400 results on '"Stenke, Andrea"'
Search Results
2. A fully coupled solid-particle microphysics scheme for stratospheric aerosol injections within the aerosol–chemistry–climate model SOCOL-AERv2.
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Vattioni, Sandro, Weber, Rahel, Feinberg, Aryeh, Stenke, Andrea, Dykema, John A., Luo, Beiping, Kelesidis, Georgios A., Bruun, Christian A., Sukhodolov, Timofei, Keutsch, Frank N., Peter, Thomas, and Chiodo, Gabriel
- Subjects
STRATOSPHERIC aerosols ,OZONE layer depletion ,SURFACE chemistry ,SULFURIC acid ,MICROPHYSICS ,SULFUR cycle - Abstract
Recent studies have suggested that injection of solid particles such as alumina and calcite particles for stratospheric aerosol injection (SAI) instead of sulfur-based injections could reduce some of the adverse side effects of SAI such as ozone depletion and stratospheric heating. Here, we present a version of the global aerosol–chemistry–climate model SOCOL-AERv2 and the Earth system model (ESM) SOCOLv4 which incorporate a solid-particle microphysics scheme for assessment of SAI of solid particles. Microphysical interactions of the solid particle with the stratospheric sulfur cycle were interactively coupled to the heterogeneous chemistry scheme and the radiative transfer code (RTC) for the first time within an ESM. Therefore, the model allows simulation of heterogeneous chemistry at the particle surface as well as feedbacks between microphysics, chemistry, radiation and climate. We show that sulfur-based SAI results in a doubling of the stratospheric aerosol burden compared to the same mass injection rate of calcite and alumina particles with a radius of 240 nm. Most of the sulfuric acid aerosol mass resulting from SO2 injection does not need to be lifted to the stratosphere but is formed after in situ oxidation and subsequent water uptake in the stratosphere. Therefore, to achieve the same radiative forcing, larger injection rates are needed for calcite and alumina particle injection than for sulfur-based SAI. The stratospheric sulfur cycle would be significantly perturbed, with a reduction in stratospheric sulfuric acid burden by 53 %, when injecting 5 Mtyr-1 (megatons per year) of alumina or calcite particles of 240 nm radius. We show that alumina particles will acquire a sulfuric acid coating equivalent to about 10 nm thickness if the sulfuric acid is equally distributed over the whole available particle surface area in the lower stratosphere. However, due to the steep contact angle of sulfuric acid on alumina particles, the sulfuric acid coating would likely not cover the entire alumina surface, which would result in available surface for heterogeneous reactions other than the ones on sulfuric acid. When applying realistic uptake coefficients of 1.0, 10-5 and 10-4 for H2SO4 , HCl and HNO3 , respectively, the same scenario with injections of calcite particles results in 94 % of the particle mass remaining in the form of CaCO3. This likely keeps the optical properties of the calcite particles intact but could significantly alter the heterogeneous reactions occurring on the particle surfaces. The major process uncertainties of solid-particle SAI are (1) the solid-particle microphysics in the injection plume and degree of agglomeration of solid particles on the sub-ESM grid scale, (2) the scattering properties of the resulting agglomerates, (3) heterogeneous chemistry on the particle surface, and (4) aerosol–cloud interactions. These uncertainties can only be addressed with extensive, coordinated experimental and modelling research efforts. The model presented in this work offers a useful tool for sensitivity studies and incorporating new experimental results on SAI of solid particles. [ABSTRACT FROM AUTHOR]
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- 2024
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3. Supplementary material to "A fully coupled solid particle microphysics scheme for stratospheric aerosol injections within the aerosol-chemistry-climate-model SOCOL-AERv2"
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Vattioni, Sandro, primary, Weber, Rahel, additional, Feinberg, Aryehe, additional, Stenke, Andrea, additional, Dykema, John A., additional, Luo, Beiping, additional, Kelesidis, Georgios A., additional, Bruun, Christian A., additional, Sukhodolov, Timofei, additional, Keutsch, Frank N., additional, Peter, Thomas, additional, and Chiodo, Gabriel, additional
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- 2024
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4. A fully coupled solid particle microphysics scheme for stratospheric aerosol injections within the aerosol-chemistry-climate-model SOCOL-AERv2
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Vattioni, Sandro, primary, Weber, Rahel, additional, Feinberg, Aryehe, additional, Stenke, Andrea, additional, Dykema, John A., additional, Luo, Beiping, additional, Kelesidis, Georgios A., additional, Bruun, Christian A., additional, Sukhodolov, Timofei, additional, Keutsch, Frank N., additional, Peter, Thomas, additional, and Chiodo, Gabriel, additional
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- 2024
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5. Deriving Global OH Abundance and Atmospheric Lifetimes for Long-Lived Gases: A Search for CH3CCl3 Alternatives.
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Liang, Qing, Chipperfield, Martyn, Fleming, Eric, Abraham, N, Braesicke, Peter, Burkholder, James, Daniel, John, Dhomse, Sandip, Fraser, Paul, Hardiman, Steven, Jackman, Charles, Kinnison, Douglas, Krummel, Paul, Montzka, Stephen, Morgenstern, Olaf, McCulloch, Archie, Mühle, Jens, Newman, Paul, Orkin, Vladimir, Pitari, Giovanni, Prinn, Ronald, Rigby, Matthew, Rozanov, Eugene, Stenke, Andrea, Tummon, Fiona, Velders, Guus, Visioni, Daniele, and Weiss, Ray
- Abstract
An accurate estimate of global hydroxyl radical (OH) abundance is important for projections of air quality, climate, and stratospheric ozone recovery. As the atmospheric mixing ratios of methyl chloroform (CH3CCl3) (MCF), the commonly used OH reference gas, approaches zero, it is important to find alternative approaches to infer atmospheric OH abundance and variability. The lack of global bottom-up emission inventories is the primary obstacle in choosing a MCF alternative. We illustrate that global emissions of long-lived trace gases can be inferred from their observed mixing ratio differences between the Northern Hemisphere (NH) and Southern Hemisphere (SH), given realistic estimates of their NH-SH exchange time, the emission partitioning between the two hemispheres, and the NH versus SH OH abundance ratio. Using the observed long-term trend and emissions derived from the measured hemispheric gradient, the combination of HFC-32 (CH2F2), HFC-134a (CH2FCF3, HFC-152a (CH3CHF2), and HCFC-22 (CHClF2), instead of a single gas, will be useful as a MCF alternative to infer global and hemispheric OH abundance and trace gas lifetimes. The primary assumption on which this multispecies approach relies is that the OH lifetimes can be estimated by scaling the thermal reaction rates of a reference gas at 272 K on global and hemispheric scales. Thus, the derived hemispheric and global OH estimates are forced to reconcile the observed trends and gradient for all four compounds simultaneously. However, currently, observations of these gases from the surface networks do not provide more accurate OH abundance estimate than that from MCF.
