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dc.contributor.authorRusson, T
dc.contributor.authorTudhope, AW
dc.contributor.authorCollins, Matthew
dc.contributor.authorHegerl, GC
dc.date.accessioned2016-04-05T10:15:19Z
dc.date.issued2015-01-10
dc.description.abstractOne common approach to investigating past changes in El Niño–Southern Oscillation (ENSO) amplitude is through quantifying the variance of ENSO-influenced proxy records. However, a component of the variance of all such proxies will reflect influences that are unrelated to the instrumental climatic indices from which modern ENSO amplitudes are defined. The unrelated component of proxy variance introduces a fundamental source of uncertainty to all such constraints on past ENSO amplitudes. Based on a simple parametric approach to modeling this uncertainty, we present guidelines for the magnitudes of proxy variance change required to robustly infer the following: (i) any change at all in ENSO amplitude and (ii) a change in ENSO amplitude that exceeds the plausible range of unforced variability. It is noted that more extreme changes in proxy variance are required to robustly infer decreases, as opposed to increases, in past ENSO amplitude from modern levels.en_GB
dc.description.sponsorshipThis work was funded through NERC grant NE/H009957/1.en_GB
dc.identifier.citationVolume 42, Issue 4, pp. 1197–1204en_GB
dc.identifier.doi10.1002/2014GL062331
dc.identifier.urihttp://hdl.handle.net/10871/20970
dc.language.isoenen_GB
dc.publisherWileyen_GB
dc.relation.urlhttp://hdl.handle.net/10871/19727
dc.rightsThis is an open access article under the terms of the Creative Commons Attribution License, which permits use, distribution and reproduction in any medium, provided the original work is properly cited.en_GB
dc.titleInferring changes in ENSO amplitude from the variance of proxy recordsen_GB
dc.typeArticleen_GB
dc.date.available2016-04-05T10:15:19Z
dc.identifier.issn0094-8276
dc.descriptionThis is the final version of the article. Available from Wiley via the DOI in this record.en_GB
dc.descriptionThere is another ORE record for this article: http://hdl.handle.net/10871/19727
dc.identifier.eissn1944-8007
dc.identifier.journalGeophysical Research Lettersen_GB


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