10 results on '"Maria Gonçalves Ageitos"'
Search Results
2. Mineral Dust Cycle in the Multiscale Online Nonhydrostatic AtmospheRe CHemistry Model (Monarch) Version 2.0
- Author
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Martina Klose, Oriol Jorba, Maria Gonçalves Ageitos, Jeronimo Escribano, Matthew L Dawson, Vincenzo Obiso, Enza Di Tomaso, Sara Basart, Glibert Montane Pinto, Francesca Macchia, Paul Ginoux, Juan Guerschmann, Catherine Prigent, Yue Huang, Jasper F Kok, Ronald L Miller, and Carlos Perez Garcia-Pando
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Meteorology And Climatology - Abstract
We present the dust module in the Multiscale Online Non-hydrostatic AtmospheRe CHemistry model (MONARCH) version 2.0, a chemical weather prediction system that can be used for regional and global modeling at a range of resolutions. The representations of dust processes in MONARCH were upgraded with a focus on dust emission (emission parameterizations, entrainment thresholds, considerations of soil moisture and surface cover), lower boundary conditions (roughness, potential dust sources), and dust–radiation interactions. MONARCH now allows modeling of global and regional mineral dust cycles using fundamentally different paradigms, ranging from strongly simplified to physics-based parameterizations. We present a detailed description of these updates along with four global benchmark simulations, which use conceptually different dust emission parameterizations, and we evaluate the simulations against observations of dust optical depth. We determine key dust parameters, such as global annual emission/deposition flux, dust loading, dust optical depth, mass-extinction efficiency, single-scattering albedo, and direct radiative effects. For dust-particle diameters up to 20 µm, the total annual dust emission and deposition fluxes obtained with our four experiments range between about 3500 and 6000 Tg, which largely depend upon differences in the emitted size distribution. Considering ellipsoidal particle shapes and dust refractive indices that account for size-resolved mineralogy, we estimate the global total (longwave and shortwave) dust direct radiative effect (DRE) at the surface to range between about −0.90 and −0.63 W m−2 and at the top of the atmosphere between −0.20 and −0.28 W m−2. Our evaluation demonstrates that MONARCH is able to reproduce key features of the spatiotemporal variability of the global dust cycle with important and insightful differences between the different configurations.
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- 2021
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3. Pre‐Industrial, Present and Future Atmospheric Soluble Iron Deposition and the Role of Aerosol Acidity and Oxalate Under CMIP6 Emissions
- Author
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Gilbert Montané Pinto, Carlos Pérez García-Pando, Elisa Bergas-Massó, Stelios Myriokefalitakis, Philippe Le Sager, Maria Gonçalves-Ageitos, Twan Van Noije, Ron Miller, Universitat Politècnica de Catalunya. Doctorat en Enginyeria Ambiental, and Universitat Politècnica de Catalunya. Departament d'Enginyeria de Projectes i de la Construcció
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Aigua de mar -- Contingut en ferro ,Earth and Planetary Sciences (miscellaneous) ,Desenvolupament humà i sostenible::Enginyeria ambiental [Àrees temàtiques de la UPC] ,Seawater -- Iron content ,General Environmental Science - Abstract
Atmospheric iron (Fe) deposition to the open ocean affects net primary productivity, nitrogen fixation, and carbon uptake. We investigate changes in soluble Fe (SFe) deposition from the pre-industrial period to the late 21st century using the EC-Earth3-Iron Earth System model. EC-Earth3-Iron considers various sources of Fe, including dust, fossil fuel combustion, and biomass burning, and features comprehensive atmospheric chemistry, representing atmospheric oxalate, sulfate, and Fe cycles. We show that anthropogenic activity has changed the magnitude and spatial distribution of SFe deposition by increasing combustion Fe emissions and atmospheric acidity and oxalate levels. We report that SFe deposition