- Published
- 2017
6. No robust evidence of future changes in major stratospheric sudden warmings: a multi-model assessment from CCMI
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Ayarzagüena Porras, Blanca, Polvani, Lorenzo M., Langematz, Ulrike, Akiyoshi, Hideharu, Bekki, Slimane, Butchart, Neal, Dameris, Martin, Deushi, Makoto, Hardiman, Steven C., Jöckel, Patrick, Klekociuk, Andrew, Marchand, Marion, Michou, Martine, Morgenstern, Olaf, O'Connor, Fiona M., Oman, Luke D., Plummer, David A., Revell, Laura, Rozanov, Eugene, Saint-Martin, David, Scinocca, John, Stenke, Andrea, Stone, Kane, Yamashita, Yousuke, Yoshida, Kohei, Zeng, Guang, Ayarzagüena Porras, Blanca, Polvani, Lorenzo M., Langematz, Ulrike, Akiyoshi, Hideharu, Bekki, Slimane, Butchart, Neal, Dameris, Martin, Deushi, Makoto, Hardiman, Steven C., Jöckel, Patrick, Klekociuk, Andrew, Marchand, Marion, Michou, Martine, Morgenstern, Olaf, O'Connor, Fiona M., Oman, Luke D., Plummer, David A., Revell, Laura, Rozanov, Eugene, Saint-Martin, David, Scinocca, John, Stenke, Andrea, Stone, Kane, Yamashita, Yousuke, Yoshida, Kohei, and Zeng, Guang
- Abstract
Major mid-winter stratospheric sudden warmings (SSWs) are the largest instance of wintertime variability in the Arctic stratosphere. Because SSWs are able to cause significant surface weather anomalies on intra-seasonal timescales, several previous studies have focused on their potential future change, as might be induced by anthropogenic forcings. However, a wide range of results have been reported, from a future increase in the frequency of SSWs to an actual decrease. Several factors might explain these contradictory results, notably the use of different metrics for the identification of SSWs and the impact of large climatological biases in single-model studies. To bring some clarity, we here revisit the question of future SSW changes, using an identical set of metrics applied consistently across 12 different models participating in the Chemistry–Climate Model Initiative. Our analysis reveals that no statistically significant change in the frequency of SSWs will occur over the 21st century, irrespective of the metric used for the identification of the event. Changes in other SSW characteristics – such as their duration, deceleration of the polar night jet, and the tropospheric forcing – are also assessed: again, we find no evidence of future changes over the 21st century., European Research council, Deutsche Forschungsgemeinschaft, Depto. de Física de la Tierra y Astrofísica, Fac. de Ciencias Físicas, TRUE, pub
- Published
- 2024
7. Emerging investigator series: predicted losses of sulfur and selenium in european soils using machine learning: a call for prudent model interrogation and selection.
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Jones, Gerrad D., Insinga, Logan, Droz, Boris, Feinberg, Aryeh, Stenke, Andrea, Smith, Jo, Smith, Pete, and Winkel, Lenny H. E.
- Abstract
Reductions in sulfur (S) atmospheric deposition in recent decades have been attributed to S deficiencies in crops. Similarly, global soil selenium (Se) concentrations were predicted to drop, particularly in Europe, due to increases in leaching attributed to increases in aridity. Given its international importance in agriculture, reductions of essential elements, including S and Se, in European soils could have important impacts on nutrition and human health. Our objectives were to model current soil S and Se levels in Europe and predict concentration changes for the 21st century. We interrogated four machine-learning (ML) techniques, but after critical evaluation, only outputs for linear support vector regression (Lin-SVR) models for S and Se and the multilayer perceptron model (MLP) for Se were consistent with known mechanisms reported in literature. Other models exhibited overfitting even when differences in training and testing performance were low or non-existent. Furthermore, our results highlight that similarly performing models based on RMSE or R
2 can lead to drastically different predictions and conclusions, thus highlighting the need to interrogate machine learning models and to ensure they are consistent with known mechanisms reported in the literature. Both elements exhibited similar spatial patterns with predicted gains in Scandinavia versus losses in the central and Mediterranean regions of Europe, respectively, by the end of the 21st century for an extreme climate scenario. The median change was −5.5% for S (Lin-SVR) and −3.5% (MLP) and −4.0% (Lin-SVR) for Se. For both elements, modeled losses were driven by decreases in soil organic carbon, S and Se atmospheric deposition, and gains were driven by increases in evapotranspiration. [ABSTRACT FROM AUTHOR]- Published
- 2024
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8. Stratospheric circulation response to stratospheric aerosol injections remains uncertain.
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Diallo, Mohamadou, primary, Dunker, Nils, additional, Eichinger, Roland, additional, Ploeger, Felix, additional, Garny, Hella, additional, Ern, Manfred, additional, Ball, William, additional, Stenke, Andrea, additional, Revell, Laura, additional, Aquila, Valentina, additional, Tilmes, Simone, additional, Kinnison, Douglas, additional, Shepherd, Theodore, additional, and Hegglin, Michaela, additional
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- 2024
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9. Evaluating the Relationship between Interannual Variations in the Antarctic Ozone Hole and Southern Hemisphere Surface Climate in Chemistry–Climate Models
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Gillett, Zoe E., Arblaster, Julie M., Dittus, Andrea J., Deushi, Makoto, Jöckel, Patrick, Kinnison, Douglas E., Morgenstern, Olaf, Plummer, David A., Revell, Laura E., Rozanov, Eugene, Schofield, Robyn, Stenke, Andrea, Stone, Kane A., and Tilmes, Simone
- Published
- 2019
10. Reductions in the deposition of sulfur and selenium to agricultural soils pose risk of future nutrient deficiencies
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Feinberg, Aryeh, Stenke, Andrea, Peter, Thomas, Hinckley, Eve-Lyn S., Driscoll, Charles T., and Winkel, Lenny H. E.
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- 2021
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11. Importance of microphysical settings for climate forcing by stratospheric SO2 injections as modeled by SOCOL-AERv2.
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Vattioni, Sandro, Stenke, Andrea, Luo, Beiping, Chiodo, Gabriel, Sukhodolov, Timofei, Wunderlin, Elia, and Peter, Thomas
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STRATOSPHERIC aerosols , *ATMOSPHERIC chemistry , *SULFUR dioxide , *OZONE-depleting substances , *ATMOSPHERIC nucleation , *OZONE layer , *VOLCANIC eruptions - Abstract
Solar radiation modification by a sustained deliberate source of SO2 into the stratosphere (strat-SRM) has been proposed as an option for climate intervention. Global interactive aerosol–chemistry–climate models are often used to investigate the potential cooling efficiencies and associated side effects of hypothesized strat-SRM scenarios. A recent model intercomparison study for composition–climate models with interactive stratospheric aerosol suggests that the modeled climate response to a particular assumed injection strategy depends on the type of aerosol microphysical scheme used (e.g., modal or sectional representation) alongside host model resolution and transport. Compared to short-duration volcanic SO2 emissions, the continuous SO2 injections in strat-SRM scenarios may pose a greater challenge to the numerical implementation of microphysical processes such as nucleation, condensation, and coagulation. This study explores how changing the time steps and sequencing of microphysical processes in the sectional aerosol–chemistry–climate model SOCOL-AERv2 (40 mass bins) affects model-predicted climate and ozone layer impacts considering strat-SRM by SO2 injections of 5 and 25 Tg(S) yr −1 at 20 km altitude between 30° S and 30° N. The model experiments consider the year 2040 to be the boundary conditions for ozone-depleting substances and greenhouse gases (GHGs). We focus on the length of the microphysical time step and the call sequence of nucleation and condensation, the two competing sink processes for gaseous H2SO4. Under stratospheric background conditions, we find no effect of the microphysical setup on the simulated aerosol properties. However, at the high sulfur loadings reached in the scenarios injecting 25 Tg(S) yr −1 of SO2 with a default microphysical time step of 6 min, changing the call sequence from the default "condensation first" to "nucleation first" leads to a massive increase in the number densities of particles in the nucleation mode (R<0.01 µm) and a small decrease in coarse-mode particles (R>1 µm). As expected, the influence of the call sequence becomes negligible when the microphysical time step is reduced to a few seconds, with the model solutions converging to a size distribution with a pronounced nucleation mode. While the main features and spatial patterns of climate forcing by SO 2 injections are not strongly affected by the microphysical configuration, the absolute numbers vary considerably. For the extreme injection with 25 Tg(S) yr −1 , the simulated net global radiative forcing ranges from - 2.3 to - 5.3 Wm-2 , depending on the microphysical configuration. Nucleation first shifts the size distribution towards radii better suited for solar scattering (0.3 µm
