2006
DOI: 10.1016/j.quascirev.2005.06.007
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Firn-air δ15N in modern polar sites and glacial–interglacial ice: a model-data mismatch during glacial periods in Antarctica?

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Cited by 109 publications
(138 citation statements)
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“…Our new results would suggest that we can expect softening and faster densification than assumed in the model. However, δ 15 N 2 measurements performed on glacial Greenland ice, which reflect the changes in the diffusive column length of the firn, agree rather well with the firn depth predicted by firnification models (Landais et al, 2006). This apparently limits the influence of Ca ++ concentrations on glacial densification in Greenland.…”
Section: Discussionsupporting
confidence: 59%
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“…Our new results would suggest that we can expect softening and faster densification than assumed in the model. However, δ 15 N 2 measurements performed on glacial Greenland ice, which reflect the changes in the diffusive column length of the firn, agree rather well with the firn depth predicted by firnification models (Landais et al, 2006). This apparently limits the influence of Ca ++ concentrations on glacial densification in Greenland.…”
Section: Discussionsupporting
confidence: 59%
“…The observed development of seasonal cycles in density, which increase with depth and which follow the Ca++ seasonality, shows that strong seasonal cycles in impurities can induce a seasonal cycle in firn density unrelated to the temperature. This contradicts the hypothesis that the deep firn seasonal density cycle is induced by temperature at the surface (for example Landais et al, 2006;Zwally and Li, 2002). The relative maximum in density variability in deeper firn (Freitag et al, 2004;Gerland et al, 1999;Hörhold et al, 2011) can likely be attributed to the impurity effect.…”
Section: Discussionmentioning
confidence: 75%
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“…δ 15 N of N 2 ). Our precision for the gravitational correction of 0.05 ‰ per mass unit obtained from δ 136 Xe is lower than the results from a dedicated system for δ 15 N (Landais et al, 2006), yet sufficient for our purpose here. Note that using δ 136 Xe to correct for gravitational effects of any gas species in the firn column assumes that the gravitational enrichment of the gases in the firn column is only dependent on the absolute mass difference of two species.…”
Section: Xenon-based Mixing Ratiosmentioning
confidence: 69%