has doubled since the early industrial era, using the Coupled Model Intercomparison Project Phase 6 emission inventory. We highlight acidity as the main solubilization pathway for dust-Fe and oxalate-promoted processing for the solubilization of combustion-Fe. We project a global SFe deposition increase of 40% by the late 21st century relative to present day under Shared Socioeconomic Pathway (SSP) 3–7.0, which assumes weak climate change mitigation policies. Conversely, SSPs with stronger mitigation pathways (1–2.6 and 2–4.5) result in 35% and 10% global decreases, respectively. Despite these differences, SFe deposition increases over the equatorial Pacific and decreases in the Southern Ocean (SO) for all SSPs. We further observe that deposition over the equatorial Pacific and SO are highly sensitive to future changes in dust emissions from Australia and South America, as well as from North Africa. Future studies should focus on the potential impact of climate- and human-induced changes in dust and wildfires combined. This work was funded by the European Research Council under the Horizon 2020 research and innovation programme through the ERC Consolidator Grant FRAGMENT (grant agreement no. 773051), the AXA Research Fund through the AXA Chair on Sand and Dust Storms at BSC, the Spanish Ministerio de Economía y Competitividad through the NUTRIENT project (CGL2017-88911-R), the European Union's Horizon 2020 research and innovation programme under grant agreement no 821205 (FORCeS), and ESA through the DOMOS project (ESA AO/1-10546/20/I-NB). We acknowledge the EMIT project, which is supported by the National Aeronautics and Space Administration Earth Venture Instrument program, under the Earth Science Division of the Science Mission Directorate. RLM received additional support from the NASA Modeling, Analysis and Prediction Program (NNG14HH42I). We also acknowledge the resources obtained on the Marenostrum4 supercomputer at BSC, granted through the PRACE project eFRAGMENT2 and RES project AECT-2020-3-0020, along with the technical support provided by BSC and the Computational Earth Sciences team of the BSC Earth Sciences Department.
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- 2023
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4. How important are secondary ice processes – preliminary results from FOR-ICE
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Luisa Ickes, Montserrat Costa Surós, Patrick Eriksson, Hannah Frostenberg, Paraskevi Georgakaki, Maria Gonçalves Ageitos, Hanna Hallborn, Anna Lewinschal, Eleanor May, Athanasios Nenes, David Neubauer, Carlos Pérez García-Pando, Ulrike Proske, and Georgia Sotiropoulou
- Abstract
Global climate models poorly represent mixed-phase clouds, which leads to uncertainties in cloud radiative forcing and precipitation. In the FORCeS ice experiment (FOR-ICE) we compare three global climate models (ECHAM-HAM, NorESM, EC-Earth) and show which processes are crucial for a realistic representation of cloud ice and supercooled water in each global climate model framework using the factorial method as a statistical approach. A specific focus of the experiments is on secondary ice production (SIP) - which apart from one mechanism (rime splintering) is typically not represented in models, even if observations of ice crystal concentrations of ice crystal number in warm mixed-phase clouds often exceed available ice nuclei by orders of magnitude. We evaluate the importance of three SIP mechanisms combined (rime splintering, ice-ice collisions, and droplet shattering) compared to all other processes that can modulate ice mass and number in mixed-phase clouds: ice nucleation, sedimentation, and transport of ice crystals, and the Wegener-Bergeron-Findeisen process. To describe SIP we adopt two approaches: an explicit microphysical representation of the processes, and a parameterization based on a random forest regression of high-resolution two-year simulations in the Arctic using the polar Weather Research and Forecast model (polar-WRF). Satellite observations are used to evaluate if including descriptions of SIP leads to a more realistic representation of mixed phase clouds.
