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Decoding Dust Storms: Namibia’s Etosha Pan Reveals Global Climate Connections

geog.ox.ac.uk · last updated

The Etosha Pan, a vast salt pan—essentially a dry lakebed where water evaporates to leave behind layers of salt and fine sediments—is one of the Southern Hemisphere’s most active dust sources. 

Atmospheric dust plays a critical role in Earth system processes – from influencing cloud properties and radiation balance to fertilising remote ocean ecosystems. Improving how dynamic dust sources like Etosha are modelled is vital for accurate projections of future climate. Understanding these dynamics is critical not only for local air quality and land surface processes but also is essential for representing dryland dust emissions in climate models. 

In a newly published study in Science of the Total Environment, in collaboration with Professor Giles Wiggs (University of Oxford) and Dr Robert Bryant (University of Sheffield), we examined how seasonal rainfall, pan flooding, and large-scale ocean-atmosphere dynamics interact to drive dust emissions from this vast ephemeral lakebed by drawing on more than 20 years of satellite observations. 

Our analysis showed that dust emissions from Etosha Pan are highly sensitive to rainfall. During wet periods, the pan surface becomes saturated, reducing dust activity by limiting the potential for wind erosion. However, once the surface dries, dust emissions can return quickly – sometimes within just a few months. In contrast, extended dry periods leave the pan’s salt-rich and highly erodible sediments exposed, resulting in frequent and intense dust storms.

These local dust dynamics are strongly influenced by global climate modes. The study found that years associated with El Niño events (a warming of the Pacific Ocean) and negative phases of the Subtropical Indian Ocean Dipole typically bring drier conditions to the region and lead to increased dust activity. Conversely, La Niña events and positive phases of the Subtropical Indian Ocean Dipole are associated with higher rainfall and widespread flooding, which act to stabilise the pan surface and suppress emissions.

Another key focus of the study was the timing of dust recovery following flooding. Previous assumptions suggested a delay of one to two years before dust storms resumed after major flooding. However, we found that emissions can return in as little as three months after the surface dries, revealing a much faster response than expected and underscoring the sensitivity of the system to short-term climate fluctuations.

This shows the potential for predicting dust activity using seasonal climate indicators. As climate variability increases and dust-prone regions expand, the ability to anticipate dust trends would greatly benefit environmental monitoring, public health preparedness, and policy planning in affected areas.