47 results on '"Tummon, F."'
Search Results
2. Variability between Hirst-type pollen traps is reduced by resistance-free flow adjustment
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Triviño, M. M., Maya-Manzano, J. M., Tummon, F., Clot, B., Grewling, Ł., Schmidt-Weber, C., and Buters, J.
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- 2023
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3. Correction to: Variability between Hirst-type pollen traps is reduced by resistance-free flow adjustment
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Triviño, M. M., Maya-Manzano, J. M., Tummon, F., Clot, B., Grewling, Ł., Schmidt-Weber, C., and Buters, J.
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- 2023
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4. High solar cycle spectral variations inconsistent with stratospheric ozone observations
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Ball, W. T., Haigh, J. D., Rozanov, E. V., Kuchar, A., Sukhodolov, T., Tummon, F., Shapiro, A. V., and Schmutz, W.
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Physics - Atmospheric and Oceanic Physics - Abstract
Some of the natural variability in climate is understood to come from changes in the Sun. A key route whereby the Sun may influence surface climate is initiated in the tropical stratosphere by the absorption of solar ultraviolet (UV) radiation by ozone, leading to a modification of the temperature and wind structures and consequently to the surface through changes in wave propagation and circulation. While changes in total, spectrally-integrated, solar irradiance lead to small variations in global mean surface temperature, the `top-down' UV effect preferentially influences on regional scales at mid-to-high latitudes with, in particular, a solar signal noted in the North Atlantic Oscillation (NAO). The amplitude of the UV variability is fundamental in determining the magnitude of the climate response but understanding of the UV variations has been challenged recently by measurements from the SOlar Radiation and Climate Experiment (SORCE) satellite, which show UV solar cycle changes up to 10 times larger than previously thought. Indeed, climate models using these larger UV variations show a much greater response, similar to NAO observations. Here we present estimates of the ozone solar cycle response using a chemistry-climate model (CCM) in which the effects of transport are constrained by observations. Thus the photolytic response to different spectral solar irradiance (SSI) datasets can be isolated. Comparison of the results with the solar signal in ozone extracted from observational datasets yields significantly discriminable responses. According to our evaluation the SORCE UV dataset is not consistent with the observed ozone response whereas the smaller variations suggested by earlier satellite datasets, and by UV data from empirical solar models, are in closer agreement with the measured stratospheric variations. Determining the most appropriate SSI variability to apply in models..., Comment: This is the original version submitted to Nature Geoscience in July 2015 with the title "Ozone observations reveal lower solar cycle spectral variations", this has changed to the one given above. 4 Figures, Nature Geoscience, 2016, http://www.nature.com/ngeo/journal/vaop/ncurrent/full/ngeo2640.html
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- 2016
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5. Attribution of extreme weather to anthropogenic greenhouse gas emissions: Sensitivity to spatial and temporal scales
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Angélil, O, Stone, DA, Tadross, M, Tummon, F, Wehner, M, and Knutti, R
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attribution ,extremes ,spatial ,Meteorology & Atmospheric Sciences - Abstract
Recent studies have examined the anthropogenic contribution to specific extreme weather events, such as the European (2003) and Russian (2010) heat waves. While these targeted studies examine the attributable risk of an event occurring over a specified temporal and spatial domain, it is unclear how effectively their attribution statements can serve as a proxy for similar events occurring at different temporal and spatial scales. Here we test the sensitivity of attribution results to the temporal and spatial scales of extreme precipitation and temperature events by applying a probabilistic event attribution framework to the output of two global climate models, each run with and without anthropogenic greenhouse gas emissions. Attributable risk tends to be more sensitive to the temporal than spatial scale of the event, increasing as event duration increases. Globally, correlations between attribution statements at different spatial scales are very strong for temperature extremes and moderate for heavy precipitation extremes. © 2014. American Geophysical Union. All Rights Reserved.
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- 2014
6. The influence of Middle Range Energy Electrons on atmospheric chemistry and regional climate
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Arsenovic, P., Rozanov, E., Stenke, A., Funke, B., Wissing, J.M., Mursula, K., Tummon, F., and Peter, T.
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- 2016
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7. The need for Pan-European automatic pollen and fungal spore monitoring: A stakeholder workshop position paper
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Tummon, F., Alados-Arboledas, Lucas, Bonini, Maira, Guinot, Benjamin, Hicke, Martin, Jacob, C., Kendorvski, Vladimir, McCairns, William, Peuch, Vincent-Henri, Pfaar, Oliver, Sicard, Michaël, Sikoparija, Branko, Clot, Bernard, Tummon, F., Alados-Arboledas, Lucas, Bonini, Maira, Guinot, Benjamin, Hicke, Martin, Jacob, C., Kendorvski, Vladimir, McCairns, William, Peuch, Vincent-Henri, Pfaar, Oliver, Sicard, Michaël, Sikoparija, Branko, and Clot, Bernard
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Background: Information about airborne pollen concentrations is required by a range of end users, particularly from the health sector who use both observations and forecasts to diagnose and treat allergic patients. Manual methods are the standard for such measurements but, despite the range of pollen taxa that can be identified, these techniques suffer from a range of drawbacks. This includes being available at low temporal resolution (usually daily averages) and with a delay (usually 3–9 days from the measurement). Recent technological developments have made possible automatic pollen measurements, which are available at high temporal resolution and in real time, although currently only scattered in a few locations across Europe. Materials & Methods: To promote the development of an extensive network across Europe and to ensure that this network will respond to end user needs, a stakeholder workshop was organised under the auspices of the EUMETNET AutoPollen Programme. Participants discussed requirements for the groups they represented, ranging from the need for information at various spatial scales, at high temporal resolution, and for targeted services to be developed. Results: The provision of real-time information is likely to lead to a notable decrease in the direct and indirect health costs associated with allergy in Europe, currently estimated between €50–150 billion/year.. Discussion & Conclusion: A European measurement network to meet end user requirements would thus more than pay for itself in terms of potential annual savings and provide significant impetus to research across a range of disciplines from climate science and public health to agriculture and environmental management.
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- 2021
8. Multimodel Estimates of Atmospheric Lifetimes of Long-Lived Ozone-Depleting Substances: Present and Future
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Chipperfield, M. P, Liang, Q, Strahan, S. E, Morgenstern, O, Dhomse, S. S, Abraham, N. L, Archibald, A. T, Bekki, S, Braesicke, P, Di Genova, G, Fleming, E. L, Hardiman, S. C, Iachetti, D, Jackman, C. H, Kinnison, D. E, Marchand, M, Pitari, G, Pyle, J. A, Rozanov, E, Stenke, A, and Tummon, F
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Meteorology And Climatology ,Geophysics - Abstract
We have diagnosed the lifetimes of long-lived source gases emitted at the surface and removed in the stratosphere using six three-dimensional chemistry-climate models and a two-dimensional model. The models all used the same standard photochemical data. We investigate the effect of different definitions of lifetimes, including running the models with both mixing ratio (MBC) and flux (FBC) boundary conditions. Within the same model, the lifetimes diagnosed by different methods agree very well. Using FBCs versus MBCs leads to a different tracer burden as the implied lifetime contained in theMBC value does not necessarilymatch a model's own calculated lifetime. In general, there are much larger differences in the lifetimes calculated by different models, the main causes of which are variations in the modeled rates of ascent and horizontal mixing in the tropical midlower stratosphere. The model runs have been used to compute instantaneous and steady state lifetimes. For chlorofluorocarbons (CFCs) their atmospheric distribution was far from steady state in their growth phase through to the 1980s, and the diagnosed instantaneous lifetime is accordingly much longer. Following the cessation of emissions, the resulting decay of CFCs is much closer to steady state. For 2100 conditions the model circulation speeds generally increase, but a thicker ozone layer due to recovery and climate change reduces photolysis rates. These effects compensate so the net impact on modeled lifetimes is small. For future assessments of stratospheric ozone, use of FBCs would allow a consistent balance between rate of CFC removal and model circulation rate.
