Atlantic Meridional Overturning Circulation during Heinrich-Stadial 1 & 2 as seen by 231Pa/230Th
Abstract:
The sedimentary activity ratio 231Pa/230Th has been increasingly used as a kinematic circulation proxy in the Atlantic Ocean over the past decade [Gherardi et al. 2009; McManus et al. 2004; Lippold et al. 2012]. Here we present 231Pa/230Th ratios from several Atlantic sediment cores across Heinrich Events 1 (~17 ka BP) and 2 (~24 ka BP). The comparison of the profiles demonstrates the potential pitfalls when interpreating a single 231Pa/230Th profile. E. g. core IODP 1313 (Mid Atlantic Ridge, 3412 m water depth) shows 231Pa/230Th between 0.04 and 0.06, which would indicate a vigorous circulation over the entire time period. On the other hand core GeoB 16202-2 (Brasilan coastal area, 2248 m water depth) has a profile similar to the well known data set of [McManus et al. 2004] (i.e. during Heinrich Stadials values close to the production ratio of ~0.093, lower values at Holocene and LGM).
Such divergency can be explained by 231Pa/230Th dependence on water depth, latitude, water mass and water mass age [Luo et al. 2010; Lippold et al. 2011], but also on changes in bioproductivity especially the flux of biogenic opal [Anderson et al. 1983A; Bradtmiller et al. 2007; Chase et al. 2002]. To avoid misleading interpretations, the here shown data set is accompanied by measurements of biogenic opal contents to appraise possible influences on the proxies. We observe large variations of opal contents - up to 10% at location IODP 1314 (close to Iceland, 2899 m water depth) in contrast to GeoB 16202-2 with an average of about 1-2% - and with a few data points showing correlation with 231Pa/230Th.
With an inverse model approach [Luo et al. 2010] strength of the AMOC before, during and after the Heinrich-Stadials 1 & 2 will be derived from this database.