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- 2024
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12. Chemical Impact of Stratospheric Alumina Particle Injection for Solar Radiation Modification and Related Uncertainties
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Vattioni, Sando, primary, Luo, Beiping, additional, Feinberg, Aryeh, additional, Stenke, Andrea, additional, Vockenhuber, Christof, additional, Weber, Rahel, additional, Dykema, John A., additional, Krieger, Ulrich K., additional, Ammann, Markus, additional, Keutsch, Frank, additional, Peter, Thomas, additional, and Chiodo, Gabriel, additional
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- 2023
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13. Isotopic source signatures: Impact of regional variability on the [formula omitted] trend and spatial distribution
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Feinberg, Aryeh I., Coulon, Ancelin, Stenke, Andrea, Schwietzke, Stefan, and Peter, Thomas
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- 2018
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14. Emerging role of wetland methane emissions in driving 21st century climate change
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Zhang, Zhen, Zimmermann, Niklaus E., Stenke, Andrea, Li, Xin, Hodson, Elke L., Zhu, Gaofeng, Huang, Chunlin, and Poulter, Benjamin
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- 2017
15. Stratospheric dynamics modulates ozone layer response to molecular oxygen variations
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Józefiak, Iga, primary, Sukhodolov, Timofei, additional, Egorova, Tatiana, additional, Chiodo, Gabriel, additional, Peter, Thomas, additional, Rieder, Harald, additional, Sedlacek, Jan, additional, Stenke, Andrea, additional, and Rozanov, Eugene, additional
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- 2023
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16. Weakening of springtime Arctic ozone depletion with climate change
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Friedel, Marina, primary, Chiodo, Gabriel, additional, Sukhodolov, Timofei, additional, Keeble, James, additional, Peter, Thomas, additional, Seeber, Svenja, additional, Stenke, Andrea, additional, Akiyoshi, Hideharu, additional, Rozanov, Eugene, additional, Plummer, David, additional, Jöckel, Patrick, additional, Zeng, Guang, additional, Morgenstern, Olaf, additional, and Josse, Béatrice, additional
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- 2023
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17. Supplementary material to "Importance of microphysical settings for climate forcing by stratospheric SO2 injections as modelled by SOCOL-AERv2"
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Vattioni, Sandro, primary, Stenke, Andrea, additional, Luo, Beiping, additional, Chiodo, Gabriel, additional, Sukhodolov, Timofei, additional, Wunderlin, Elia, additional, and Peter, Thomas, additional
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- 2023
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18. Importance of microphysical settings for climate forcing by stratospheric SO2 injections as modelled by SOCOL-AERv2
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Vattioni, Sandro, primary, Stenke, Andrea, additional, Luo, Beiping, additional, Chiodo, Gabriel, additional, Sukhodolov, Timofei, additional, Wunderlin, Elia, additional, and Peter, Thomas, additional
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- 2023
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19. The influence of springtime Arctic ozone recovery on stratospheric and surface climate
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Chiodo, Gabriel, primary, Friedel, Marina, additional, Seeber, Svenja, additional, Stenke, Andrea, additional, Sukhodolov, Timofei, additional, and Zilker, Franziska, additional
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- 2023
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20. Weakening of springtime Arctic ozone depletion with climate change
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Friedel, Marina, Chiodo, Gabriel, Sukhodolov, Timofei, Keeble, James, Peter, Thomas, Seeber, Svenja, Stenke, Andrea, Akiyoshi, Hideharu, Rozanov, Eugene, Plummer, David, Jöckel, Patrick, Zeng, Guang, Morgenstern, Olaf, Josse, Béatrice, Friedel, Marina, Chiodo, Gabriel, Sukhodolov, Timofei, Keeble, James, Peter, Thomas, Seeber, Svenja, Stenke, Andrea, Akiyoshi, Hideharu, Rozanov, Eugene, Plummer, David, Jöckel, Patrick, Zeng, Guang, Morgenstern, Olaf, and Josse, Béatrice
- Abstract
In the Arctic stratosphere, the combination of chemical ozone depletion by halogenated ozone-depleting substances (hODSs) and dynamic fluctuations can lead to severe ozone minima. These Arctic ozone minima are of great societal concern due to their health and climate impacts. Owing to the success of the Montreal Protocol, hODSs in the stratosphere are gradually declining, resulting in a recovery of the ozone layer. On the other hand, continued greenhouse gas (GHG) emissions cool the stratosphere, possibly enhancing the formation of polar stratospheric clouds (PSCs) and, thus, enabling more efficient chemical ozone destruction. Other processes, such as the acceleration of the Brewer-Dobson circulation, also affect stratospheric temperatures, further complicating the picture. Therefore, it is currently unclear whether major Arctic ozone minima will still occur at the end of the 21st century despite decreasing hODSs. We have examined this question for different emission pathways using simulations conducted within the Chemistry-Climate Model Initiative (CCMI-1 and CCMI-2022) and found large differences in the models' ability to simulate the magnitude of ozone minima in the present-day climate. Models with a generally too-cold polar stratosphere (cold bias) produce pronounced ozone minima under present-day climate conditions because they simulate more PSCs and, thus, high concentrations of active chlorine species (ClOx). These models predict the largest decrease in ozone minima in the future. Conversely, models with a warm polar stratosphere (warm bias) have the smallest sensitivity of ozone minima to future changes in hODS and GHG concentrations. As a result, the scatter among models in terms of the magnitude of Arctic spring ozone minima will decrease in the future. Overall, these results suggest that Arctic ozone minima will become weaker over the next decades, largely due to the decline in hODS abundances. We note that none of the models analysed here project a notab
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- 2023
21. Natural control on ozone pollution
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Stenke, Andrea
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- 2020
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22. In situ measurements of perturbations to stratospheric aerosol and modeled ozone and radiative impacts following the 2021 La Soufrière eruption.
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Li, Yaowei, Pedersen, Corey, Dykema, John, Vernier, Jean-Paul, Vattioni, Sandro, Pandit, Amit Kumar, Stenke, Andrea, Asher, Elizabeth, Thornberry, Troy, Todt, Michael A., Bui, Thao Paul, Dean-Day, Jonathan, and Keutsch, Frank N.
