Snow covered pack ice gave the highest albedo values
(Å 70%), while flooded sea ice and thin ice reflected
much less (Å 30%).
- For each sea ice type, short term observations showed
a good relationship between albedo and ice
concentration.
- The albedo increased with decreasing solar
elevation.
- The net long wave radiation was negative (mean -27
Wm-2); this small value is due to a high amount of
fractional cloud cover. There was a weak diurnal
variation with a maximum loss (-33 Wm-2) in the early
afternoon.
- On the average, the net radiation was positive for 17
hours, and negative for 7 hours a day. However, the
duration of a positive balance depended strongly on the
surface albedo.
- 2. For the observed albedo values, modeling results
showed that the net radiation was always positive when
averaged over a day. The magnitude, however, depended
strongly on the surface albedo, varying by more than the
factor of three.
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