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- 2014
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9. Training EarlyCareer Polar Weather and Climate Researchers
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Tummon, F, Day, J, and Svensson, G
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GeneralLiterature_MISCELLANEOUS - Abstract
Thepolar prediction problemis inherently multidisciplinary and requires cooperation across a wide community. Thus, an international group of agencies specifically designed a 10-day training course to bring together a wide group of students and lecturers to cover important topics related to polar prediction. Topics included satellite and conventional observation techniques; numerical modeling of the polar atmosphere, sea ice, and ocean; and data assimilation andmodel evaluation. The course included an innovative combination of theory lectures, practical exercises, and fieldwork, as well as a dedicated science communication program, each of which forms a crucial pillar of the prediction problem.
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- 2018
10. Multi-model comparison of the volcanic sulfate deposition from the 1815 eruption of Mt. Tambora
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Marshall, L., Schmidt, A., Toohey, M., Carslaw, K. S., Mann, G. W., Sigl, M., Khodri, Myriam, Timmreck, C., Zanchettin, D., Ball, W. T., Bekki, S., Brooke, J. S. A., Dhomse, S., Johnson, C., Lamarque, J. F., LeGrande, A. N., Mills, M. J., Niemeier, U., Pope, J. O., Poulain, V., Robock, A., Rozanov, E., Stenke, A., Sukhodolov, T., Tilmes, S., Tsigaridis, K., Tummon, F., Institute for Climate and Atmospheric Science [Leeds] (ICAS), School of Earth and Environment [Leeds] (SEE), University of Leeds-University of Leeds, Leibniz-Institut für Meereswissenschaften (IFM-GEOMAR), Max-Planck-Institut für Meteorologie (MPI-M), Max-Planck-Gesellschaft, National Centre for Atmospheric Science [Leeds] (NCAS), Natural Environment Research Council (NERC), Laboratory of Environmental Chemistry [Villigen] (LUC), Paul Scherrer Institute (PSI), Océan et variabilité du climat (VARCLIM), Laboratoire d'Océanographie et du Climat : Expérimentations et Approches Numériques (LOCEAN), Muséum national d'Histoire naturelle (MNHN)-Institut de Recherche pour le Développement (IRD)-Institut national des sciences de l'Univers (INSU - CNRS)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS)-Institut Pierre-Simon-Laplace (IPSL (FR_636)), École normale supérieure - Paris (ENS-PSL), Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université de Versailles Saint-Quentin-en-Yvelines (UVSQ)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut national des sciences de l'Univers (INSU - CNRS)-École polytechnique (X)-Centre National d'Études Spatiales [Toulouse] (CNES)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS)-Université Paris Cité (UPCité)-École normale supérieure - Paris (ENS-PSL), Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université de Versailles Saint-Quentin-en-Yvelines (UVSQ)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-École polytechnique (X)-Centre National d'Études Spatiales [Toulouse] (CNES)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS)-Université Paris Cité (UPCité)-Muséum national d'Histoire naturelle (MNHN)-Institut de Recherche pour le Développement (IRD)-Institut national des sciences de l'Univers (INSU - CNRS)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS)-Institut Pierre-Simon-Laplace (IPSL (FR_636)), Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université de Versailles Saint-Quentin-en-Yvelines (UVSQ)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-École polytechnique (X)-Centre National d'Études Spatiales [Toulouse] (CNES)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS)-Université Paris Cité (UPCité), Max Planck Institute for Meteorology (MPI-M), Department of Environmental Sciences, Informatics and Statistics [Venezia], University of Ca’ Foscari [Venice, Italy], Institute for Atmospheric and Climate Science [Zürich] (IAC), Eidgenössische Technische Hochschule - Swiss Federal Institute of Technology [Zürich] (ETH Zürich), Physikalisch-Meteorologisches Observatorium Davos/World Radiation Center (PMOD/WRC), STRATO - LATMOS, Laboratoire Atmosphères, Milieux, Observations Spatiales (LATMOS), Université de Versailles Saint-Quentin-en-Yvelines (UVSQ)-Institut national des sciences de l'Univers (INSU - CNRS)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS)-Université de Versailles Saint-Quentin-en-Yvelines (UVSQ)-Institut national des sciences de l'Univers (INSU - CNRS)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS), School of Chemistry [Leeds], University of Leeds, Met Office Hadley Centre for Climate Change (MOHC), United Kingdom Met Office [Exeter], Atmospheric Chemistry Observations and Modeling Laboratory (ACOML), National Center for Atmospheric Research [Boulder] (NCAR), NASA Goddard Space Flight Center (GSFC), British Antarctic Survey (BAS), Processus de la variabilité climatique tropicale et impacts (PARVATI), Muséum national d'Histoire naturelle (MNHN)-Institut de Recherche pour le Développement (IRD)-Université Pierre et Marie Curie - Paris 6 (UPMC)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS)-Institut Pierre-Simon-Laplace (IPSL (FR_636)), Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université de Versailles Saint-Quentin-en-Yvelines (UVSQ)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut national des sciences de l'Univers (INSU - CNRS)-Université Paris Diderot - Paris 7 (UPD7)-École polytechnique (X)-Centre National d'Études Spatiales [Toulouse] (CNES)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS)-École normale supérieure - Paris (ENS-PSL), Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université de Versailles Saint-Quentin-en-Yvelines (UVSQ)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris Diderot - Paris 7 (UPD7)-École polytechnique (X)-Centre National d'Études Spatiales [Toulouse] (CNES)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS)-Muséum national d'Histoire naturelle (MNHN)-Institut de Recherche pour le Développement (IRD)-Université Pierre et Marie Curie - Paris 6 (UPMC)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS)-Institut Pierre-Simon-Laplace (IPSL (FR_636)), Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université de Versailles Saint-Quentin-en-Yvelines (UVSQ)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris Diderot - Paris 7 (UPD7)-École polytechnique (X)-Centre National d'Études Spatiales [Toulouse] (CNES)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS), Department of Environmental Sciences [New Brunswick], School of Environmental and Biological Sciences [New Brunswick], Rutgers, The State University of New Jersey [New Brunswick] (RU), Rutgers University System (Rutgers)-Rutgers University System (Rutgers)-Rutgers, The State University of New Jersey [New Brunswick] (RU), Rutgers University System (Rutgers)-Rutgers University System (Rutgers), NASA Goddard Institute for Space Studies (GISS), Center for Climate Systems Research [New York] (CCSR), Columbia University [New York], The Arctic University of Norway [Tromsø, Norway] (UiT), US National Science Foundation grant AGS-1430051, German Federal Ministry of Education and Research (BMBF), research program 'MiKliP' (FKZ: 01LP1517B, Swiss National Science Foundation grant 20F121_138017, NERC grant NEK/K012150/1, ANR-10-LABX-0018,L-IPSL,LabEx Institut Pierre Simon Laplace (IPSL): Understand climate and anticipate future changes(2010), European Project: 603557,EC:FP7:ENV,FP7-ENV-2013-two-stage,STRATOCLIM(2013), Institut de Recherche pour le Développement (IRD)-Centre National de la Recherche Scientifique (CNRS)-Institut national des sciences de l'Univers (INSU - CNRS)-Université Pierre et Marie Curie - Paris 6 (UPMC)-Muséum national d'Histoire naturelle (MNHN)-Institut Pierre-Simon-Laplace (IPSL (FR_636)), École normale supérieure - Paris (ENS Paris), Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université de Versailles Saint-Quentin-en-Yvelines (UVSQ)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut national des sciences de l'Univers (INSU - CNRS)-Université Paris Diderot - Paris 7 (UPD7)-École polytechnique (X)-Centre National d'Études Spatiales [Toulouse] (CNES)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS)-École normale supérieure - Paris (ENS Paris), Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université de Versailles Saint-Quentin-en-Yvelines (UVSQ)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris Diderot - Paris 7 (UPD7)-École polytechnique (X)-Centre National d'Études Spatiales [Toulouse] (CNES)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS)-Institut de Recherche pour le Développement (IRD)-Centre National de la Recherche Scientifique (CNRS)-Institut national des sciences de l'Univers (INSU - CNRS)-Université Pierre et Marie Curie - Paris 6 (UPMC)-Muséum national d'Histoire naturelle (MNHN)-Institut Pierre-Simon-Laplace (IPSL (FR_636)), Sorbonne Université (SU)-Université de Versailles Saint-Quentin-en-Yvelines (UVSQ)-Centre National de la Recherche Scientifique (CNRS)-Institut national des sciences de l'Univers (INSU - CNRS)-Sorbonne Université (SU)-Université de Versailles Saint-Quentin-en-Yvelines (UVSQ)-Centre National de la Recherche Scientifique (CNRS)-Institut national des sciences de l'Univers (INSU - CNRS), and The Arctic University of Norway (UiT)
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[SDU.STU.VO]Sciences of the Universe [physics]/Earth Sciences/Volcanology ,Settore GEO/12 - Oceanografia e Fisica dell'Atmosfera - Abstract
Source at https://doi.org/10.5194/acp-18-2307-2018. 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 analyse 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 kg km−2 and on Greenland from 31 to 194 kg km−2, as compared to the mean ice-core-derived estimates of roughly 50 kg km−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.
