Deep and intermediate water mass history of the Western Indian Ocean
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Abstract
This research focuses on reconstructing the history of various oceanic conditions,
ranging from surface to deep layers, in the Western Indian Ocean over the last
glacial cycle.
A new data set is presented, composed of various palaeoceanographic proxies
from marine sediment cores 64PE304-8 (752m), 64PE303-16 (1350m) and 64PE303-
15 (1985m) retrieved along a depth transect during the “Tropical Temperature History
During Paleogene Global Warming Events” (GLOW) ? and “Indian – Atlantic
Exchange” (INATEX) ? expeditions of the research vessel Pelagia.
Interpretation of this new data, forming a vertical transect of geochemical proxies
of terrigenous hydrological change and foraminiferal stable isotope records anchored
in robust radiocarbon based age models, provides a significant contribution
to an area of poor data coverage in the western Indian Ocean.
Geochemical records of eastern African hydrological change provide a record
of monsoon driven rainfall changes. We show that orbitally driven cycles in the
log (Ti/Ca) series are a direct response to regional equatorial insolation. We notice
that the structure of the precessionally driven cycles shows no similarity with the
widely cited monsoonal influenced Chinese cave speleothem records (??). The offshore
Tanzanian records show a remarkable resemblance with the newly published
Borneo cave speleothem record (?), both likely driven by near regional equatorial
insolation patterns.
Millennial scale events are strongly manifest in the log(Ti/Ca) series in intervals
where sedimentation rates are relatively high, punctuating the longer-term
precessionally driven cycles. The log(Ti/Ca) series show a number of distinct dry
events, which occurred synchronously with the northern hemisphere cold Heinrich
events. The data show a strong coupling between changes in monsoon rainfall offshore
Tanzania and the northern hemisphere Heinrich cold events, likely mediated
by the average position of the intertropical convergence zone.
The stable isotope data helps our understanding of variability of surface, intermediate
and deep ocean circulation in the western Indian Ocean on the millennial
time-scale. The depth transect approach allows us to investigate time offsets between
the individual stable isotope records of the surface, intermediate and deep
waters during the late glacial-Holocene cycle. The time off sets are useful indicators
of connections between changes in western Indian Ocean water masses and climate
change in the high latitudes. Our new data highlights significant differences across
the water column in the timing of deglaciation. We can robustly report that the
intermediate depth ocean in the region of our cores was the first to record an oxygen
isotope signal of the deglaciation. The rate of change records calculated further
show the offsets and elucidate the apparent relationship between our surface
records and Greenland in terms of timing of change.
The records presented here are also placed in a broader Indian Ocean/Arabian
sea context to asses to role of the intermediate depths of the Indian Ocean in millennial
scale change, particularly during Heinrich events. Using the combined insights
provided by the new δ18O and δ13C records, the new transect of records highlights
changes in the nature of intermediate depth Indian Ocean circulation changes over
the last 40kyr. This contributes to the discussion of the origin of the oxygenation
pulses in the Arabian Sea, that either reflect local changes in intermediate water
properties, or indeed bear evidence of a larger, Indian Ocean wide expansion of
glacial Antarctic Intermediate water. The new data are combined with published
data to assess modes of ocean circulation in the Indian Ocean. This helps to elucidate
the role played by this part of the global ocean system in the millennial-scale
climate shifts - including the bipolar seesaw phenomenon - that occurred during
this time period.
In particular, two valuable insights into past changes in ocean circulation in the
western Indian Ocean are presented, with important implications for our understanding
of the role of ocean circulation in millennial scale and deglacial climate
shifts. First, our new data supports the notion of expanded glacial AAIW at intermediate
depths within the Indian Ocean during Heinrich events. Second, we see
evidence of a deglacial reorganistaion of the ventilation pattern in the region across
the deglaciation. This involves an chemically aged watermass reaching the upper
1000m of the western Indian Ocean via the Indonesian Through-flow and the SEC.
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