Hamish O. Couper , Christopher C. Day , Julia J. Barrott , Samuel J. Hollowood , Stacy A. Carolin , Ben Lovett , Abdeljalil Bouzouggar , Nick Barton , Gideon M. Henderson
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引用次数: 0
Abstract
The West African Monsoon (WAM), Atlantic north-westerlies and Mediterranean cyclones are significant sources of rainfall in north-west Africa, supplying moisture to the fringes of the Sahara. Rainfall patterns and the extent of the desert vary through time with strong evidence of a wetter Sahara during the early- to mid-Holocene (widely referred to as the African Humid Period). North of 28°N there is a particular lack of palaeorainfall reconstructions, with higher spatial- and temporal-resolution required to constrain the mechanisms responsible for past sub-tropical climate change, and the impacts of environmental change on human developments. We provide palaeorainfall reconstructions from stalagmites from today's arid north-west Sahara, inland from the coast and south of the Atlas Mountains in Morocco (30–32°N). The records show increased rainfall between 8.7–4.3 kyr BP. The timing, and oxygen isotopes of the speleothem growth, in comparison with other records, strongly suggest that South-of-Atlas rainfall continued after the decline of the West African Monsoon in the mid-Holocene. We propose that additional rainfall was supplied by increased tropical-plume rainfall in the South-of-Atlas region. We suggest that an increased North-South inter-hemispheric temperature anomaly, shifting the ITCZ northwards, increased the supply of tropical-moisture to tropical-plumes. For the first time this study provides evidence supporting tropical-plumes as an additional source of past-rainfall, helping to reconcile palaeo-archives and modelling studies. Increased South-of-Atlas rainfall improved habitability and increased recharge to rivers flowing south into the Sahara, which likely facilitated connectivity through the Sahara, during a key period in the development of land use and animal production.
期刊介绍:
Earth and Planetary Science Letters (EPSL) is a leading journal for researchers across the entire Earth and planetary sciences community. It publishes concise, exciting, high-impact articles ("Letters") of broad interest. Its focus is on physical and chemical processes, the evolution and general properties of the Earth and planets - from their deep interiors to their atmospheres. EPSL also includes a Frontiers section, featuring invited high-profile synthesis articles by leading experts on timely topics to bring cutting-edge research to the wider community.