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- 2018
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11. The Upper Stratospheric Solar Cycle Ozone Response
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Ball, W. T., primary, Rozanov, E. V., additional, Alsing, J., additional, Marsh, D. R., additional, Tummon, F., additional, Mortlock, D. J., additional, Kinnison, D., additional, and Haigh, J. D., additional
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- 2019
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12. The Upper Stratospheric Solar Cycle Ozone Response
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Ball, W. T., Rozanov, E., Alsing, J., Marsh, D. R., Tummon, F., Mortlock, Daniel J., Kinnison, D., Haigh, J. D., Ball, W. T., Rozanov, E., Alsing, J., Marsh, D. R., Tummon, F., Mortlock, Daniel J., Kinnison, D., and Haigh, J. D.
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The solar cycle (SC) stratospheric ozone response is thought to influence surface weather and climate. To understand the chain of processes and ensure climate models adequately represent them, it is important to detect and quantify an accurate SC ozone response from observations. Chemistry climate models (CCMs) and observations display a range of upper stratosphere (1-10 hPa) zonally averaged spatial responses; this and the recommended data set for comparison remains disputed. Recent data-merging advancements have led to more robust observational data. Using these data, we show that the observed SC signal exhibits an upper stratosphere U-shaped spatial structure with lobes emanating from the tropics (5-10 hPa) to high altitudes at midlatitudes (1-3 hPa). We confirm this using two independent chemistry climate models in specified dynamics mode and an idealized timeslice experiment. We recommend the BASIC(v2) ozone composite to best represent historical upper stratospheric solar variability, and that those based on SBUV alone should not be used. Plain Language Summary Changes in the output of the Sun are thought to influence surface weather and climate through a set of processes initiated by the enhancement of upper stratosphere (32-48 km) ozone. In order to understand and assess the solar impact on the climate system, it is important that models reproduce the observed solar signal. However, the recommended data set for comparison with climate models remains disputed. We use newly improved observed ozone composites to determine both why there is disagreement between composites and which is most likely to be correct. We find that artifact-corrected composites represent the response better than those based on SBUV data alone. Further, we identify a U-shaped spatial structure with lobes emanating from the tropics to high altitudes at midlatitudes. An idealized chemistry climate model experiment and simulations considering historical meteorological conditions both support
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- 2019
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13. Overview of the antarctic circumnavigation expedition: Study of preindustrial-like aerosols and their climate effects (ACE-SPACE)
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Schmale, J, Baccarini, A, Thurnherr, I, Henning, S, Efraim, A, Regayre, L, Bolas, C, Hartmann, M, Welti, A, Lehtipalo, K, Aemisegger, F, Tatzelt, C, Landwehr, S, Modini, RL, Tummon, F, Johnson, JS, Harris, N, Schnaiter, M, Toffoli, A, Derkani, M, Bukowiecki, N, Stratmann, F, Dommen, J, Sperger, UB, Wernli, H, Rosenfeld, D, Gysel-Beer, M, Carslaw, KS, Schmale, J, Baccarini, A, Thurnherr, I, Henning, S, Efraim, A, Regayre, L, Bolas, C, Hartmann, M, Welti, A, Lehtipalo, K, Aemisegger, F, Tatzelt, C, Landwehr, S, Modini, RL, Tummon, F, Johnson, JS, Harris, N, Schnaiter, M, Toffoli, A, Derkani, M, Bukowiecki, N, Stratmann, F, Dommen, J, Sperger, UB, Wernli, H, Rosenfeld, D, Gysel-Beer, M, and Carslaw, KS
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The first results from ACE-SPACE highlight that the Southern Ocean is a region with highly heterogeneous aerosol properties. The areas around the strong westerly wind belt are characterized by significant sea spray contributions to the total particle and CCN number concentrations in the MBL. Future work will link detailed wave and wind observations to sea spray production. In the Ross and Amundsen Sea polynyas (leg 2), biogenic emissions appear to play an important role for CCN abundance. There are a number of open questions associated with this observation. First, even though this particular region was probed during a phytoplankton bloom period, it was not the only region with microbial activity but showed the clearest link to high CCN concentrations. Hence, either DMS production from dimethylsulfoniopropionate in the water and/or DMS fluxes into the atmosphere were enhanced. Second, the major pathway of how MSA is added to the particle phase remains to be identified. There are two possibilities: It can condense from the gas into the particle phase, or it can be added during cloud processing. The latter process would be consistent with the reduced efficiency of wet removal because of droplet evaporation or snowflake sublimation in the cold and dry airmasses from Antarctica. Our results also indicate that the absence of MSA-related processes in the aerosol model could explain the underestimation of CCN concentration, particularly in high aerosol-MSA regions. Given that the number of CCN influence Nd, this is an important issue to solve, especially close to the coast of Antarctica where clouds could impact the surface snow mass balance by influencing both the surface energy budget and precipitation. Further studies are planned that more closely investigate the linkages between CCN number concentrations and model simulations that take DMS emissions fluxes and particle phase MSA into account. A comparison of satellite-retrieved Nd90 and ship-based measurements of CCN s
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- 2019
14. Deriving Global OH Abundance and Atmospheric Lifetimes for Long-Lived Gases: A Search for CH 3 CCl 3 Alternatives
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Liang, Q, Chipperfield, MP, Fleming, EL, Abraham, NL, Braesicke, P, Burkholder, JB, Daniel, JS, Dhomse, S, Fraser, PJ, Hardiman, SC, Jackman, CH, Kinnison, DE, Krummel, PB, Montzka, SA, Morgenstern, O, McCulloch, A, Mühle, J, Newman, PA, Orkin, VL, Pitari, G, Prinn, RG, Rigby, M, Rozanov, E, Stenke, A, Tummon, F, Velders, GJM, Visioni, D, and Weiss, RF
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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.
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- 2017
15. Tropospheric ozone in CCMI models and Gaussian process emulation to understand biases in the SOCOLv3 chemistry-climate model
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Revell, LE, Stenke, A, Tummon, F, Feinberg, A, Rozanov, E, Peter, T, Abraham, NL, Akiyoshi, H, Archibald, AT, Butchart, N, Deushi, M, Joeckel, P, Kinnison, D, Michou, M, Morgenstern, O, O'Connor, FM, Oman, LD, Pitari, G, Plummer, DA, Schofield, R, Stone, K, Tilmes, S, Visioni, D, Yamashita, Y, Zeng, G, Revell, LE, Stenke, A, Tummon, F, Feinberg, A, Rozanov, E, Peter, T, Abraham, NL, Akiyoshi, H, Archibald, AT, Butchart, N, Deushi, M, Joeckel, P, Kinnison, D, Michou, M, Morgenstern, O, O'Connor, FM, Oman, LD, Pitari, G, Plummer, DA, Schofield, R, Stone, K, Tilmes, S, Visioni, D, Yamashita, Y, and Zeng, G
- Abstract
Previous multi-model intercomparisons have shown that chemistry-climate models exhibit significant biases in tropospheric ozone compared with observations. We investigate annual-mean tropospheric column ozone in 15 models participating in the SPARC-IGAC (Stratosphere-troposphere Processes And their Role in Climate-International Global Atmospheric Chemistry) Chemistry-Climate Model Initiative (CCMI). These models exhibit a positive bias, on average, of up to 40 %-50 % in the Northern Hemisphere compared with observations derived from the Ozone Monitoring Instrument and Microwave Limb Sounder (OMI/MLS), and a negative bias of up to ∼ 30 % in the Southern Hemisphere. SOCOLv3.0 (version 3 of the Solar-Climate Ozone Links CCM), which participated in CCMI, simulates global-mean tropospheric ozone columns of 40.2 DU- A pproximately 33 % larger than the CCMI multi-model mean. Here we introduce an updated version of SOCOLv3.0, SOCOLv3.1, which includes an improved treatment of ozone sink processes, and results in a reduction in the tropospheric column ozone bias of up to 8 DU, mostly due to the inclusion of N2O5 hydrolysis on tropospheric aerosols. As a result of these developments, tropospheric column ozone amounts simulated by SOCOLv3.1 are comparable with several other CCMI models. We apply Gaussian process emulation and sensitivity analysis to understand the remaining ozone bias in SOCOLv3.1. This shows that ozone precursors (nitrogen oxides (NOx), carbon monoxide, methane and other volatile organic compounds, VOCs) are responsible for more than 90 % of the variance in tropospheric ozone. However, it may not be the emissions inventories themselves that result in the bias, but how the emissions are handled in SOCOLv3.1, and we discuss this in the wider context of the other CCMI models. Given that the emissions data set to be used for phase 6 of the Coupled Model Intercomparison Project includes approximately 20 % more NOx than the data set used for CCMI, further work is u
- Published
- 2018
16. The influence of Middle Range Energy Electrons on atmospheric chemistry and regional climate
- Author
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Arsenovic, P. (P.), Rozanov, E. (E.), Stenke, A. (A.), Funke, B. (B.), Wissing, J. (J.M.), Mursula, K. (Kalevi), Tummon, F. (F.), Peter, T. (T.), Arsenovic, P. (P.), Rozanov, E. (E.), Stenke, A. (A.), Funke, B. (B.), Wissing, J. (J.M.), Mursula, K. (Kalevi), Tummon, F. (F.), and Peter, T. (T.)
