The new Kr-86 excess ice core proxy for synoptic activity: West Antarctic storminess possibly linked to Intertropical Convergence Zone (ITCZ) movement through the last deglaciation
Here we present a newly developed ice core gas-phase proxy that directly samples a component of the large-scale atmospheric circulation: synoptic-scale pressure variability. Surface pressure changes weakly disrupt gravitational isotopic settling in the firn layer, which is recorded in krypton-86 exc...
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Published in | Climate of the past Vol. 19; no. 3; pp. 579 - 606 |
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Main Authors | , , , , , , , , , , , , , , , , , , , , |
Format | Journal Article |
Language | English |
Published |
Katlenburg-Lindau
Copernicus GmbH
15.03.2023
European Geosciences Union (EGU) Copernicus Publications |
Subjects | |
Online Access | Get full text |
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Summary: | Here we present a newly developed ice core gas-phase proxy that directly samples a component of the large-scale atmospheric circulation: synoptic-scale pressure variability. Surface pressure changes weakly disrupt gravitational isotopic settling in the firn layer, which is recorded in krypton-86 excess (.sup.86 Kr.sub.xs). The .sup.86 Kr.sub.xs may therefore reflect the time-averaged synoptic pressure variability over several years (site "storminess"), but it likely cannot record individual synoptic events as ice core gas samples typically average over several years. We validate .sup.86 Kr.sub.xs using late Holocene ice samples from 11 Antarctic ice cores and 1 Greenland ice core that collectively represent a wide range of surface pressure variability in the modern climate. We find a strong spatial correlation (r=-0.94, p<0.01) between site average .sup.86 Kr.sub.xs and time-averaged synoptic variability from reanalysis data. The main uncertainties in the analysis are the corrections for gas loss and thermal fractionation and the relatively large scatter in the data. Limited scientific understanding of the firn physics and potential biases of .sup.86 Kr.sub.xs require caution in interpreting this proxy at present. We show that Antarctic .sup.86 Kr.sub.xs appears to be linked to the position of the Southern Hemisphere eddy-driven subpolar jet (SPJ), with a southern position enhancing pressure variability. |
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ISSN: | 1814-9332 1814-9324 1814-9332 |
DOI: | 10.5194/cp-19-579-2023 |