Abstract
The occurrence of Antarctic ablation areas in Dronning Maud Land, the Lambert
Glacier Basin, Victoria Land, the Transantarctic Mountains and the Antarctic Peninsula is
realistically predicted by the regional atmospheric climate model RACMO2/ANT, with
snowdrift-related processes calculated offline. Antarctic ablation areas are characterized
by a low solid precipitation flux in combination with strong sublimation, snowdrift erosion
and/or melt. The strong interaction between atmospheric circulation and topography plays
a decisive role in the precipitation distribution and hence that of ablation areas. Three
types of Antarctic ablation areas can be distinguished, all occurring in dry regions: Type 1
is the erosion-driven ablation area, caused by 1-D and/or 2-D divergence in the katabatic
wind field at high elevations (2000–3200 m asl). Type 2 is the sublimation-driven ablation
area. This type occurs at lower elevations (
Original language | Undefined/Unknown |
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Pages (from-to) | D18110/1-D18110/14 |
Number of pages | 14 |
Journal | Journal of Geophysical Research: Atmospheres |
Volume | 111 |
Publication status | Published - 2006 |