- Abstract
We investigate the influence of Middle Range Energy Electrons (MEE; typically 30–300 keV) precipitation on the atmosphere using the SOCOL3-MPIOM chemistry-climate model with coupled ocean. Model simulations cover the 2002–2010 period for which ionization rates from the AIMOS dataset and atmospheric composition observations from MIPAS are available. Results show that during geomagnetically active periods MEE significantly increase the amount of NOy and HOx in the polar winter mesosphere, in addition to other particles and sources, resulting in local ozone decreases of up to 35%. These changes are followed by an intensification of the polar night jet, as well as mesospheric warming and stratospheric cooling. The contribution of MEE also substantially enhances the difference in the ozone anomalies between geomagnetically active and quiet periods. Comparison with MIPAS NOy observations indicates that the additional source of NOy from MEE improves the model results, however substantial underestimation above 50 km remains and requires better treatment of the NOy source from the thermosphere. A surface air temperature response is detected in several regions, with the most pronounced warming occurring in the Antarctic during austral winter. Surface warming of up to 2 K is also seen over continental Asia during boreal winter.
- Published
- 2016
17. The influence of Middle Range Energy Electrons on atmospheric chemistry and regional climate
- Author
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Academy of Finland, Swiss National Science Foundation, Arsenovic, P., Rozanov, E., Stenke, A., Funke, Bernd, Wissing, J.M., Mursula, K., Tummon, F., Peter, Thomas, Academy of Finland, Swiss National Science Foundation, Arsenovic, P., Rozanov, E., Stenke, A., Funke, Bernd, Wissing, J.M., Mursula, K., Tummon, F., and Peter, Thomas
- Abstract
We investigate the influence of Middle Range Energy Electrons (MEE; typically 30-300 keV) precipitation on the atmosphere using the SOCOL3-MPIOM chemistry-climate model with coupled ocean. Model simulations cover the 2002-2010 period for which ionization rates from the AIMOS dataset and atmospheric composition observations from MIPAS are available. Results show that during geomagnetically active periods MEE significantly increase the amount of NO and HO in the polar winter mesosphere, in addition to other particles and sources, resulting in local ozone decreases of up to 35%. These changes are followed by an intensification of the polar night jet, as well as mesospheric warming and stratospheric cooling. The contribution of MEE also substantially enhances the difference in the ozone anomalies between geomagnetically active and quiet periods. Comparison with MIPAS NO observations indicates that the additional source of NO from MEE improves the model results, however substantial underestimation above 50 km remains and requires better treatment of the NO source from the thermosphere. A surface air temperature response is detected in several regions, with the most pronounced warming occurring in the Antarctic during austral winter. Surface warming of up to 2 K is also seen over continental Asia during boreal winter. © 2016 The Authors
- Published
- 2016
18. Global OH abundance and lifetime of long-lived OH-removal species inferred from CH3CCl3: Implications from box model inversion analysis and flux-based CCMs
- Author
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Liang, Q, Chipperfield, Mp, Rigby, M, Morganstern, O, Velders, Gjm, Abraham, L, Braesicke, P, Dhomse, S, Fleming, El, Hardiman, S, Iachetti, D, Jackman, Ch, Kinnison, De, Pitari, Giovanni, Rozanov, E, Stenke, A, and Tummon, F.
- Subjects
Lifetime ,OH-removal species ,CCMs - Published
- 2013
19. High solar cycle spectral variations inconsistent with stratospheric ozone observations
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Ball, W. T., primary, Haigh, J. D., additional, Rozanov, E. V., additional, Kuchar, A., additional, Sukhodolov, T., additional, Tummon, F., additional, Shapiro, A. V., additional, and Schmutz, W., additional
- Published
- 2016
- Full Text
- View/download PDF
20. Past changes in the vertical distribution of ozone - Part 3: analysis and interpretation of trends
- Author
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Harris, Neil R. P, Hassler, B, Tummon, F, Bodeker, G E, Hubert, D, Petropavlovskikh, I, Steinbrecht, W, Anderson, John, Bhartia, P K, Boone, C D, Bourassa, A E, Davis, S M, Degenstein, D A, Delcloo, A, Frith, S M, Froidevaux, L, Godin-Beekmann, S, Jones, Nicholas B, Kurylo, M J, Kyrola, E, Laine, M, Leblanc, S T, Lambert, J C, Liley, B, Mahieu, Emmanuel, Maycock, A, de Maziere, M, Parrish, A, Querel, R, Rosenlof, K H, Roth, C, Sioris, C, Staehelin, J, Stolarski, R S, Stubi, R, Tamminen, J, Vigouroux, C, Walker, K, Wang, H J, Wild, J, Zawodny, J M, Harris, Neil R. P, Hassler, B, Tummon, F, Bodeker, G E, Hubert, D, Petropavlovskikh, I, Steinbrecht, W, Anderson, John, Bhartia, P K, Boone, C D, Bourassa, A E, Davis, S M, Degenstein, D A, Delcloo, A, Frith, S M, Froidevaux, L, Godin-Beekmann, S, Jones, Nicholas B, Kurylo, M J, Kyrola, E, Laine, M, Leblanc, S T, Lambert, J C, Liley, B, Mahieu, Emmanuel, Maycock, A, de Maziere, M, Parrish, A, Querel, R, Rosenlof, K H, Roth, C, Sioris, C, Staehelin, J, Stolarski, R S, Stubi, R, Tamminen, J, Vigouroux, C, Walker, K, Wang, H J, Wild, J, and Zawodny, J M
- Abstract
Trends in the vertical distribution of ozone are reported and compared for a number of new and recently revised data sets. The amount of ozone-depleting compounds in the stratosphere (as measured by equivalent effective stratospheric chlorine - EESC) was maximised in the second half of the 1990s. We examine the periods before and after the peak to see if any change in trend is discernible in the ozone record that might be attributable to a change in the EESC trend, though no attribution is attempted. Prior to 1998, trends in the upper stratosphere (~ 45 km, 4 hPa) are found to be −5 to −10 % per decade at mid-latitudes and closer to −5 % per decade in the tropics. No trends are found in the mid-stratosphere (28 km, 30 hPa). Negative trends are seen in the lower stratosphere at mid-latitudes in both hemispheres and in the deep tropics. However, it is hard to be categorical about the trends in the lower stratosphere for three reasons: (i) there are fewer measurements, (ii) the data quality is poorer, and (iii) the measurements in the 1990s are perturbed by aerosols from the Mt Pinatubo eruption in 1991. These findings are similar to those reported previously even though the measurements for the main satellite and ground-based records have been revised. There is no sign of a continued negative trend in the upper stratosphere since 1998: instead there is a hint of an average positive trend of ~ 2 % per decade in mid-latitudes and ~ 3 % per decade in the tropics. The significance of these upward trends is investigated using different assumptions of the independence of the trend estimates found from different data sets. The averaged upward trends are significant if the trends derived from various data sets are assumed to be independent (as in Pawson et al., 2014) but are generally not significant if the trends are not independent. This occurs because many of the underlying measurement records are used in more than one merged data set. At this point it is not possible to s
- Published
- 2015
21. The changing ozone depletion potential of N2O in a future climate
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Revell, L. E., primary, Tummon, F., additional, Salawitch, R. J., additional, Stenke, A., additional, and Peter, T., additional
- Published
- 2015
- Full Text
- View/download PDF
22. Past changes in the vertical distribution of ozone – Part 3: Analysis and interpretation of trends
- Author