- Subjects
STRATOSPHERIC aerosols ,OZONE layer ,VOLCANIC eruptions ,OZONE ,VOLCANIC plumes ,OZONE layer depletion ,RADIATIVE forcing - Abstract
Stratospheric aerosols play important roles in Earth's radiative budget and in heterogeneous chemistry. Volcanic eruptions modulate the stratospheric aerosol layer by injecting particles and particle precursors like sulfur dioxide (SO 2) into the stratosphere. Beginning on 9 April 2021, La Soufrière erupted, injecting SO 2 into the tropical upper troposphere and lower stratosphere, yielding a peak SO 2 loading of 0.3–0.4 Tg. The resulting volcanic aerosol plumes dispersed predominately over the Northern Hemisphere (NH), as indicated by the CALIOP/CALIPSO satellite observations and model simulations. From June to August 2021 and May to July 2022, the NASA ER-2 high-altitude aircraft extensively sampled the stratospheric aerosol layer over the continental United States during the Dynamics and Chemistry of the Summer Stratosphere (DCOTSS) mission. These in situ aerosol measurements provide detailed insights into the number concentration, size distribution, and spatiotemporal variations of particles within volcanic plumes. Notably, aerosol surface area density and number density in 2021 were enhanced by a factor of 2–4 between 380–500 K potential temperature compared to the 2022 DCOTSS observations, which were minimally influenced by volcanic activity. Within the volcanic plume, the observed aerosol number density exhibited significant meridional and zonal variations, while the mode and shape of aerosol size distributions did not vary. The La Soufrière eruption led to an increase in the number concentration of small particles (<400 nm), resulting in a smaller aerosol effective diameter during the summer of 2021 compared to the baseline conditions in the summer of 2022, as observed in regular ER-2 profiles over Salina, Kansas. A similar reduction in aerosol effective diameter was not observed in ER-2 profiles over Palmdale, California, possibly due to the values that were already smaller in that region during the limited sampling period in 2022. Additionally, we modeled the eruption with the SOCOL-AERv2 aerosol–chemistry–climate model. The modeled aerosol enhancement aligned well with DCOTSS observations, although the direct comparison was complicated by issues related to the model's background aerosol burden. This study indicates that the La Soufrière eruption contributed approximately 0.6 % to Arctic and Antarctic ozone column depletion in both 2021 and 2022, which is well within the range of natural variability. The modeled top-of-atmosphere 1-year global average radiative forcing was -0.08 W m -2 clear-sky and -0.04 W m -2 all-sky. The radiative effects were concentrated in the tropics and NH midlatitudes and diminished to near-baseline levels after 1 year. [ABSTRACT FROM AUTHOR]
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- 2023
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23. Risks and benefits of stratospheric solid particle injection for climate intervention
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Vattioni, Sandro, primary, Weber, Rahel, additional, Klaus, Oliver, additional, Luo, Beiping, additional, Dykema, John, additional, Stenke, Andrea, additional, Feinberg, Aryehe, additional, Döbeli, Max, additional, Vockenhuber, Christof, additional, Kreiger, Ulrich, additional, Weers, Uwe, additional, Artiglia, Luca, additional, Yang, Huanyu, additional, Longetti, Luca, additional, Gabathuler, Jerome, additional, Ammann, Markus, additional, Keutsch, Frank, additional, Peter, Thomas, additional, and Chiodo, Gabriel, additional
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- 2023
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24. Tracking the environmental redistribution of arsenic (As) via the atmosphere: long l(As)ting & legacy effects
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Nghiem, Athena, primary, Winkel, Lenny, additional, and Stenke, Andrea, additional
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- 2023
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25. Integrating models and measurements to advance the understanding of Se cycling across the atmosphere-soil interface, session
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Winkel, Lenny, primary, Stenke, Andrea, additional, Breuninger, Esther, additional, and Tolu, Julie, additional
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- 2023
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26. Decision strategies for policy decisions under uncertainties: The case of mitigation measures addressing methane emissions from ruminants
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Hirsch Hadorn, Gertrude, Brun, Georg, Soliva, Carla Riccarda, Stenke, Andrea, and Peter, Thomas
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- 2015
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27. Attribution of the ozone band radiative flux bias in Chemistry-Climate Model Initiative (CCMI) models from satellites
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Kunze, Markus, Jöckel, Patrick, Shibata, Kiyotaka, Deushi, Makoto, Plummer, David, Revell, Laura, Stenke, Andrea, Rozanov, Eugene, Strode, Sarah, Oman, Luke, Paynter, David, Paulot, Fabien, Kulawik, Susan, Lamarque, Jean-François, Conley, Andrew, Worden, Helen, Miyazaki, Kazuyuki, Bowman, Kevin W, and Kuai, Le
- Abstract
UNKNOWN
- Published
- 2019
28. Attribution of the ozone band radiative flux bias in Chemistry-Climate Model Initiative (CCMI) models from satellites
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Kuai, Le, Bowman, Kevin W, Miyazaki, Kazuyuki, Worden, Helen, Conley, Andrew, Lamarque, Jean-François, Kulawik, Susan, Paulot, Fabien, Paynter, David, Oman, Luke, Strode, Sarah, Rozanov, Eugene, Stenke, Andrea, Revell, Laura, Plummer, David, Deushi, Makoto, Shibata, Kiyotaka, Jöckel, Patrick, and Kunze, Markus
- Published
- 2019
29. Attribution of the ozone band radiative flux bias in Chemistry-Climate Model Initiative (CCMI) models from satellites
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Kulawik, Susan, Kunze, Markus, Jöckel, Patrick, Shibata, Kiyotaka, Deushi, Makoto, Plummer, David, Revell, Laura, Stenke, Andrea, Rozanov, Eugene, Strode, Sarah, Oman, Luke, Paynter, David, Paulot, Fabien, Lamarque, Jean-François, Conley, Andrew, Miyazaki, Kazuyuki, Worden, Helen, Bowman, Kevin W, and Kuai, Le
- Abstract
UNKNOWN
- Published
- 2019
30. Methane Modeling: From Process Modeling to Global Climate Models
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Stenke, Andrea, Deckert, Rudolf, Gottschaldt, Klaus-Dirk, and Schumann, Ulrich, editor
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- 2012
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31. Effects of Arctic ozone on the stratospheric spring onset and its surface impact
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Friedel, Marina, Chiodo, Gabriel, Stenke, Andrea, Domeisen, Daniela I. V., and Peter, Thomas
- Abstract
Ozone in the Arctic stratosphere is subject to large interannual variability, driven by both chemical ozone depletion and dynamical variability. Anomalies in Arctic stratospheric ozone become particularly important in spring, when returning sunlight allows them to alter stratospheric temperatures via shortwave heating, thus modifying atmospheric dynamics. At the same time, the stratospheric circulation undergoes a transition in spring with the final stratospheric warming (FSW), which marks the end of winter. A causal link between stratospheric ozone anomalies and FSWs is plausible and might increase the predictability of stratospheric and tropospheric responses on sub-seasonal to seasonal timescales. However, it remains to be fully understood how ozone influences the timing and evolution of the springtime vortex breakdown. Here, we contrast results from chemistry climate models with and without interactive ozone chemistry to quantify the impact of ozone anomalies on the timing of the FSW and its effects on surface climate. We find that ozone feedbacks increase the variability in the timing of the FSW, especially in the lower stratosphere. In ozone-deficient springs, a persistent strong polar vortex and a delayed FSW in the lower stratosphere are partly due to the lack of heating by ozone in that region. High-ozone anomalies, on the other hand, result in additional shortwave heating in the lower stratosphere, where the FSW therefore occurs earlier. We further show that FSWs in high-ozone springs are predominantly followed by a negative phase of the Arctic Oscillation (AO) with positive sea level pressure anomalies over the Arctic and cold anomalies over Eurasia and Europe. These conditions are to a significant extent (at least 50 %) driven by ozone. In contrast, FSWs in low-ozone springs are not associated with a discernible surface climate response. These results highlight the importance of ozone-circulation coupling in the climate system and the potential value of interactive ozone chemistry for sub-seasonal to seasonal predictability., Atmospheric Chemistry and Physics, 22 (21), ISSN:1680-7375, ISSN:1680-7367
- Published
- 2022
32. Contemporary atmospheric oxygen levels maximize global protection by ozone
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Józefiak, Iga, primary, Sukhodolov, Timofei, additional, Egorova, Tatiana, additional, Chiodo, Gabriel, additional, Stenke, Andrea, additional, Rieder, Harald, additional, Peter, Thomas, additional, and Rozanov, Eugene, additional
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- 2022
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33. Effects of Arctic ozone on the stratospheric spring onset and its surface impact
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Friedel, Marina, primary, Chiodo, Gabriel, additional, Stenke, Andrea, additional, Domeisen, Daniela I. V., additional, and Peter, Thomas, additional
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- 2022
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34. The influence of future changes in springtime Arctic ozone on stratospheric and surface climate.
