Abstract. Surface snow in polar and mountainous regions is often mobile
and this mobility influences surface mass balance and isotopic composition
before final deposition, which is poorly understood thus far. In
December 2016 and January 2017, during a field campaign in Queen Maud Land,
Antarctica, a snowfall and subsequent drifting snow events were recorded by
meteorological and drifting snow stations. Associated small-scale topography
changes and snow hardness changes were measured by terrestrial laser scanning
and with a SnowMicroPen. The polar field measurements show that drifting snow
is necessary for wind packing and thereby confirm previous findings from wind
tunnel experiments. However, the snow hardness in Antarctica was
significantly higher than what was achieved in the wind tunnel. This is most
likely due to higher wind speeds and more intense saltation in the natural
environment. As in the wind tunnel, no influence of time at a scale of days
was observed on the hardness. This suggests that time and sintering are not
the dominating processes in wind packing but that the impact compaction at
the moment of deposition may be more important. Furthermore, it is
quantitatively demonstrated how the reorganization of fresh snow into barchan
dunes during subsequent drifting snow events is accompanied by significant
increases in surface hardness at all locations on the dune. However, with the
available data, the hardness variability on the dune could not be explained
satisfactorily. In particular and unlike in the wind tunnel, there was no
correlation between the hardness and the wind exposure parameter Sx. This is
most likely because the measurements of hardness and the wind exposure
situation were not simultaneous. This shows that highly temporally resolved
snow depth data are necessary to investigate wind packing in more detail.
These results form an important step in understanding how drifting snow links
precipitation to deposition via snow hardening.