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- 2023
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5. Performance and Early Results from the Earth Surface Mineral Dust Source Investigation (EMIT) Imaging Spectroscopy Mission
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Robert O. Green, Natalie Mahowald, David R. Thompson, Charlene Ung, Phil Brodrick, Randy Pollock, Matthew Bennett, Sarah Lundeen, Michael Joyce, Winston Olson-Duvall, Bogdan Oaida, Christine Bradley, Ernesto Diaz, Roger Clark, Suresh Vannan, Gregg Swayze, Ray Kokaly, Paul Ginoux, Ron Miller, Gregory Okin, Carlos Perez Garcia-Pando, Bethany Ehlmann, Olga Kalashnikova, Thomas H. Painter, Vincent Realmuto, Dana Chadwick, Eyal Ben-Dor, Daniela Heller Pearlshtien, Luis Guanter, Benjamin Phillips, Kevin Reath, Andrew Thorpe, Lucas Shaw, Abigail Keebler, Francisco Ochoa, Kathleen Grant, Amit Sen, Riley Duren, Vincenzo Obiso, Maria Gonçalves-Ageitos, and Yue Huang
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- 2023
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6. Impacts of recent atmospheric dust deposition on ocean biogeochemical cycles
- Author
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Joan Llort, Carlos Pérez García-Pando, Elisa Bergas-Massó, Stelios Myriokefalitakis, Raffaele Bernardello, and Maria Gonçalves-Ageitos
- Abstract
The ocean plays a key role in climate change mitigation by absorbing heat and CO2 accumulating in the atmosphere due to anthropogenic greenhouse gases emissions. While it is commonly accepted that anthropogenic CO2 is absorbed by the ocean primarily through physical and chemical mechanisms, biological cycling of carbon is mainly responsible for maintaining the vertical gradient of dissolved inorganic carbon in the ocean. Thanks to a series of processes known as the biological carbon pump, oceanic phytoplankton uptakes carbon and promotes sinking of particulate organic matter to the deeper ocean. Uncertainty about the strength of these processes and about their response to ongoing and projected climate change is large enough to confound predictions of future ocean carbon uptake. One of the most important limiting factors for phytoplankton growth over large oceanic areas is the availability of iron. While there is no doubt regarding the importance of dust transport and deposition over open oceans as the most important iron source, questions remain still open regarding closing the relationship between dust sources, long-range transport, iron solubilisation during transport and deposition processes. Overall, better understanding the mechanisms behind the spatial and temporal variability of atmospheric dust-ocean interactions is key to interpret the response of ocean biogeochemistry and to increase confidence in future climate projections. In this work, we present a reconstruction of global ocean biogeochemistry for the last 30 years, where we evaluate the impact on ocean biogeochemical cycles of newly produced iron deposition fields. These were derived with EC-Earth3-Iron, a version of the Earth System Model EC-Earth3 with a state-of-the-art description of the atmospheric iron cycle. EC-Earth3-Iron estimates iron emissions considering explicitly the mineralogy of dust sources, and accounts for the contribution of anthropogenic combustion and biomass burning sources. The model includes an advanced representation of the iron solubilization in the atmosphere, which occurs through acidic attack, organic-ligand mediated dissolution and photo-reductive processes. Furthermore, it allows distinguishing the contribution to the soluble (and total) iron deposition in the ocean of the natural and anthropogenic dust sources, fossil fuels combustion and biomass burning, and characterizing thus separately their impact on ocean biogeochemistry. We compare the ocean biogeochemistry reconstruction against a control where commonly used climatologies for iron deposition fields are prescribed.
