Longlei Li, N. M. Mahowald, Vincenzo Obiso, Jasper F. Kok, R. L. Miller, Xiaohong Liu, Marı́a Gonçalves Ageitos, Carlos Pérez García‐Pando, Danny M. Leung, Ziming Ke, Philip G. Brodrick, R. N. Clark, Paola Formenti, Claudia Di Biagio, Paul Ginoux, Gregory S. Okin, Zhou Bo, David R. Thompson, Robert O. Green
Abstract The direct radiative effect (DRE) of dust aerosols in Earth system models (ESMs) remains highly uncertain, largely due to inadequate representations of particle size distribution (PSD) and mineral composition. Using NASA's Earth Surface Mineral Dust Source Investigation (EMIT) soil mineralogy data and observed PSD in an ESM that resolves dust mineral composition and emitted diameters from 0.1 to 70 μm, we find a near‐neutral global dust net DRE (−0.057 W m −2 ), weaker than most previous estimates. Large dust (diameter >10 μm) contributes 30% of the global longwave dust optical depth, providing observational constraints on large‐particle abundance, and offsets 20% of the dust shortwave cooling over major source regions. Incorporation of EMIT mineralogy reduces shortwave uncertainty by more than 50%. The remaining uncertainty mainly exists in processes controlling dust abundance, particularly the poorly understood transport of large dust, and longwave optical properties, which require additional observational constraints to more accurately quantify the dust DRE.