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Chiodo, Gabriel, Friedel, Marina, Seeber, Svenja, Domeisen, Daniela, Stenke, Andrea, Sukhodolov, Timofei, and Zilker, Franziska
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OZONE layer ,SPRING ,OZONE-depleting substances ,STRATOSPHERIC circulation ,POLAR vortex ,ATMOSPHERIC models - Abstract
Stratospheric ozone is expected to recover by the mid-century due to the success of the Montreal Protocol in regulating the emission of ozone-depleting substances (ODSs). In the Arctic, ozone abundances are projected to surpass historical levels due to the combined effect of decreasing ODSs and elevated greenhouse gases (GHGs). While long-term changes in stratospheric ozone have been shown to be a major driver of future surface climate in the Southern Hemisphere during summertime, the dynamical and climatic impacts of elevated ozone levels in the Arctic have not been investigated. In this study, we use two chemistry climate models (the SOlar Climate Ozone Links – Max Planck Ocean Model (SOCOL-MPIOM) and the Community Earth System Model – Whole Atmosphere Community Climate Model (CESM-WACCM)) to assess the climatic impacts of future changes in Arctic ozone on stratospheric dynamics and surface climate in the Northern Hemisphere (NH) during the 21st century. Under the high-emission scenario (RCP8.5) examined in this work, Arctic ozone returns to pre-industrial levels by the middle of the century. Thereby, the increase in Arctic ozone in this scenario warms the lower Arctic stratosphere; reduces the strength of the polar vortex, advancing its breakdown; and weakens the Brewer–Dobson circulation. The ozone-induced changes in springtime generally oppose the effects of GHGs on the polar vortex. In the troposphere, future changes in Arctic ozone induce a negative phase of the Arctic Oscillation, pushing the jet equatorward over the North Atlantic. These impacts of future ozone changes on NH surface climate are smaller than the effects of GHGs, but they are remarkably robust among the two models employed in this study, canceling out a portion of the GHG effects (up to 20 % over the Arctic). In the stratosphere, Arctic ozone changes cancel out a much larger fraction of the GHG-induced signal (up to 50 %–100 %), resulting in no overall change in the projected springtime stratospheric northern annular mode and a reduction in the GHG-induced delay of vortex breakdown of around 15 d. Taken together, our results indicate that future changes in Arctic ozone actively shape the projected changes in the stratospheric circulation and their coupling to the troposphere, thereby playing an important and previously unrecognized role as a driver of the large-scale atmospheric circulation response to climate change. [ABSTRACT FROM AUTHOR]
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- 2023
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35. Importance of microphysical settings for climate forcing by stratospheric SO2 injections as modelled by SOCOL-AERv2.
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Vattioni, Sandro, Stenke, Andrea, Beiping Luo, Chiodo, Gabriel, Sukhodolov, Timofei, Wunderlin, Elia, and Peter, Thomas
- Subjects
- *
STRATOSPHERIC aerosols , *ATMOSPHERIC chemistry , *SOLAR radiation management , *ATMOSPHERIC nucleation , *VOLCANIC eruptions , *OZONE layer , *RADIATIVE forcing - Abstract
Solar radiation management as a sustained deliberate source of SO2 into the stratosphere (strat-SRM) has been proposed as an option for climate intervention. Global interactive aerosol-chemistry-climate models are often used to investigate the potential cooling efficiencies and side effects of hypothesised strat-SRM scenarios. A recent strat-SRM model intercompar-ison study for composition-climate models with interactive stratospheric aerosol suggests that the modelled climate response 5 to a particular assumed injection strategy, depends on the type of aerosol microphysical scheme used (e.g., modal or sectional representation), alongside also host model resolution and transport. Compared to short-duration volcanic SO2 emission, the continuous SO2 injections in strat-SRM scenarios may pose a greater challenge to the numerical implementation of of microphysical processes such as nucleation, condensation, and coagulation. This study explores how changing the timesteps and sequencing of microphysical processes in the sectional aerosol-chemistry-climate model SOCOL-AERv2 (40 size bins) 10 affect model predicted climate and ozone layer impacts considering strat-SRM SO2 injections of of 5 and 25 Tg(S) yr-1 at 20 km altitude between 30°S and 30°N. The model experiments consider year 2040 boundary conditions for ozone depleting substances and green house gases. We focus on the length of the microphysical timestep and the call sequence of nucleation and condensation, the two competing sink processes for gaseous H2SO4. Under stratospheric background conditions, we find no effect of the microphysical setup on the simulated aerosol properties. However, at the high sulfur loadings reached in the 15 scenarios injecting 25 Mt/yr of sulfur with a default microphysical timesetp of 6 min, changing the call sequence from the default "condensation first" to "nucleation first" leads to a massive increase in the number densities of particles in the nucle-ation mode (R < 0.01 µm) and a small decrease in coarse mode particles (R > 1 µm). As expected, the influence of the call sequence becomes negligible when the microphysical timestep is reduced to a few seconds, with the model solutions converging to a size distribution with a pronounced nucleation mode. While the main features and spatial patterns of climate forcing 20 by SO2 injections are not strongly affected by the microphysical configuration, the absolute numbers vary considerably. For the extreme injection with 25 Tg(S) yr-1, the simulated net global radiative forcing ranges from -2.3 W m-2 to -5.3 W m-2, depending on the microphysical configuration. "Nucleation first" shifts the size distribution towards radii better suited for solar scattering (0.3 µm < R < 0.4 µm), enhancing the intervention efficiency. The size-distribution shift however generates more ultra-fine aerosol particles, increasing the surface area density, resulting in 10 DU less ozone (about 3% of total column) in 25 the northern midlatitudes and 20 DU less ozone (6%) over the polar caps, compared to the "condensation first" approach. Our results suggest that a reasonably short microphysical time step of 2 minutes or less must be applied to accurately capture the magnitude of the H2SO2 supersaturation resulting from SO2 injection scenarios or volcanic eruptions. Taken together these results underscore how structural aspects of model representation of aerosol microphysical processes become important under conditions of elevated stratospheric sulfur in determining atmospheric chemistry and climate impacts. [ABSTRACT FROM AUTHOR]
- Published
- 2023
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36. In situ measurements of perturbations to stratospheric aerosol and modeled ozone and radiative impacts following the 2021 La Soufrière eruption.
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Yaowei Li, Pedersen, Corey, Dykema, John, Vernier, Jean-Paul, Vattioni, Sandro, Pandit, Amit Kumar, Stenke, Andrea, Asher, Elizabeth, Thornberry, Troy, Todt, Michael A., ThaoPaul Bui, Dean-Day, Jonathan, and Keutsch, Frank N.
