资源环境科技发展态势分析平台

Fohn winds are warm, strong, downslope winds on the leeside of mountains, which can last from several hours to a few days. The years 1995 and 2002 saw the dramatic breakup of huge parts of the Larsen Ice Shelf (LIS) on the east of the Antarctic Peninsula. It is widely accepted that hydrofracturing, the widening of crevasses due to the excess hydrostatic pressure exerted by meltwater which accumulates inside them, is the mechanism behind the breakup of the Larsen A and Larsen B ice shelves. On the LIS, in the lee of the mountain range that runs along the spine of the Antarctic Peninsula, Fohn winds are thought to provide the atmospheric conditions for significant warming over the ice shelf, leading to the initial firn densification, and subsequently providing the melt water for hydrofracturing. Measurements provide evidence that in some cases Fohn events reach an Automatic Weather Station on the LIS at over 100 km distance. In this paper, we examine the representation of Fohn events during 2011 as they were observed in measurements by an Automatic Weather Station and in simulations with the Weather Research and Forecasting Model as run for the Antarctic Mesoscale Prediction System (AMPS). We find that, while the model generally simulates meteorological parameters very well and shows good skill in capturing the occurrence, frequency, and duration of Fohn events, it underestimates the temperature increase and humidity decrease during the Fohn significantly and may thus underestimate the contribution of Fohn to driving surface melt on LIS.