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Harris, N. R. P., primary, Hassler, B., additional, Tummon, F., additional, Bodeker, G. E., additional, Hubert, D., additional, Petropavlovskikh, I., additional, Steinbrecht, W., additional, Anderson, J., additional, Bhartia, P. K., additional, Boone, C. D., additional, Bourassa, A., additional, Davis, S. M., additional, Degenstein, D., additional, Delcloo, A., additional, Frith, S. M., additional, Froidevaux, L., additional, Godin-Beekmann, S., additional, Jones, N., additional, Kurylo, M. J., additional, Kyrölä, E., additional, Laine, M., additional, Leblanc, S. T., additional, Lambert, J.-C., additional, Liley, B., additional, Mahieu, E., additional, Maycock, A., additional, de Mazière, M., additional, Parrish, A., additional, Querel, R., additional, Rosenlof, K. H., additional, Roth, C., additional, Sioris, C., additional, Staehelin, J., additional, Stolarski, R. S., additional, Stübi, R., additional, Tamminen, J., additional, Vigouroux, C., additional, Walker, K. A., additional, Wang, H. J., additional, Wild, J., additional, and Zawodny, J. M., additional
- Published
- 2015
- Full Text
- View/download PDF
23. Drivers of the tropospheric ozone budget throughout the 21st century under the medium-high climate scenario RCP 6.0
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Revell, L. E., primary, Tummon, F., additional, Stenke, A., additional, Sukhodolov, T., additional, Coulon, A., additional, Rozanov, E., additional, Garny, H., additional, Grewe, V., additional, and Peter, T., additional
- Published
- 2015
- Full Text
- View/download PDF
24. Intercomparison of vertically resolved merged satellite ozone data sets: interannual variability and long-term trends
- Author
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Tummon, F., primary, Hassler, B., additional, Harris, N. R. P., additional, Staehelin, J., additional, Steinbrecht, W., additional, Anderson, J., additional, Bodeker, G. E., additional, Bourassa, A., additional, Davis, S. M., additional, Degenstein, D., additional, Frith, S. M., additional, Froidevaux, L., additional, Kyrölä, E., additional, Laine, M., additional, Long, C., additional, Penckwitt, A. A., additional, Sioris, C. E., additional, Rosenlof, K. H., additional, Roth, C., additional, Wang, H.-J., additional, and Wild, J., additional
- Published
- 2015
- Full Text
- View/download PDF
25. Western African Aerosols Modelling with Updated Biomass Burning Emission Inventories in the Frame of the AMMA-IDAF Program
- Author
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LIOUSSE C., GUILLAUME B., GREGOIRE Jean-Marie, MALLET M., GALY-LACAUX1 C., PONT V., AKPO A., BEDOU M., CASTERA P., DUNGALL L., GARDRAT E., GRANIER C., KONARE A., MALAVELLE F., MARISCAL A., MIEVILLE Aude, ROSSET R., SERÇA D., SOLMON F., TUMMON F., YOBOUÉ V., and VAN VELTHOVEN P.
- Abstract
African biomass burning emission inventories for gases and particles (AMMABB) have been constructed at a resolution of 1km by 1km with daily coverage for the 2000-2007 period. They have been evaluated using the ORISAM-TM4 global chemistry transport model, which includes a detailed aerosol module. This paper discussed comparisons between modelled results and new AMMA measurements for surface BC and OC concentrations and scattering coefficients, aerosol optical depths and single scattering albedo from sunphotometer and satellite data. Major aerosol seasonal and interannual evolution over the period 2004-2007 observed at Djougou (Benin) and Banizoumbou (Niger) AMMA/IDAF sites are well reproduced by our global model, showing the importance of using accurate biomass burning emissions. It is the first time to our knowledge that a global model treating core/shell mixing for optical calculations reproduces aerosol optical depths (AOD) values of the same order than satellite and AERONET data. Comparison of simulated and measured concentrations for different class sizes simulated by the model give information on possible refinements of the emissions, according to the particulate size fraction, which have an impact on aerosol optical properties., JRC.DDG.H.3-Global environement monitoring
- Published
- 2010
26. Intercomparison of vertically resolved merged satellite ozone data sets: interannual variability and long-term trends
- Author
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Tummon, F., primary, Hassler, B., additional, Harris, N. R. P., additional, Staehelin, J., additional, Steinbrecht, W., additional, Anderson, J., additional, Bodeker, G. E., additional, Bourassa, A., additional, Davis, S. M., additional, Degenstein, D., additional, Frith, S. M., additional, Froidevaux, L., additional, Kyrölä, E., additional, Laine, M., additional, Long, C., additional, Penckwitt, A. A., additional, Sioris, C. E., additional, Rosenlof, K. H., additional, Roth, C., additional, Wang, H. J., additional, and Wild, J., additional
- Published
- 2014
- Full Text
- View/download PDF
27. Trajectory matching of ozonesondes and MOZAIC measurements in the UTLS – Part 2: Application to the global ozonesonde network
- Author
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Staufer, J., primary, Staehelin, J., additional, Stübi, R., additional, Peter, T., additional, Tummon, F., additional, and Thouret, V., additional
- Published
- 2014
- Full Text
- View/download PDF
28. Trajectory matching of ozonesondes and MOZAIC measurements in the UTLS – Part 1: Method description and application at Payerne, Switzerland
- Author
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Staufer, J., primary, Staehelin, J., additional, Stübi, R., additional, Peter, T., additional, Tummon, F., additional, and Thouret, V., additional
- Published
- 2013
- Full Text
- View/download PDF
29. Trajectory matching of ozonesondes and MOZAIC measurements in the UTLS – Part 2: Application to the global ozonesonde network
- Author
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Staufer, J., primary, Staehelin, J., additional, Stübi, R., additional, Peter, T., additional, Tummon, F., additional, and Thouret, V., additional
- Published
- 2013
- Full Text
- View/download PDF
30. Updated African biomass burning emission inventories in the framework of the AMMA-IDAF program, with an evaluation of combustion aerosols
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Liousse, C., primary, Guillaume, B., additional, Grégoire, J. M., additional, Mallet, M., additional, Galy, C., additional, Pont, V., additional, Akpo, A., additional, Bedou, M., additional, Castéra, P., additional, Dungall, L., additional, Gardrat, E., additional, Granier, C., additional, Konaré, A., additional, Malavelle, F., additional, Mariscal, A., additional, Mieville, A., additional, Rosset, R., additional, Serça, D., additional, Solmon, F., additional, Tummon, F., additional, Assamoi, E., additional, Yoboué, V., additional, and Van Velthoven, P., additional
- Published
- 2010
- Full Text
- View/download PDF
31. Simulation of the direct and semidirect aerosol effects on the southern Africa regional climate during the biomass burning season
- Author
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Tummon, F., primary, Solmon, F., additional, Liousse, C., additional, and Tadross, M., additional
- Published
- 2010
- Full Text
- View/download PDF
32. Western african aerosols modelling with updated biomass burning emission inventories in the frame of the AMMA-IDAF program
- Author
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Liousse, C., primary, Guillaume, B., additional, Grégoire, J. M., additional, Mallet, M., additional, Galy, C., additional, Pont, V., additional, Akpo, A., additional, Bedou, M., additional, Castéra, P., additional, Dungall, L., additional, Gardrat, E., additional, Granier, C., additional, Konaré, A., additional, Malavelle, F., additional, Mariscal, A., additional, Mieville, A., additional, Rosset, R., additional, Serça, D., additional, Solmon, F., additional, Tummon, F., additional, Assamoi, E., additional, Yoboué, V., additional, and Van Velthoven, P., additional
- Published
- 2010
- Full Text
- View/download PDF
33. The changing ozone depletion potential of N2O in a future climate.
- Author
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Revell, L. E., Tummon, F., Salawitch, R. J., Stenke, A., and Peter, T.
