Improved representation of the global dust cycle using observational constraints on dust properties and abundance
dc.contributor.author | Kok, Jasper F. | |
dc.contributor.author | Adebiyi, Adeyemi A. | |
dc.contributor.author | Albani, Samuel | |
dc.contributor.author | Balkanski, Yves | |
dc.contributor.author | Checa-Garcia, Ramiro | |
dc.contributor.author | Chin, Mian | |
dc.contributor.author | Colarco, Peter R. | |
dc.contributor.author | Hamilton, Douglas Stephen | |
dc.contributor.author | Huang, Yue | |
dc.contributor.author | Ito, Akinori | |
dc.contributor.author | Klose, Martina | |
dc.contributor.author | Leung, Danny M. | |
dc.contributor.author | Li, Longlei | |
dc.contributor.author | Mahowald, Natalie M. | |
dc.contributor.author | Miller, Ron L. | |
dc.contributor.author | Obiso, Vincenzo | |
dc.contributor.author | García-Pando, Carlos Pérez | |
dc.contributor.author | Rocha-Lima, Adriana | |
dc.contributor.author | Wan, Jessica S. | |
dc.contributor.author | Whicker, Chloe A. | |
dc.date.accessioned | 2020-12-11T17:34:21Z | |
dc.date.available | 2020-12-11T17:34:21Z | |
dc.date.issued | 2020-11-23 | |
dc.description.abstract | Even though desert dust is the most abundant aerosol by mass in Earth's atmosphere, atmospheric models struggle to accurately represent its spatial and temporal distribution. These model errors are partially caused by fundamental difficulties in simulating dust emission in coarse-resolution models and in accurately representing dust microphysical properties. Here we mitigate these problems by developing a new methodology that yields an improved representation of the global dust cycle. We present an analytical framework that uses inverse modeling to integrate an ensemble of global model simulations with observational constraints on the dust size distribution, extinction efficiency, and regional dust aerosol optical depth. We then compare the inverse model results against independent measurements of dust surface concentration and deposition flux and find that errors are reduced by approximately a factor of two relative to current model simulations of the Northern Hemisphere dust cycle. The inverse model results show smaller improvements in the less dusty Southern Hemisphere, most likely because both the model simulations and the observational constraints used in the inverse model are less accurate. On a global basis, we find that the emission flux of dust with geometric diameter up to 20 μm (PM20) is approximately 5,000 Tg/year, which is greater than most models account for. This larger PM20 dust flux is needed to match observational constraints showing a large atmospheric loading of coarse dust. We obtain gridded data sets of dust emission, vertically integrated loading, dust aerosol optical depth, (surface) concentration, and wet and dry deposition fluxes that are resolved by season and particle size. As our results indicate that this data set is more accurate than current model simulations and the MERRA-2 dust reanalysis product, it can be used to improve quantifications of dust impacts on the Earth system. | en_US |
dc.description.sponsorship | This work was developed with support from the National Science Foundation (NSF) grants 1552519 and 1856389 and the Army Research Office under Cooperative Agreement Number W911NF-20-2-0150 awarded to J.F.K, from the University of California President’s Postdoctoral Fellowship awarded to A.A.A., from the European Union’s Horizon 2020 research and innovation programme under the Marie Skłodowska-Curie grant agreement No 708119 awarded to S.A. and No. 789630 awarded to M.K. R. C.-G. received funding from the European Union’s Horizon 2020 research and innovation grant 641816 (CRESCENDO), and from JSPS KAKENHI Grant Number 20H04329 and Integrated Research Program for Advancing Climate Models (TOUGOU) Grant Number JPMXD0717935715 from the Ministry of Education, Culture, Sports, Science and Technology (MEXT), Japan to A.I. P.R.C. and A.R.- L. acknowledge support from the NASA Atmospheric Composition: Modeling and Analysis Program (R. Eckman, program manager) and the NASA Center for Climate Simulation (NCCS) for computational resources, Y.H. acknowledges NASA grant 80NSSC19K1346, awarded under the Future Investigators in NASA Earth and Space Science and Technology (FINESST) program, and R.L.M. acknowledges support from the NASA Modeling, Analysis and Prediction Program (NNG14HH42I). C.P.G.P. acknowledges support by the European Research Council (grant no. 773051, FRAGMENT), the EU H2020 project FORCES (grant no. 821205), the AXA Research Fund, and the Spanish Ministry of Science, Innovation and Universities (RYC-2015-18690 and CGL2017-88911-R). M.K. and C.P.G.P. acknowledge PRACE for awarding access to MareNostrum at Barcelona Supercomputing Center to run MONARCH. L.L. acknowledges support from the NASA EMIT project and the Earth Venture – Instrument program (grant no. E678605). We also acknowledge high-performance computing support from Cheyenne (doi:10.5065/D6RX99HX) provided by NCAR's Computational and Information Systems Laboratory, sponsored by the National Science Foundation. We further thank Anna Benedictow for assistance in accessing the AeroCom modeling data, the AeroCom modeling groups for making their simulations available, Joseph Prospero and Nicolas Huneeus for providing dust surface concentration data from in situ measurements from the University of Miami Ocean Aerosol Network, and the investigators of the Sahelian Dust Transect for making their dust concentration measurements available. The MERRA-2 data used in this study/project have been provided by the Global Modeling and Assimilation Office (GMAO) at NASA Goddard Space Flight Center | en_US |
dc.description.uri | https://acp.copernicus.org/preprints/acp-2020-1131/ | en_US |
dc.format.extent | 45 pages | en_US |
dc.genre | journal articles preprints | en_US |
dc.identifier | doi:10.13016/m28ql4-trl3 | |
dc.identifier.citation | Kok, J. F., Adebiyi, A. A., Albani, S., Balkanski, Y., Checa-Garcia, R., Chin, M., Colarco, P. R., Hamilton, D. S., Huang, Y., Ito, A., Klose, M., Leung, D. M., Li, L., Mahowald, N. M., Miller, R. L., Obiso, V., Pérez García-Pando, C., Rocha-Lima, A., Wan, J. S., and Whicker, C. A.: Improved representation of the global dust cycle using observational constraints on dust properties and abundance, Atmos. Chem. Phys. Discuss., https://doi.org/10.5194/acp-2020-1131, in review, 2020. | en_US |
dc.identifier.uri | https://doi.org/10.5194/acp-2020-1131 | |
dc.identifier.uri | http://hdl.handle.net/11603/20237 | |
dc.language.iso | en_US | en_US |
dc.publisher | Copernicus Publications | en_US |
dc.relation.isAvailableAt | The University of Maryland, Baltimore County (UMBC) | |
dc.relation.ispartof | UMBC Physics Department Collection | |
dc.relation.ispartof | UMBC Faculty Collection | |
dc.relation.ispartof | UMBC Joint Center for Earth Systems Technology (JCET) | |
dc.rights | This item is likely protected under Title 17 of the U.S. Copyright Law. Unless on a Creative Commons license, for uses protected by Copyright Law, contact the copyright holder or the author. | |
dc.rights | Public Domain Mark 1.0 | * |
dc.rights | This work was written as part of one of the author's official duties as an Employee of the United States Government and is therefore a work of the United States Government. In accordance with 17 U.S.C. 105, no copyright protection is available for such works under U.S. Law. | |
dc.rights.uri | http://creativecommons.org/publicdomain/mark/1.0/ | * |
dc.title | Improved representation of the global dust cycle using observational constraints on dust properties and abundance | en_US |
dc.type | Text | en_US |