Articles | Volume 15, issue 4
https://doi.org/10.5194/cp-15-1537-2019
https://doi.org/10.5194/cp-15-1537-2019
Research article
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08 Aug 2019
Research article | Highlight paper |  | 08 Aug 2019

Spatial pattern of accumulation at Taylor Dome during Marine Isotope Stage 4: stratigraphic constraints from Taylor Glacier

James A. Menking, Edward J. Brook, Sarah A. Shackleton, Jeffrey P. Severinghaus, Michael N. Dyonisius, Vasilii Petrenko, Joseph R. McConnell, Rachael H. Rhodes, Thomas K. Bauska, Daniel Baggenstos, Shaun Marcott, and Stephen Barker

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Status: closed
AC: Author comment | RC: Referee comment | SC: Short comment | EC: Editor comment
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Peer-review completion

AR: Author's response | RR: Referee report | ED: Editor decision
ED: Reconsider after major revisions (30 Nov 2018) by Denis-Didier Rousseau
AR by Anna Wenzel on behalf of the Authors (19 Feb 2019)  Author's response
ED: Referee Nomination & Report Request started (19 Feb 2019) by Denis-Didier Rousseau
RR by Anonymous Referee #2 (25 Feb 2019)
RR by Anonymous Referee #3 (27 Feb 2019)
RR by Anonymous Referee #1 (13 Mar 2019)
RR by Anonymous Referee #4 (30 Jun 2019)
ED: Publish subject to technical corrections (01 Jul 2019) by Denis-Didier Rousseau
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Short summary
An ice core from Taylor Glacier, Antarctica, spans a period ~ 70 000 years ago when Earth entered the last ice age. Chemical analyses of the ice and air bubbles allow for an independent determination of the ages of the ice and gas bubbles. The difference between the age of the ice and the bubbles at any given depth, called ∆age, is unusually high in the Taylor Glacier core compared to the Taylor Dome ice core situated to the south. This implies a dramatic accumulation gradient between the sites.