- Abstract
Stratospheric aerosols play important roles in Earth's radiative budget and in heterogeneous chemistry. Volcanic eruptions modulate the stratospheric aerosol layer by injecting particles and particle precursors like sulfur dioxide (SO2) into the stratosphere. Beginning on April 9th, 2021, La Soufrière erupted injecting SO2 into the tropical upper troposphere and lower stratosphere, yielding a peak SO2 loading of 0.3-0.4 Tg. The resulting volcanic aerosol plumes dispersed predominately over the northern hemisphere (NH), as indicated by the CALIOP/CALIPSO satellite observations and model simulations. From June to August 2021 and May to July 2022, the NASA ER-2 high-altitude aircraft extensively sampled the stratospheric aerosol layer over the continental United States during the Dynamics and Chemistry of the Summer Stratosphere (DCOTSS) mission. These in situ aerosol measurements provide detailed insights into the number concentration, size distribution, and spatiotemporal variations of particles within volcanic plumes. Notably, aerosol surface area density and number density in 2021 were enhanced by a factor of 2-4 between 380-500 K potential temperature compared to the 2022 DCOTSS observations, which were minimally influenced by volcanic activity. Within the volcanic plume, the observed aerosol number density exhibited significant meridional and zonal variations while the mode and shape of aerosol size distributions did not vary. The La Soufrière eruption led to an increase in the number concentration of small particles (<400 nm), resulting in a smaller aerosol effective diameter during the summer of 2021 compared to the baseline conditions in the summer of 2022, as observed in regular ER-2 profiles over Salina, Kansas. A similar reduction in aerosol effective diameter was not observed in ER-2 profiles over Palmdale, California, possibly due to the already smaller values in that region during the limited sampling period in 2022. The La Soufrière eruption was modeled with the SOCOL-AERv2 aerosol-chemistry-climate model. The modeled aerosol enhancement aligned well with DCOTSS observations, although the direct comparison was complicated by issues related to the model's background aerosol burden. This study indicates that the La Soufrière eruption contributed at most 0.6% to Arctic and Antarctic ozone column depletion in both 2021 and 2022, which is well within the range of natural variability. The modeled top-of-atmosphere one-year global average radiative forcing was -0.08 W/m2 clear-sky and -0.04 W/m2 all-sky. The radiative effects were concentrated in the tropics and NH midlatitudes and diminished to near-baseline levels after one year. [ABSTRACT FROM AUTHOR]
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- 2023
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37. Quantifying the Effect of Mixing on the Mean Age of Air in CCMVal-2 and CCMI-1 Models
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Dietmüller, Simone, Eichinger, Roland, Garny, Hella, Birner, Thomas, Boenisch, Harald, Pitari, Giovanni, Mancini, Eva, Visioni, Daniele, Stenke, Andrea, Revell, Laura, Rozanov, Eugene, Plummer, David A, Scinocca, John, Jöckel, Patrick, Oman, Luke, Deushi, Makoto, Kiyotaka, Shibata, Kinnison, Douglas E, Garcia, Rolando, Morgenstern, Olaf, Zeng, Guang, Stone, Kane Adam, and Schofield, Robyn
- Subjects
Meteorology And Climatology - Abstract
The stratospheric age of air (AoA) is a useful measure of the overall capabilities of a general circulation model (GCM) to simulate stratospheric transport. Previous studies have reported a large spread in the simulation of AoA by GCMs and coupled chemistry-climate models (CCMs). Compared to observational estimates, simulated AoA is mostly too low. Here we attempt to untangle the processes that lead to the AoA differences between the models and between models and observations. AoA is influenced by both mean transport by the residual circulation and two-way mixing; we quantify the effects of these processes using data from the CCM inter-comparison projects CCMVal-2 (Chemistry-Climate Model Validation Activity 2) and CCMI-1 (Chemistry-Climate Model Initiative, phase 1). Transport along the residual circulation is measured by the residual circulation transit time (RCTT). We interpret the difference between AoA and RCTT as additional aging by mixing. Aging by mixing thus includes mixing on both the resolved and subgrid scale. We find that the spread in AoA between the models is primarily caused by differences in the effects of mixing and only to some extent by differences in residual circulation strength. These effects are quantified by the mixing efficiency, a measure of the relative increase in AoA by mixing. The mixing efficiency varies strongly between the models from 0.24 to 1.02. We show that the mixing efficiency is not only controlled by horizontal mixing, but by vertical mixing and vertical diffusion as well. Possible causes for the differences in the models' mixing efficiencies are discussed. Differences in subgrid-scale mixing (including differences in advection schemes and model resolutions) likely contribute to the differences in mixing efficiency. However, differences in the relative contribution of resolved versus parameterized wave forcing do not appear to be related to differences in mixing efficiency or AoA.
- Published
- 2018
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38. Tropospheric Jet Response to Antarctic Ozone Depletion: An Update with Chemistry-Climate Model Initiative (CCMI) Models
- Author
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Son, Seok-Woo, Han, Bo-Reum, Garfinkel, Chaim I, Kim, Seo-Yeon, Park, Rokjin, Abraham, N. Luke, Akiyoshi, Hideharu, Archibald, Alexander T, Butchart, N, Chipperfield, Martyn P, Dameris, Martin, Deushi, Makoto, Dhomse, Sandip S, Hardiman, Steven C, Jockel, Patrick, Kinnison, Douglas, Michou, Martine, Morgenstern, Olaf, O’Connor, Fiona M, Oman, Luke D, Plummer, David A, Pozzer, Andrea, Revell, Laura E, Rozanov, Eugene, Stenke, Andrea, Stone, Kane, Tilmes, Simone, Yamashita, Yousuke, and Zeng, Guang
- Subjects
Geosciences (General) - Abstract
The Southern Hemisphere (SH) zonal-mean circulation change in response to Antarctic ozone depletion is re-visited by examining a set of the latest model simulations archived for the Chemistry-Climate Model Initiative (CCMI) project. All models reasonably well reproduce Antarctic ozone depletion in the late 20th century. The related SH-summer circulation changes, such as a poleward intensification of westerly jet and a poleward expansion of the Hadley cell, are also well captured. All experiments exhibit quantitatively the same multi-model mean trend, irrespective of whether the ocean is coupled or prescribed. Results are also quantitatively similar to those derived from the Coupled Model Intercomparison Project phase 5 (CMIP5) high-top model simulations in which the stratospheric ozone is mostly prescribed with monthly- and zonally-averaged values. These results suggest that the ozone-hole-induced SH-summer circulation changes are robust across the models irrespective of the specific chemistry-atmosphere-ocean coupling.
- Published
- 2018
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39. Multi-model Comparison of the Volcanic Sulfate Deposition from the 1815 Eruption of Mt. Tambora
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Marshall, Lauren, Schmidt, Anja, Toohey, Matthew, Carslaw, Ken S, Mann, Graham W, Sigl, Michael, Khodri, Myriam, Timmreck, Claudia, Zanchettin, Davide, Ball, William T, Bekki, Slimane, Brooke, James S. A, Dhomse, Sandip, Johnson, Colin, Lamarque, Jean-Francois, LeGrande, Allegra N, Mills, Michael J, Niemeier, Ulrike, Pope, James O, Poulain, Virginie, Robock, Alan, Rozanov, Eugene, Stenke, Andrea, Sukhodolov, Timofei, Tilmes, Simone, Tsigaridis, Kostas, and Tummon, Fiona
- Subjects
Geophysics - Abstract
The eruption of Mt. Tambora in 1815 was the largest volcanic eruption of the past 500 years. The eruption had significant climatic impacts, leading to the 1816 "year without a summer", and remains a valuable event from which to understand the climatic effects of large stratospheric volcanic sulfur dioxide injections. The eruption also resulted in one of the strongest and most easily identifiable volcanic sulfate signals in polar ice cores, which are widely used to reconstruct the timing and atmospheric sulfate loading of past eruptions. As part of the Model Intercomparison Project on the climatic response to Volcanic forcing (VolMIP), five state-of-the-art global aerosol models simulated this eruption. We analyze both simulated background (no Tambora) and volcanic (with Tambora) sulfate deposition to polar regions and compare to ice core records. The models simulate overall similar patterns of background sulfate deposition, although there are differences in regional details and magnitude. However, the volcanic sulfate deposition varies considerably between the models with differences in timing, spatial pattern and magnitude. Mean simulated deposited sulfate on Antarctica ranges from 19 to 264 kgkm-2 and on Greenland from 31 to 194 kgkm-2, as compared to the mean ice-core derived estimates of roughly 50 kgkm-2 for both Greenland and Antarctica. The ratio of the hemispheric atmospheric sulfate aerosol burden after the eruption to the average ice sheet deposited sulfate varies between models by up to a factor of 15. Sources of this inter-model variability include differences in both the formation and the transport of sulfate aerosol. Our results suggest that deriving relationships between sulfate deposited on ice sheets and atmospheric sulfate burdens from model simulations may be associated with greater uncertainties than previously thought.