- Published
- 2015
- Full Text
- View/download PDF
34. Trajectory matching of ozonesondes and MOZAIC measurements in the UTLS – Part 2: Application to the global ozonesonde network.
- Author
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Staufer, J., Staehelin, J., Stübi, R., Peter, T., Tummon, F., and Thouret, V.
- Subjects
OZONESONDES ,TROPOPAUSE ,STRATOSPHERE ,GREENHOUSE gases ,NITROGEN oxides ,ATMOSPHERIC water vapor measurement ,ELECTRIC batteries ,PHOTOMETERS - Abstract
Ozone, an important greenhouse gas, has the largest climate forcing in the tropopause region, meaning that knowledge of long-term ozone changes in the upper troposphere/ lower stratosphere (UTLS) is particularly important. Here, we perform a 16 yr comparison (1994–2009) of UTLS ozone measurements from balloon-borne ozonesondes and MOZAIC (measurements of ozone, water vapor, carbon monoxide and nitrogen oxides by in-service Airbus aircraft). The analysis uses trajectories computed from ERA-Interim wind fields to find matches between the two measurement platforms. Ozonesonde data quality is most critical in the UTLS, where natural variability is high, particularly close to the tropopause. On average, at the 28 launch sites considered, ozone mixing ratios measured by the sondes exceed MOZAIC data by 5– 15 %, with differences being smaller in the LS than in the UT at many launch sites. For most sites, sondes and MOZAIC data are in close agreement after 1998. Before 1998 ozone mixing ratios measured by the Brewer–Mast (BM) sondes and Electrochemical Concentration Cell (ECC) sondes are systematically (up to 20%) higher than the MOZAIC UV photometers. The reason for this large difference remains unclear. Results also show that after 1998 large background current signals may affect ozonesonde performance, limiting the determination of reliable ozone trends in the UTLS. Sonde measurements appear to be insensitive to changing the type of ECC ozonesonde, provided the cathode sensing solution strength remains unchanged. Only Scoresbysund (Greenland) showed systematically higher readings after changing from Science Pump Corporation sondes to ENSCI Corporation sondes, while keeping a 1.0% KI cathode electrolyte. This suggests that ECC sondes, provided their background current and sensing solutions are properly monitored, are robust and reliable tools for ozone trend studies in the UTLS. [ABSTRACT FROM AUTHOR]
- Published
- 2013
- Full Text
- View/download PDF
35. Western african aerosols modelling with updated biomass burning emission inventories in the frame of the AMMA-IDAF program.
- Author
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Liousse, C., Guillaume, B., Gr'egoire, J. M., Mallet, M., Galy, C., Pont, V., Akpo, A., Bedou, M., Cast'era, P., Dungall, L., Gardrat, E., Granier, C., Konar'e, A., Malavelle, F., Mariscal, A., Mieville, A., Rosset, R., Serca, D., Solmon, F., and Tummon, F.
- Abstract
African biomass burning emission inventories for gases and particles (AMMABB) have been constructed at a resolution of 1 km by 1km with daily coverage for the 2000-2007 period. They have been evaluated using the ORISAM-TM4 global chemistry transport model, which includes a detailed aerosol module. This paper discussed comparisons between modelled results and new AMMA measurements for surface BC and OC concentrations and scattering coefficients, aerosol optical depths and single scattering albedo from sunphotometer and satellite data. Major aerosol seasonal and interannual evolution over the period 2004-2007 observed at Djougou (Benin) and Banizoumbou (Niger) AMMA/IDAF sites are well reproduced by our global model, showing the importance of using accurate biomass burning emissions. It is the first time to our knowledge that a global model treating core/shell mixing for optical calculations reproduces aerosol optical depths (AOD) values of the same order as satellite and AERONET data. Comparison of simulated and measured concentrations for different class sizes simulated by the model give information on possible refinements of the emissions, according to the particulate size fraction, which have an impact on aerosol optical properties. [ABSTRACT FROM AUTHOR]
- Published
- 2010
- Full Text
- View/download PDF
36. EAACI guidelines on environmental science for allergy and asthma: The impact of short-term exposure to outdoor air pollutants on asthma-related outcomes and recommendations for mitigation measures.
- Author
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Agache I, Annesi-Maesano I, Cecchi L, Biagioni B, Chung KF, Clot B, D'Amato G, Damialis A, Del Giacco S, Dominguez-Ortega J, Galàn C, Gilles S, Holgate S, Jeebhay M, Kazadzis S, Nadeau K, Papadopoulos N, Quirce S, Sastre J, Tummon F, Traidl-Hoffmann C, Walusiak-Skorupa J, Jutel M, and Akdis CA
- Subjects
- Humans, Air Pollution adverse effects, Asthma etiology, Asthma prevention & control, Air Pollutants adverse effects, Environmental Exposure adverse effects
- Abstract
The EAACI Guidelines on the impact of short-term exposure to outdoor pollutants on asthma-related outcomes provide recommendations for prevention, patient care and mitigation in a framework supporting rational decisions for healthcare professionals and patients to individualize and improve asthma management and for policymakers and regulators as an evidence-informed reference to help setting legally binding standards and goals for outdoor air quality at international, national and local levels. The Guideline was developed using the GRADE approach and evaluated outdoor pollutants referenced in the current Air Quality Guideline of the World Health Organization as single or mixed pollutants and outdoor pesticides. Short-term exposure to all pollutants evaluated increases the risk of asthma-related adverse outcomes, especially hospital admissions and emergency department visits (moderate certainty of evidence at specific lag days). There is limited evidence for the impact of traffic-related air pollution and outdoor pesticides exposure as well as for the interventions to reduce emissions. Due to the quality of evidence, conditional recommendations were formulated for all pollutants and for the interventions reducing outdoor air pollution. Asthma management counselled by the current EAACI guidelines can improve asthma-related outcomes but global measures for clean air are needed to achieve significant impact., (© 2024 European Academy of Allergy and Clinical Immunology and John Wiley & Sons Ltd.)
- Published
- 2024
- Full Text
- View/download PDF
37. Atmospheric isoprene measurements reveal larger-than-expected Southern Ocean emissions.
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Ferracci V, Weber J, Bolas CG, Robinson AD, Tummon F, Rodríguez-Ros P, Cortés-Greus P, Baccarini A, Jones RL, Galí M, Simó R, Schmale J, and Harris NRP
- Abstract
Isoprene is a key trace component of the atmosphere emitted by vegetation and other organisms. It is highly reactive and can impact atmospheric composition and climate by affecting the greenhouse gases ozone and methane and secondary organic aerosol formation. Marine fluxes are poorly constrained due to the paucity of long-term measurements; this in turn limits our understanding of isoprene cycling in the ocean. Here we present the analysis of isoprene concentrations in the atmosphere measured across the Southern Ocean over 4 months in the summertime. Some of the highest concentrations ( >500 ppt) originated from the marginal ice zone in the Ross and Amundsen seas, indicating the marginal ice zone is a significant source of isoprene at high latitudes. Using the United Kingdom Earth System Model we show that current estimates of sea-to-air isoprene fluxes underestimate observed isoprene by a factor >20. A daytime source of isoprene is required to reconcile models with observations. The model presented here suggests such an increase in isoprene emissions would lead to >8% decrease in the hydroxyl radical in regions of the Southern Ocean, with implications for our understanding of atmospheric oxidation and composition in remote environments, often used as proxies for the pre-industrial atmosphere., (© 2024. The Author(s).)
- Published
- 2024
- Full Text
- View/download PDF
38. Automatic real-time monitoring of fungal spores: the case of Alternaria spp.
- Author
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Erb S, Berne A, Burgdorfer N, Clot B, Graber MJ, Lieberherr G, Sallin C, Tummon F, and Crouzy B
- Abstract
We present the first implementation of the monitoring of airborne fungal spores in real-time using digital holography. To obtain observations of Alternaria spp. spores representative of their airborne stage, we collected events measured in the air during crop harvesting in a contaminated potato field, using a Swisens Poleno device. The classification algorithm used by MeteoSwiss for operational pollen monitoring was extended by training the system using this additional dataset. The quality of the retrieved concentrations is evaluated by comparison with parallel measurements made with a manual Hirst-type trap. Correlations between the two measurements are high, especially over the main dispersion period of Alternaria spp., demonstrating the potential for automatic real-time monitoring of fungal spores., Competing Interests: Conflict of interestThe authors declare that they have no conflict of interest., (© The Author(s) 2023.)
