Radiocarbon ages and plateau definitions of sediments from the abyssal ocean

Ice core records demonstrate a glacial-interglacial atmospheric CO2 increase by ~100 ppm, while 14C calibration efforts document a strong decrease in atmospheric 14C concentration during this period. A calculated transfer of ~530 Gt of 14C depleted carbon is required to produce the deglacial coeval rise of carbon in the atmosphere and terrestrial biosphere. This amount is usually ascribed to oceanic carbon release, although the actual mechanisms remained elusive, since an adequately old and carbon-enriched deep-ocean reservoir seemed unlikely. Here we present a new, though still fragmentary, ocean-wide d14C dataset showing that during the Last Glacial Maximum (LGM) and Heinrich Stadial 1 (HS-1) the maximum 14C age difference between ocean deep waters and the atmosphere exceeded the modern values by up to 1500 14C yr, in the extreme reaching 5100 14C yr. Below 2000 m depth the 14C ventilation age of modern ocean waters is directly linked to the concentration of dissolved inorganic carbon (DIC). We propose as working hypothesis that the modern regression of DIC vs d14C also applies for LGM times, which implies that a mean LGM aging by ~600 14C yr corresponded to a global rise of ~85-115 µmol DIC/kg in the deep ocean. Thus, the prolonged residence time of ocean deep waters may indeed have made it possible to absorb an additional ~730-980 Gt DIC, one third of which possibly originated from intermediate waters. We also infer that LGM deep-water O2 dropped to suboxic values of <10µmol/kg in the Atlantic sector of the Southern Ocean, possibly also in the subpolar North Pacific. The outlined deglacial transfer of the extra aged, deep-ocean carbon to the atmosphere via the dynamic ocean-atmosphere carbon exchange would be sufficient to account for two trends observed, (1) for the increase in atmospheric CO2 and (2) for the 190-permil drop in atmospheric d14C during the so-called HS-1 'Mystery Interval', when atmospheric 14C production rates were largely constant.

Global Ocean Biomes: Mean and time-varying maps (NetCDF 7.8 MB)

Large-scale studies of ocean biogeochemistry and carbon cycling have often partitioned the ocean into regions along lines of latitude and longitude despite the fact that spatially more complex boundaries would be closer to the true biogeography of the ocean. Herein, we define 17 open-ocean biomes classified from four observational data sets: sea surface temperature (SST), spring/summer chlorophyll a concentrations (Chl a), ice fraction, and maximum mixed layer depth (maxMLD) on a 1° × 1° grid. By considering interannual variability for each input, we create dynamic ocean biome boundaries that shift annually between 1998 and 2010. Additionally we create a core biome map, which includes only the grid cells that do not change biome assignment across the 13 years of the time-varying biomes. These biomes can be used in future studies to distinguish large-scale ocean regions based on biogeochemical function.

Globale räumlich-zeitliche Klimavariabilität im Holozän (GHOST) [Global Holocene Spatial and Temporal Climate Variability]

Verbindung mariner Paläotemperatur-Kurven mit dreidimensionaler, gekoppelter Atmosphäre-Ozean Modellierung [Integrating marine multiproxy temperature estimates and three-dimensional coupled atmosphere/ocean modelling] Das Projekt war ein Beitrag zur Untersuchung des Klimas des Holozäns. Es basierte auf zwei Standbeinen: Der Heranziehung von weltweit verfügbaren, unbearbeiteten, aktualisierten und neu zusammengestellten marinen multiproxy Temperaturrekonstruktionen einerseits und der Verwendung von gekoppelten Zirkulationsmodellen für Atmosphäre und Ozean andererseits. Das Modell arbeitete mit relativ geringer Auflösung und Rechenzeit und ist für transiente Simulationen des Paläoklimas angepaßt. Für eine möglichst große globale Abdeckung der Zeitserien von Klimaproxies wurden Sedimentdaten herangezogen, die eine geringe aber dennoch höchstmögliche zeitliche Auflösung im Bereich von 50 bis 200 Jahren besitzen. Sowohl Datenrekonstruktion als auch gekoppelte Klimamodellierung erzeugten dreidimensionale Datensätze, zwei räumliche Dimensionen auf der Erdoberfläche, sowie die Zeit als dritte Dimension. Raumzeitliche Muster wurden im Rahmen des Projektes untersucht. Die eingehende Analyse rekonstruierter wie der Modell-Daten sollte einerseits das Verständnis für Klimaänderungen verbessern, die in Proxydaten gefunden werden und andererseits eine Validierung der Klimavariabilität im Modell ermöglichen. Die Musteranalyse ergab Einblicke in die Mechanismen, die zur Heterogenität von Erwärmung und Abkühlung im Holozän beitragen. Die Weiterführung der Klimasimulationen des Holozäns in die Zukunft der nächsten Jahrhunderte diente einer besseren Abschätzung der zukünftigen Klimaänderung.

Regional ocean model for the Mediterranean, links to model files

A regional ocean general circulation model of the Mediterranean is used to study the climate of the Last Glacial Maximum. The atmospheric forcing for these simulations has been derived from simulations with an atmospheric general circulation model, which in turn was forced with surface conditions from a coarse resolution earth system model. The model is successful in reproducing the general patterns of reconstructed sea surface temperature anomalies with the strongest cooling in summer in the northwestern Mediterranean and weak cooling in the Levantine, although the model underestimates the extent of the summer cooling in the western Mediterranean. However, there is a strong vertical gradient associated with this pattern of summer cooling, which makes the comparison with reconstructions complicated. The exchange with the Atlantic is decreased to roughly one half of its present value, which can be explained by the shallower Strait of Gibraltar as a consequence of lower global sea level. This reduced exchange causes a strong increase of salinity in the Mediterranean in spite of reduced net evaporation.