- Published
- 2018
- Full Text
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40. Evidence for a Continuous Decline in Lower Stratospheric Ozone Offsetting Ozone Layer Recovery
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Ball, William T, Alsing, Justin, Mortlock, Daniel J, Staehelin, Johannes, Haigh, Joanna D, Peter, Thomas, Tummon, Fiona, Stuebi, Rene, Stenke, Andrea, Anderson, John, Bourassa, Adam, Davis, Sean M, Degenstein, Doug, Frith, Stacey, Froidevaux, Lucien, Roth, Chris, Sofieva, Viktoria, Wang, Ray, Wild, Jeanette, Yu, Pengfei, Ziemke, Jerald R, and Rozanov, Eugene V
- Subjects
Geosciences (General) - Abstract
Ozone forms in the Earth's atmosphere from the photodissociation of molecular oxygen, primarily in the tropical stratosphere. It is then transported to the extratropics by the Brewer-Dobson circulation (BDC), forming a protective "ozone layer" around the globe. Human emissions of halogen-containing ozone-depleting substances (hODSs) led to a decline in stratospheric ozone until they were banned by the Montreal Protocol, and since 1998 ozone in the upper stratosphere is rising again, likely the recovery from halogen-induced losses. Total column measurements of ozone between the Earth's surface and the top of the atmosphere indicate that the ozone layer has stopped declining across the globe, but no clear increase has been observed at latitudes between 60degS and 60degN outside the polar regions (60-90deg). Here we report evidence from multiple satellite measurements that ozone in the lower stratosphere between 60degS and 60degN has indeed continued to decline since 1998. We find that, even though upper stratospheric ozone is recovering, the continuing downward trend in the lower stratosphere prevails, resulting in a downward trend in stratospheric column ozone between 60degS and 60degN. We find that total column ozone between 60degS and 60degN appears not to have decreased only because of increases in tropospheric column ozone that compensate for the stratospheric decreases. The reasons for the continued reduction of lower stratospheric ozone are not clear; models do not reproduce these trends, and thus the causes now urgently need to be established.
- Published
- 2018
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41. Ozone Sensitivity to Varying Greenhouse Gases and Ozone-Depleting Substances in CCMI-1 Simulations
- Author
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Morgenstern, Olaf, Stone, Kane A, Schofield, Robyn, Akiyoshi, Hideharu, Yamashita, Yousuke, Kinnison, Douglas E, Garcia, Rolando R, Sudo, Kengo, Plummer, David A, Scinocca, John, Oman, Luke D, Manyin, Michael E, Zeng, Guang, Rozanov, Eugene, Stenke, Andrea, Revell, Laura E, Pitari, Giovanni, Mancini, Eva, Genova, Glauco Di, Visioni, Daniele, Dhomse, Sandip S, and Chipperfield, Martyn P
- Subjects
Geosciences (General) - Abstract
Ozone fields simulated for the first phase of the Chemistry-Climate Model Initiative (CCMI-1) will be used as forcing data in the 6th Coupled Model Intercomparison Project. Here we assess, using reference and sensitivity simulations produced for CCMI-1, the suitability of CCMI-1 model results for this process, investigating the degree of consistency amongst models regarding their responses to variations in individual forcings. We consider the influences of methane, nitrous oxide, a combination of chlorinated or brominated ozone-depleting substances, and a combination of carbon dioxide and other greenhouse gases. We find varying degrees of consistency in the models' responses in ozone to these individual forcings, including some considerable disagreement. In particular, the response of total-column ozone to these forcings is less consistent across the multi-model ensemble than profile comparisons. We analyse how stratospheric age of air, a commonly used diagnostic of stratospheric transport, responds to the forcings. For this diagnostic we find some salient differences in model behaviour, which may explain some of the findings for ozone. The findings imply that the ozone fields derived from CCMI-1 are subject to considerable uncertainties regarding the impacts of these anthropogenic forcings. We offer some thoughts on how to best approach the problem of generating a consensus ozone database from a multi-model ensemble such as CCMI-1.
- Published
- 2018
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42. 29. Connecting the spheres: modeling global trace element biogeochemical cycling
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Nghiem, Athena, Stenke, Andrea, and Winkel, Lenny
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ComputingMethodologies_GENERAL - Abstract
Poster presentation
- Published
- 2022
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43. Effects of Arctic ozone on the stratospheric spring onset and its surface response
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Friedel, Marina, primary, Chiodo, Gabriel, additional, Stenke, Andrea, additional, Domeisen, Daniela I. V., additional, and Peter, Thomas, additional
- Published
- 2022
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44. The influence of springtime Arctic ozone recovery on stratospheric and surface climate.
- Author
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Chiodo, Gabriel, Friedel, Marina, Seeber, Svenja, Stenke, Andrea, Sukhodolov, Timofei, and Zilker, Franziska
- Abstract
Stratospheric ozone is expected to recover by mid-century due to the success of the Montreal Protocol in regulating the emission of ozone-depleting substances (ODSs). In the Arctic, ozone abundances are projected to surpass historical levels due to the combined effect of decreasing ODSs and elevated greenhouse gases (GHGs). While ozone recovery has been shown to be a major driver of future surface climate in the Southern Hemisphere during summertime, the dynamical and climatic impacts of elevated ozone levels in the Arctic have not been investigated. In this study, we use two chemistry climate models (SOCOL-MPIOM and CESM-WACCM) to assess the climatic impacts of Arctic ozone recovery on stratospheric dynamics and surface climate in the Northern Hemisphere (NH) during the 21st century. Under the high-emission scenario (RCP8.5) examined in this work, Arctic ozone returns to pre-industrial levels by the middle of the century. Thereby, it warms the lower Arctic stratosphere, reduces the strength of the polar vortex, advancing its breakdown, and weakening the Brewer-Dobson circulation. In the troposphere, Arctic ozone recovery induces a negative phase of the Arctic Oscillation, pushing the jet equatorward over the Atlantic. These impacts of ozone recovery in the NH are smaller than the effects of GHGs, but they are remarkably robust among the two models employed in this study, cancelling out some of the GHG effects. Taken together, our results indicate that Arctic ozone recovery actively shapes the projected changes in the stratospheric circulation and their coupling to the troposphere, thereby playing an important and previously unrecognized role as driver of the large-scale atmospheric circulation response to climate change [ABSTRACT FROM AUTHOR]
- Published
- 2023
- Full Text
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45. Review of the Global Models Used Within Phase 1 of the Chemistry-Climate Model Initiative (CCMI)
- Author
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Morgenstern, Olaf, Hegglin, Michaela I, Rozanov, Eugene, O’Connor, Fiona M, Abraham, N. Luke, Akiyoshi, Hideharu, Archibald, Alexander T, Bekki, Slimane, Butchart, Neal, Chipperfield, Martyn P, Deushi, Makoto, Dhomse, Sandip S, Garcia, Rolando R, Hardiman, Steven C, Horowitz, Larry W, Jockel, Patrick, Josse, Beatrice, Kinnison, Douglas, Lin, Meiyun, Mancini, Eva, Manyin, Michael E, Marchand, Marion, Marecal, Virginie, Michou, Martine, Oman, Luke D, Pitari, Giovanni, Plummer, David A, Revell, Laura E, Saint-Martin, David, Schofield, Robyn, Stenke, Andrea, Stone, Kane, Sudo, Kengo, Tanaka, Taichu Y, Tilmes, Simone, Yamashita, Yousuke, Yoshida, Kohei, and Zeng, Guang
- Subjects
Geosciences (General) - Abstract
We present an overview of state-of-the-art chemistry-climate and chemistry transport models that are used within phase 1 of the Chemistry-Climate Model Initiative (CCMI-1). The CCMI aims to conduct a detailed evaluation of participating models using process-oriented diagnostics derived from observations in order to gain confidence in the models' projections of the stratospheric ozone layer, tropospheric composition, air quality, where applicable global climate change, and the interactions between them. Interpretation of these diagnostics requires detailed knowledge of the radiative, chemical, dynamical, and physical processes incorporated in the models. Also an understanding of the degree to which CCMI-1 recommendations for simulations have been followed is necessary to understand model responses to anthropogenic and natural forcing and also to explain inter-model differences. This becomes even more important given the ongoing development and the ever-growing complexity of these models. This paper also provides an overview of the available CCMI-1 simulations with the aim of informing CCMI data users.