- Published
- 2024
- Full Text
- View/download PDF
39. Machine learning methods for low-cost pollen monitoring - Model optimisation and interpretability.
- Author
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Mills SA, Maya-Manzano JM, Tummon F, MacKenzie AR, and Pope FD
- Abstract
Pollen is a major issue globally, causing as much as 40 % of the population to suffer from hay fever and other allergic conditions. Current techniques for monitoring pollen are either laborious and slow, or expensive, thus alternative methods are needed to provide timely and more localised information on airborne pollen concentrations. We have demonstrated previously that low-cost Optical Particle Counter (OPC) sensors can be used to estimate pollen concentrations when machine learning methods are used to process the data and learn the relationships between OPC output data and conventionally measured pollen concentrations. This study demonstrates how methodical hyperparameter tuning can be employed to significantly improve model performance. We present the results of a range of models based on tuned hyperparameter configurations trained to predict Poaceae (Barnhart), Quercus (L.), Betula (L.), Pinus (L.) and total pollen concentrations. The results achieved here are a significant improvement on results we previously reported: the average R2 scores for the total pollen models have at least doubled compared to using previous parameter settings. Furthermore, we employ the explainable Artificial Intelligence (XAI) technique, SHAP, to interpret the models and understand how each of the input features (i.e. particle sizes) affect the estimated output concentration for each pollen type. In particular, we found that Quercus pollen has a strong positive correlation with particles of optical diameter 1.7-2.3 μm, which distinguishes it from other pollen types such as Poaceae and may suggest that type-specific subpollen particles are present in this size range. There is much further work to be done, especially in training and testing models on data obtained across different environments to evaluate the extent of generalisability. Nevertheless, this work demonstrates the potential this method can offer for low-cost monitoring of pollen and the valuable insight we can gain from what the model has learned., Competing Interests: Declaration of competing interest The authors declare that they have no known competing financial interests or personal relationships that could have appeared to influence the work reported in this paper., (Copyright © 2023 The Authors. Published by Elsevier B.V. All rights reserved.)
- Published
- 2023
- Full Text
- View/download PDF
40. Designing an automatic pollen monitoring network for direct usage of observations to reconstruct the concentration fields.
- Author
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Sofiev M, Buters J, Tummon F, Fatahi Y, Sozinova O, Adams-Groom B, Bergmann KC, Dahl Å, Gehrig R, Gilge S, Seliger AK, Kouznetsov R, Lieberherr G, O'Connor D, Oteros J, Palamarchuk J, Ribeiro H, Werchan B, Werchan M, and Clot B
- Abstract
We consider several approaches to a design of a regional-to-continent-scale automatic pollen monitoring network in Europe. Practical challenges related to the arrangement of such a network limit the range of possible solutions. A hierarchical network is discussed, highlighting the necessity of a few reference sites that follow an extended observations protocol and have corresponding capabilities. Several theoretically rigorous approaches to a network design have been developed so far. However, before starting the process, a network purpose, a criterion of its performance, and a concept of the data usage should be formalized. For atmospheric composition monitoring, developments follow one of the two concepts: a network for direct representation of concentration fields and a network for model-based data assimilation, inverse problem solution, and forecasting. The current paper demonstrates the first approach, whereas the inverse problems are considered in a follow-up paper. We discuss the approaches for the network design from theoretical and practical standpoints, formulate criteria for the network optimality, and consider practical constraints for an automatic pollen network. An application of the methodology is demonstrated for a prominent example of Germany's pollen monitoring network. The multi-step method includes (i) the network representativeness and (ii) redundancy evaluation followed by (iii) fidelity evaluation and improvement using synthetic data., Competing Interests: Declaration of competing interest The authors declare that they have no known competing financial interests or personal relationships that could have appeared to influence the work reported in this paper., (Copyright © 2023 The Authors. Published by Elsevier B.V. All rights reserved.)
- Published
- 2023
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41. Is exposure to pollen a risk factor for moderate and severe asthma exacerbations?
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Annesi-Maesano I, Cecchi L, Biagioni B, Chung KF, Clot B, Collaud Coen M, D'Amato G, Damialis A, Dominguez-Ortega J, Galàn C, Gilles S, Holgate S, Jeebhay M, Kazadzis S, Papadopoulos NG, Quirce S, Sastre J, Tummon F, Traidl-Hoffmann C, Walusiak-Skorupa J, Alonso-Coello P, Canelo-Aybar C, Cantero-Fortiz Y, Rigau D, Salazar J, Verdugo-Paiva F, Jutel M, Akdis CA, and Agache I
- Subjects
- Child, Humans, Adolescent, Infant, Newborn, Allergens analysis, Pollen, Risk Factors, Asthma epidemiology, Asthma etiology, Air Pollution
- Abstract
Limited number of studies have focused on the impact of pollen exposure on asthma. As a part of the EAACI Guidelines on Environment Science, this first systematic review on the relationship of pollen exposure to asthma exacerbations aimed to bridge this knowledge gap in view of implementing recommendations of prevention. We searched electronic iPubMed, Embase, and Web of Science databases using a set of MeSH terms and related synonyms and identified 73 eligible studies that were included for systemic review. When possible, meta-analyses were conducted. Overall meta-analysis suggests that outdoor pollen exposure may have an effect on asthma exacerbation, but caution is needed due to the low number of studies and their heterogeneity. The strongest associations were found between asthma attacks, asthma-related ED admissions or hospitalizations, and an increase in grass pollen concentration in the previous 2-day overall in children aged less than 18 years of age. Tree pollen may increase asthma-related ED visits or admissions lagged up to 7-day overall in individuals younger than 18 years. Rare data show that among subjects under 18 years of age, an exposure to grass pollen lagged up to 3 days may lower lung function. Further research considering effect modifiers of pollen sensitization, hay fever, asthma, air pollution, green spaces, and pre-existing medications is urgently warranted to better evaluate the impacts of pollen on asthma exacerbation. Preventive measures in relation to pollen exposure should be integrated in asthma control as pollen increase continues due to climate change., (© 2023 The Authors. Allergy published by European Academy of Allergy and Clinical Immunology and John Wiley & Sons Ltd.)
- Published
- 2023
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42. Constructing a pollen proxy from low-cost Optical Particle Counter (OPC) data processed with Neural Networks and Random Forests.
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Mills SA, Bousiotis D, Maya-Manzano JM, Tummon F, MacKenzie AR, and Pope FD
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- Neural Networks, Computer, Particulate Matter analysis, Particle Size, Poaceae, Allergens, Environmental Monitoring methods, Random Forest, Pollen chemistry
- Abstract
Pollen allergies affect a significant proportion of the global population, and this is expected to worsen in years to come. There is demand for the development of automated pollen monitoring systems. Low-cost Optical Particle Counters (OPCs) measure particulate matter and have attractive advantages of real-time high time resolution data and affordable costs. This study asks whether low-cost OPC sensors can be used for meaningful monitoring of airborne pollen. We employ a variety of methods, including supervised machine learning techniques, to construct pollen proxies from hourly-average OPC data and evaluate their performance, holding out 40 % of observations to test the proxies. The most successful methods are supervised machine learning Neural Network (NN) and Random Forest (RF) methods, trained from pollen concentrations collected from a Hirst-type sampler. These perform significantly better than using a simple particle size-filtered proxy or a Positive Matrix Factorisation (PMF) source apportionment pollen proxy. Twelve NN and RF models were developed to construct a pollen proxy, each varying by model type, input features and target variable. The results show that such models can construct useful information on pollen from OPC data. The best metrics achieved (Spearman correlation coefficient = 0.85, coefficient of determination = 0.67) were for the NN model constructing a Poaceae (grass) pollen proxy, based on particle size information, temperature, and relative humidity. Ability to distinguish high pollen events was evaluated using F1 Scores, a score reflecting the fraction of true positives with respect to false positives and false negatives, with promising results (F1 ≤ 0.83). Model-constructed proxies demonstrated the ability to follow monthly and diurnal trends in pollen. We discuss the suitability of OPCs for monitoring pollen and offer advice for future progress. We demonstrate an attractive alternative for automated pollen monitoring that could provide valuable and timely information to the benefit of pollen allergy sufferers., Competing Interests: Declaration of competing interest The authors declare that they have no known competing financial interests or personal relationships that could have appeared to influence the work reported in this paper., (Copyright © 2023. Published by Elsevier B.V.)
