Article

Stormier mid-Holocene southwest Indian Ocean due to poleward trending tropical cyclones

Details

Citation

Green A, Cooper J, Loureiro C, Dixon S, Hahn A & Zabel M (2022) Stormier mid-Holocene southwest Indian Ocean due to poleward trending tropical cyclones. Nature Geoscience, 15, Art. No.: 60-66. https://doi.org/10.1038/s41561-021-00842-w

Abstract
Geological evidence of past storminess is fundamental for contextualizing long-term climate variability and investigating future climate. Unlike the Atlantic and Pacific basins, robust storminess reconstructions do not exist for most of the Indian Ocean, despite the hazard that tropical cyclones pose to the SE African margin. Here we combine seismic stratigraphy with analysis of marine sediment cores to look for regionally representative storm-related sediment deposits (tempestites) intercalated in shoreface sediments from the SW Indian Ocean off South Africa. Tempestites, represented by hummocky seismic units, whose sediments have clear marine geochemical signatures, are found to have been deposited between 7.0 and 4.8 cal kyr BP, when sea level was between 0 and +3 m above present. Deposition and preservation of the tempestites reflect unprecedented tropical cyclone impacts, associated with periods of strongly positive Indian Ocean Dipole anomalies and linked to warmer sea surface temperatures. Future climate projections suggest stronger positive IOD anomalies and further intensification and poleward migration of tropical cyclones, like their mid-Holocene predecessors. Given the rarity of tropical cyclone landfalls in South Africa, this urges a revaluation of hazards in areas along the SE African coast likely to become more vulnerable to landfalling tropical cyclones in the future.

Keywords
Atmospheric science; Palaeoclimate; Sedimentology

Journal
Nature Geoscience: Volume 15

StatusPublished
FundersGerman Research Foundation
Publication date31/01/2022
Publication date online23/12/2021
Date accepted by journal17/09/2021
URLhttp://hdl.handle.net/1893/33733
ISSN1752-0894
eISSN1752-0908