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Constraining Millennial‐Scale Changes in Northern Component Water Ventilation in the Western Tropical South Atlantic
Author(s) -
Campos Marília C.,
Chiessi Cristiano M.,
Venancio Igor M.,
Pinho Tainã M.L.,
Crivellari Stefano,
Kuhnert Henning,
Schmiedl Gerhard,
Díaz Rut A.,
Albuquerque Ana Luiza S.,
PortilhoRamos Rodrigo C.,
Bahr André,
Mulitza Stefan
Publication year - 2020
Publication title -
paleoceanography and paleoclimatology
Language(s) - English
Resource type - Journals
SCImago Journal Rank - 1.927
H-Index - 127
eISSN - 2572-4525
pISSN - 2572-4517
DOI - 10.1029/2020pa003876
Subject(s) - stadial , geology , oceanography , north atlantic deep water , glacial period , holocene , climatology , thermohaline circulation , paleontology
Negative excursions in the stable carbon isotopic composition (δ 13 C) at Atlantic intermediate to mid‐depths are common features of millennial‐scale events named Heinrich Stadials. The mechanisms behind these excursions are not yet fully understood, but most hypotheses agree on the central role played by the weakening of the Atlantic meridional overturning circulation. Marine records registering millennial‐scale negative δ 13 C excursions in the Atlantic are mostly restricted to the Heinrich Stadials of the last deglacial, while the Heinrich Stadials of the last glacial are poorly studied. Here, we constrain changes in bottom water ventilation in the western tropical South Atlantic mid‐depth during Heinrich Stadials of the last glacial and deglacial by investigating marine core M125‐95‐3. The concurrent decreases in benthic foraminifera δ 13 C and increases in bulk sediment sulfur indicate an increased Northern Component Water (NCW) residence time in the western tropical South Atlantic mid‐depth during Heinrich Stadials. Furthermore, a coherent meridional pattern emerges from the comparison of our new data to previously published mid‐depth records from the western South Atlantic. While our record shows the largest negative δ 13 C excursions during almost all Heinrich Stadials, the western equatorialAtlantic showed medium and the subtropical South Atlantic showed the smallest negative excursions. This meridional pattern supports the notion that during Heinrich Stadials, a reduction in the NCW δ 13 C source signal together with the accumulation of respired carbon at NCW depths drove the negative δ 13 C excursions. We suggest that the negative δ 13 C excursions progressively increase along the NCW southwards pathway until the signal dissipates/dilutes by mixing with Southern Component Water.