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- 2023
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7. Supplementary material to 'Role of K-feldspar and quartz in global ice nucleation by mineral dust in mixed-phase clouds'
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Marios Chatziparaschos, Nikos Daskalakis, Stelios Myriokefalitakis, Nikos Kalivitis, Athanasios Nenes, Maria Gonçalves Ageitos, Montserrat Costa-Surós, Carlos Pérez García-Pando, Medea Zanoli, Mihalis Vrekoussis, and Maria Kanakidou
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- 2022
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8. Improved constraints on hematite refractive index for estimating climatic effects of dust aerosols
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Longlei Li, Natalie M. Mahowald, María Gonçalves Ageitos, Vincenzo Obiso, Ron L. Miller, Carlos Pérez García-Pando, Claudia Di Biagio, Paola Formenti, Philip G. Brodrick, Roger N. Clark, Robert O. Green, Raymond Kokaly, Gregg Swayze, and David R. Thompson
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Geology ,QE1-996.5 ,Environmental sciences ,GE1-350 - Abstract
Abstract Uncertainty in desert dust composition poses a big challenge to understanding Earth’s climate across different epochs. Of particular concern is hematite, an iron-oxide mineral dominating the solar absorption by dust particles, for which current estimates of absorption capacity vary by over two orders of magnitude. Here, we show that laboratory measurements of dust composition, absorption, and scattering provide valuable constraints on the absorption potential of hematite, substantially narrowing its range of plausible values. The success of this constraint is supported by results from an atmospheric transport model compared with station-based measurements. Additionally, we identify substantial bias in simulating hematite abundance in dust aerosols with current soil mineralogy descriptions, underscoring the necessity for improved data sources. Encouragingly, the next-generation imaging spectroscopy remote sensing data hold promise for capturing the spatial variability of hematite. These insights have implications for enhancing dust modeling, thus contributing to efforts in climate change mitigation and adaptation.
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- 2024
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9. Supplementary material to 'Quantifying the range of the dust direct radiative effect due to source mineralogy uncertainty'
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Longlei Li, Natalie M. Mahowald, Ron L. Miller, Carlos Pérez García-Pando, Martina Klose, Douglas S. Hamilton, Maria Gonçalves Ageitos, Paul Ginoux, Yves Balkanski, Robert O. Green, Olga Kalashnikova, Jasper F. Kok, Vincenzo Obiso, David Paynter, and David R. Thompson
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- 2020
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10. Pre‐Industrial, Present and Future Atmospheric Soluble Iron Deposition and the Role of Aerosol Acidity and Oxalate Under CMIP6 Emissions
- Author
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Elisa Bergas‐Massó, María Gonçalves Ageitos, Stelios Myriokefalitakis, Ron L. Miller, Twan vanNoije, Philippe Le Sager, Gilbert Montané Pinto, and Carlos Pérez García‐Pando
- Subjects
Environmental sciences ,GE1-350 ,Ecology ,QH540-549.5 - Abstract
Abstract Atmospheric iron (Fe) deposition to the open ocean affects net primary productivity, nitrogen fixation, and carbon uptake. We investigate changes in soluble Fe (SFe) deposition from the pre‐industrial period to the late 21st century using the EC‐Earth3‐Iron Earth System model. EC‐Earth3‐Iron considers various sources of Fe, including dust, fossil fuel combustion, and biomass burning, and features comprehensive atmospheric chemistry, representing atmospheric oxalate, sulfate, and Fe cycles. We show that anthropogenic activity has changed the magnitude and spatial distribution of SFe deposition by increasing combustion Fe emissions and atmospheric acidity and oxalate levels. We report that SFe deposition has doubled since the early industrial era, using the Coupled Model Intercomparison Project Phase 6 emission inventory. We highlight acidity as the main solubilization pathway for dust‐Fe and oxalate‐promoted processing for the solubilization of combustion‐Fe. We project a global SFe deposition increase of 40% by the late 21st century relative to present day under Shared Socioeconomic Pathway (SSP) 3–7.0, which assumes weak climate change mitigation policies. Conversely, SSPs with stronger mitigation pathways (1–2.6 and 2–4.5) result in 35% and 10% global decreases, respectively. Despite these differences, SFe deposition increases over the equatorial Pacific and decreases in the Southern Ocean (SO) for all SSPs. We further observe that deposition over the equatorial Pacific and SO are highly sensitive to future changes in dust emissions from Australia and South America, as well as from North Africa. Future studies should focus on the potential impact of climate‐ and human‐induced changes in dust and wildfires combined.
- Published
- 2023
- Full Text
- View/download PDF
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