Abstract: The nitrogen stable isotopic composition in nitrate (δ15N-NO−3) measured in ice cores from low-snow-accumulation regions in East Antarctica has the potential to provide constraints on past ultraviolet (UV) radiation and thereby total column ozone (TCO) due to the sensitivity of nitrate (NO−3) photolysis to UV radiation. However, understanding the transfer of reactive nitrogen at the air–snow interface in polar regions is paramount for the interpretation of ice core records of δ15N-NO−3 and NO−3 mass concentrations. As NO−3 undergoes a number of post-depositional processes before it is archived in ice cores, site-specific observations of δ15N-NO−3 and air–snow transfer modelling are necessary to understand and quantify the complex photochemical processes at play. As part of the Isotopic Constraints on Past Ozone Layer Thickness in Polar Ice (ISOL-ICE) project, we report new measurements of NO−3 mass concentration and δ15N-NO−3 in the atmosphere, skin layer (operationally defined as the top 5 mm of the snowpack), and snow pit depth profiles at Kohnen Station, Dronning Maud Land (DML), Antarctica. We compare the results to previous studies and new data, presented here, from Dome C on the East Antarctic Plateau. Additionally, we apply the conceptual 1D model of TRansfer of Atmospheric Nitrate Stable Isotopes To the Snow (TRANSITS) to assess the impact of NO−3 recycling on δ15N-NO−3 and NO−3 mass concentrations archived in snow and firn. We find clear evidence of NO−3 photolysis at DML and confirmation of previous theoretical, field, and laboratory studies that UV photolysis is driving NO−3 recycling and redistribution at DML. Firstly, strong denitrification of the snowpack is observed through the δ15N-NO−3 signature, which evolves from the enriched snowpack (−3 ‰ to 100 ‰), to the skin layer (−20 ‰ to 3 ‰), to the depleted atmosphere (−50 ‰ to −20 ‰), corresponding to mass loss of NO−3 from the snowpack. Based on the TRANSITS model, we find that NO−3 is recycled two times, on average, before it is archived in the snowpack below 15 cm and within 0.75 years (i.e. below the photic zone). Mean annual archived δ15N-NO−3 and NO−3 mass concentration values are 50 ‰ and 60 ng g−1, respectively, at the DML site. We report an e-folding depth (light attenuation) of 2–5 cm for the DML site, which is considerably lower than Dome C. A reduced photolytic loss of NO−3 at DML results in less enrichment of δ15N-NO−3 than at Dome C mainly due to the shallower e-folding depth but also due to the higher snow accumulation rate based on TRANSITS-modelled sensitivities. Even at a relatively low snow accumulation rate of 6 cm yr−1 (water equivalent; w.e.), the snow accumulation rate at DML is great enough to preserve the seasonal cycle of NO−3 mass concentration and δ15N-NO−3, in contrast to Dome C where the depth profiles are smoothed due to longer exposure of surface snow layers to incoming UV radiation before burial. TRANSITS sensitivity analysis of δ15N-NO−3 at DML highlights that the dominant factors controlling the archived δ15N-NO−3 signature are the e-folding depth and snow accumulation rate, with a smaller role from changes in the snowfall timing and TCO. Mean TRANSITS model sensitivities of archived δ15N-NO−3 at the DML site are 100 ‰ for an e-folding depth change of 8 cm, 110 ‰ for an annual snow accumulation rate change of 8.5 cm yr−1 w.e., 10 ‰ for a change in the dominant snow deposition season between winter and summer, and 10 ‰ for a TCO change of 100 DU (Dobson units). Here we set the framework for the interpretation of a 1000-year ice core record of δ15N-NO−3 from DML. Ice core δ15N-NO−3 records at DML will be less sensitive to changes in UV than at Dome C; however the higher snow accumulation rate and more accurate dating at DML allows for higher-resolution δ15N-NO−3 records.

Abstract: Aim. Dispersal explains the disjunct distributions of many austral plant lineages.
However, the role of Antarctica is largely uncertain and the routes of
dispersal have remained speculative. Based on niche conservatism we can make
predictions about the timing of disjunction establishment, as well as the availability
of direct transoceanic, Antarctic stepping-stone, and out-of-Antarctica
dispersal routes over time. We evaluate these predictions using molecular
divergence time estimates for the establishment of disjunct distributions across
multiple plant lineages.
Location. Southern Hemisphere.
Methods. We estimated the timing of disjunction establishment and determined
habitat affinities for 72 austral plant groups. We used Wilcoxon rank
sum tests to compare the timing of disjunction establishment between cold
and temperate climate lineages for the full data set, as well as within several
subsets. We compared our results with those from a literature survey.
Results. As niche conservatism predicts, the timing of disjunction establishment
in cold and temperate climate austral lineages is consistent with the availability
of the corresponding habitats over time. Our results also suggest that
disjunction establishment has involved a combination of Antarctic and direct
dispersal routes. For cold climate lineages, both out-of-Antarctica and direct
dispersal routes are required to explain the observed estimates, while stepping
stone routes cannot be ruled out. It appears that for these lineages the importance
of the three dispersal routes differs with environmental, geographical and
temporal context.
Main conclusions. Both direct and Antarctic dispersal routes are necessary to
explain the establishment of contemporary austral distributions. Evidence that
some taxa were, until recently, restricted to Antarctica changes how we view
the evolutionary histories of austral floras and the lineages they contain. Moreover,
that we detect differences in the importance of alternative dispersal routes
suggests that long-distance plant dispersal processes can be explicitly incorporated
into models of climate change response.

Abstract: invited seminar