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- 2017
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46. The influence of ozone feedbacks on Final Stratospheric Warmings and their surface impact
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Friedel, Marina, primary, Chiodo, Gabriel, additional, Stenke, Andrea, additional, Domeisen, Daniela, additional, and Peter, Thomas, additional
- Published
- 2022
- Full Text
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47. Stratospheric Aerosol--Observations, Processes, and Impact on Climate
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Kresmer, Stefanie, Thomason, Larry W, von Hobe, Marc, Hermann, Markus, Deshler, Terry, Timmreck, Claudia, Toohey, Matthew, Stenke, Andrea, Schwarz, Joshua P, Weigel, Ralf, Fueglistaler, Stephan, Prata, Fred J, Vernier, Jean-Paul, Schlager, Hans, Barnes, John E, Antuna-Marrero, Juan-Carlos, Fairlie, Duncan, Palm, Mathias, Mahieu, Emmanuel, Notholt, Justus, Rex, Markus, Bingen, Christine, Vanhellemont, Filip, Bourassa, Adam, Plane, John M. C, Klocke, Daniel, Carn, Simon A, Clarisse, Lieven, Trickl, Thomas, Neeley, Ryan, James, Alexander D, Rieger, Landon, Wilson, James C, and Meland, Brian
- Subjects
Meteorology And Climatology - Abstract
Interest in stratospheric aerosol and its role in climate have increased over the last decade due to the observed increase in stratospheric aerosol since 2000 and the potential for changes in the sulfur cycle induced by climate change. This review provides an overview about the advances in stratospheric aerosol research since the last comprehensive assessment of stratospheric aerosol was published in 2006. A crucial development since 2006 is the substantial improvement in the agreement between in situ and space-based inferences of stratospheric aerosol properties during volcanically quiescent periods. Furthermore, new measurement systems and techniques, both in situ and space based, have been developed for measuring physical aerosol properties with greater accuracy and for characterizing aerosol composition. However, these changes induce challenges to constructing a long-term stratospheric aerosol climatology. Currently, changes in stratospheric aerosol levels less than 20% cannot be confidently quantified. The volcanic signals tend to mask any nonvolcanically driven change, making them difficult to understand. While the role of carbonyl sulfide as a substantial and relatively constant source of stratospheric sulfur has been confirmed by new observations and model simulations, large uncertainties remain with respect to the contribution from anthropogenic sulfur dioxide emissions. New evidence has been provided that stratospheric aerosol can also contain small amounts of nonsulfatematter such as black carbon and organics. Chemistry-climate models have substantially increased in quantity and sophistication. In many models the implementation of stratospheric aerosol processes is coupled to radiation and/or stratospheric chemistry modules to account for relevant feedback processes.
- Published
- 2016
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48. Modeling the Sulfate Aerosol Evolution After Recent Moderate Volcanic Activity, 2008–2012
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Brodowsky, Christina, primary, Sukhodolov, Timofei, additional, Feinberg, Aryeh, additional, Höpfner, Michael, additional, Peter, Thomas, additional, Stenke, Andrea, additional, and Rozanov, Eugene, additional
- Published
- 2021
- Full Text
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49. Atmosphere–ocean–aerosol–chemistry–climate model SOCOLv4.0: description and evaluation
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Sukhodolov, Timofei, primary, Egorova, Tatiana, additional, Stenke, Andrea, additional, Ball, William T., additional, Brodowsky, Christina, additional, Chiodo, Gabriel, additional, Feinberg, Aryeh, additional, Friedel, Marina, additional, Karagodin-Doyennel, Arseniy, additional, Peter, Thomas, additional, Sedlacek, Jan, additional, Vattioni, Sandro, additional, and Rozanov, Eugene, additional
- Published
- 2021
- Full Text
- View/download PDF
50. The response of mesospheric H₂O and CO to solar irradiance variability in models and observations
- Author
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Karagodin-Doyennel, Arsenij, Rozanov, Eugene, Kuchar, Ales, Ball, William, Arsenovic, Pavle, Remsberg, Ellis, Jöckel, Patrick, Kunze, Markus, Plummer, David A., Stenke, Andrea, Marsh, Daniel, Kinnison, Doug, and Peter, Thomas
- Subjects
water vapour ,EMAC ,chemistry climate modeling ,MESSy ,upper atmosphere ,CCMI ,Erdsystem-Modellierung ,ESCiMo ,mesosphere ,chemistry climate initiative ,Earth System Chemistry Integrated Modelling ,carbon monoxide - Abstract
Water vapor (H2O) is the source of reactive hydrogen radicals in the middle atmosphere, whereas carbon monoxide (CO), being formed by CO2 photolysis, is suitable as a dynamical tracer. In the mesosphere, both H2O and CO are sensitive to solar irradiance (SI) variability because of their destruction/production by solar radiation. This enables us to analyze the solar signal in both models and observed data. Here, we evaluate the mesospheric H2O and CO response to solar irradiance variability using the Chemistry-Climate Model Initiative (CCMI-1) simulations and satellite observations. We analyzed the results of four CCMI models (CMAM, EMAC-L90MA, SOCOLv3, and CESM1-WACCM 3.5) operated in CCMI reference simulation REF-C1SD in specified dynamics mode, covering the period from 1984–2017. Multiple linear regression analyses show a pronounced and statistically robust response of H2O and CO to solar irradiance variability and to the annual and semiannual cycles. For periods with available satellite data, we compared the simulated solar signal against satellite observations, namely the GOZCARDS composite for 1992–2017 for H2O and Aura/MLS measurements for 2005–2017 for CO. The model results generally agree with observations and reproduce an expected negative and positive correlation for H2O and CO, respectively, with solar irradiance. However, the magnitude of the response and patterns of the solar signal varies among the considered models, indicating differences in the applied chemical reaction and dynamical schemes, including the representation of photolyzes. We suggest that there is no dominating thermospheric influence of solar irradiance in CO, as reported in previous studies, because the response to solar variability is comparable with observations in both low-top and high-top models. We stress the importance of this work for improving our understanding of the current ability and limitations of state-of-the-art models to simulate a solar signal in the chemistry and dynamics of the middle atmosphere.
- Published
- 2021
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