EGU25-14580, updated on 15 Mar 2025
https://doi.org/10.5194/egusphere-egu25-14580
EGU General Assembly 2025
© Author(s) 2025. This work is distributed under
the Creative Commons Attribution 4.0 License.
Remote impacts of the mid-Holocene Green Sahara
Shivangi Tiwari1, Francesco S. R. Pausata1, Allegra N. LeGrande2,3, Michael Griffiths4, Ilana Wainer5, Hugo Beltrami6,1, Anne de Vernal1, Peter O. Hopcroft7, Clay Tabor8, Deepak Chandan9, and W. Richard Peltier9
Shivangi Tiwari et al.
  • 1Université du Québec à Montréal, Département des sciences de la Terre et de l'atmosphère, Montreal, Canada (tiwari.shivangi@courrier.uqam.ca)
  • 2NASA Goddard Institute for Space Studies, New York, New York, USA
  • 3Center for Climate Systems Research, Columbia University, New York, New York, USA
  • 4Department of Environmental Science, William Paterson University, Wayne, New Jersey, USA
  • 5Departamento de Oceanografia Física, Química e Geológica, Instituto Oceanográfico da Universidade de São Paulo, Praça do Oceanográfico, Sao Paulo, Brazil
  • 6Department of Earth Sciences, St. Francis Xavier University, Antigonish, Nova Scotia, Canada
  • 7School of Geography, Earth and Environmental Sciences, University of Birmingham, Birmingham, UK
  • 8Department of Earth Sciences, University of Connecticut, Storrs, Connecticut, USA
  • 9Department of Physics, University of Toronto, Toronto, Ontario, Canada

The mid-Holocene (MH: 6,000 years before present) is a key time slice for paleoclimate studies, and is one of the two entry cards for participation in the current Paleoclimate Modelling Intercomparison Project (PMIP4). The MH was characterized by high boreal summer insolation, leading to an intensification of the Northern Hemisphere monsoons. In northern Africa, the strengthening of the West African Monsoon was further amplified by nonlinear feedbacks, resulting in the development of vegetation referred to as the “Green Sahara”. The vegetation and land surface changes over northern Africa had various remote effects impacting the global climate through teleconnections.

In this study, we analyse outputs from five fully coupled global climate models to identify the  remote impacts of the Green Sahara on global climate. Through the difference of two sets of mid-Holocene simulations – with and without the Green Sahara – we isolate the effect of the northern African vegetation and land cover changes on South American hydroclimate and tropical modes of climate variability such as the El Niño Southern Oscillation and the Atlantic Niño. Using an atmosphere-only climate model, we further investigate the Saharan-Arctic teleconnection invoked to explain the Arctic cooling concurrent with Saharan desertification. We quantify proxy-model agreement through metrics such as the Cohen’s Kappa index and the Root Mean Square Error to assess if the inclusion of the Green Saharan changes leads to greater coherence of model simulations with proxy reconstructions. Our results demonstrate the critical role of the Green Sahara in modulating the MH climate.

How to cite: Tiwari, S., S. R. Pausata, F., N. LeGrande, A., Griffiths, M., Wainer, I., Beltrami, H., de Vernal, A., O. Hopcroft, P., Tabor, C., Chandan, D., and Peltier, W. R.: Remote impacts of the mid-Holocene Green Sahara, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-14580, https://doi.org/10.5194/egusphere-egu25-14580, 2025.