- Published
- 2023
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43. Towards European automatic bioaerosol monitoring: Comparison of 9 automatic pollen observational instruments with classic Hirst-type traps.
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Maya-Manzano JM, Tummon F, Abt R, Allan N, Bunderson L, Clot B, Crouzy B, Daunys G, Erb S, Gonzalez-Alonso M, Graf E, Grewling Ł, Haus J, Kadantsev E, Kawashima S, Martinez-Bracero M, Matavulj P, Mills S, Niederberger E, Lieberherr G, Lucas RW, O'Connor DJ, Oteros J, Palamarchuk J, Pope FD, Rojo J, Šaulienė I, Schäfer S, Schmidt-Weber CB, Schnitzler M, Šikoparija B, Skjøth CA, Sofiev M, Stemmler T, Triviño M, Zeder Y, and Buters J
- Subjects
- Humans, Environmental Monitoring methods, Pollen, Seasons, Poaceae, Betula, Allergens, Hypersensitivity
- Abstract
To benefit allergy patients and the medical practitioners, pollen information should be available in both a reliable and timely manner; the latter is only recently possible due to automatic monitoring. To evaluate the performance of all currently available automatic instruments, an international intercomparison campaign was jointly organised by the EUMETNET AutoPollen Programme and the ADOPT COST Action in Munich, Germany (March-July 2021). The automatic systems (hardware plus identification algorithms) were compared with manual Hirst-type traps. Measurements were aggregated into 3-hourly or daily values to allow comparison across all devices. We report results for total pollen as well as for Betula, Fraxinus, Poaceae, and Quercus, for all instruments that provided these data. The results for daily averages compared better with Hirst observations than the 3-hourly values. For total pollen, there was a considerable spread among systems, with some reaching R
2 > 0.6 (3 h) and R2 > 0.75 (daily) compared with Hirst-type traps, whilst other systems were not suitable to sample total pollen efficiently (R2 < 0.3). For individual pollen types, results similar to the Hirst were frequently shown by a small group of systems. For Betula, almost all systems performed well (R2 > 0.75 for 9 systems for 3-hourly data). Results for Fraxinus and Quercus were not as good for most systems, while for Poaceae (with some exceptions), the performance was weakest. For all pollen types and for most measurement systems, false positive classifications were observed outside of the main pollen season. Different algorithms applied to the same device also showed different results, highlighting the importance of this aspect of the measurement system. Overall, given the 30 % error on daily concentrations that is currently accepted for Hirst-type traps, several automatic systems are currently capable of being used operationally to provide real-time observations at high temporal resolutions. They provide distinct advantages compared to the manual Hirst-type measurements., Competing Interests: Declaration of Competing Interest The authors declare the following financial interests/personal relationships which may be considered as potential competing interests: Jeroen Buters, Jose M. Maya Manzano, Carsten B. Schmidt-Weber and Marina Triviño report financial support, administrative support, equipment, drugs, or supplies, and travel were provided by Bayerisches Landesamt für Gesundheit und Lebensmittelsicherheit (LGL) and EUMETNET. Carsten Skjoth reports financial support, administrative support, article publishing charges, equipment, drugs, or supplies, and travel were provided by COST Action CA18226 ADOPT – New approaches in detection of pathogens and aeroallergens. Bernard Clot and Fiona Tummon report financial support, administrative support, article publishing charges, equipment, drugs, or supplies, and travel were provided by European Meteorological Society and the EUMETNET AutoPollen Programme. Branko Sikoparija and Predrag Matavulj report financial support, administrative support, article publishing charges, equipment, drugs, or supplies, and travel were provided by BREATHE project from the Science Fund of the Republic of Serbia PROMIS program, under grant agreement no. 6039613 and by the Ministry of Education, Science and Technological Development of the Republic of Serbia (grant agreement number 451–03-68/2022–14/200358). Evgeny Kadantsev and Julia Palamarchuk report financial support, administrative support, article publishing charges, equipment, drugs, or supplies, and travel were provided by Academy of Finland PS4A (grant 318,194). Mikhail Sofiev reports financial support, administrative support, article publishing charges, equipment, drugs, or supplies, and travel were provided by Academy of Finland project ALL-Impress (grant 329,215). Mikhail Sofiev reports financial support, administrative support, article publishing charges, equipment, drugs, or supplies, and travel were provided by European Social Fund (project no. 09.3.3-LMT-K-712-01-0066) and Research Council of Lithuania (LMTLT). Nathan Allan, Landon Bunderson, Richard W. Lucas (Pollen science TM), Jorg Haus, Stefan Schaefer, Martin Schnitzler and Tom Stemmler (Helmut Hund Wetzlar), Reto Abt, Elias Graf, Erny Niederberger and Yanick Zeder (Swisens AG) report a relationship with Pollen science TM, Helmut Hund Wetzlar and Swisens AG respectively, that includes: board membership, employment, and travel reimbursement. The investigations were carried out in compliance with good scientific practices and the support provided by these companies in terms of instrumentation had no effect on the results presented., (Copyright © 2023 Elsevier B.V. All rights reserved.)- Published
- 2023
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44. Alternaria spore exposure in Bavaria, Germany, measured using artificial intelligence algorithms in a network of BAA500 automatic pollen monitors.
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González-Alonso M, Boldeanu M, Koritnik T, Gonçalves J, Belzner L, Stemmler T, Gebauer R, Grewling Ł, Tummon F, Maya-Manzano JM, Ariño AH, Schmidt-Weber C, and Buters J
- Subjects
- Spores, Fungal, Pollen, Allergens, Algorithms, Alternaria, Artificial Intelligence
- Abstract
Although Alternaria spores are well-known allergenic fungal spores, automatic bioaerosol recognition systems have not been trained to recognize these particles until now. Here we report the development of a new algorithm able to classify Alternaria spores with BAA500 automatic bioaerosol monitors. The best validation score was obtained when the model was trained on both data from the original dataset and artificially generated images, with a validation unweighted mean Intersection over Union (IoU), also called Jaccard Index, of 0.95. Data augmentation techniques were applied to the training set. While some particles were not recognized (false negatives), false positives were few. The results correlated well with manual counts (mean of four Hirst-type traps), with R
2 = 0.78. Counts from BAA500 were 1.92 times lower than with Hirst-type traps. The algorithm was then used to re-analyze the historical automatic pollen monitoring network (ePIN) dataset (2018-2022), which lacked Alternaria spore counts. Re-analysis of past data showed that Alternaria spore exposure in Bavaria was very variable, with the highest counts in the North (Marktheidenfeld, 154 m a.s.l.), and the lowest values close to the mountains in the South (Garmisch-Partenkirchen, 735 m a.s.l.). This approach shows that in our network future algorithms can be run on past datasets. Over time, the use of different algorithms could lead to misinterpretations as stemming from climate change or other phenological causes. Our approach enables consistent, homogeneous treatment of long-term series, thus preventing variability in particle counts owing to changes in the algorithms., Competing Interests: Declaration of competing interest The authors report no conflict of interest. Tom Stemmler is currently working at Helmut Hund Gmbh., however this had no effect on the results presented as the investigations were carried out in compliance with good scientific practices., (Copyright © 2022 Elsevier B.V. All rights reserved.)- Published
- 2023
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45. The need for Pan-European automatic pollen and fungal spore monitoring: A stakeholder workshop position paper.
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Tummon F, Arboledas LA, Bonini M, Guinot B, Hicke M, Jacob C, Kendrovski V, McCairns W, Petermann E, Peuch VH, Pfaar O, Sicard M, Sikoparija B, and Clot B
- Abstract
Background: Information about airborne pollen concentrations is required by a range of end users, particularly from the health sector who use both observations and forecasts to diagnose and treat allergic patients. Manual methods are the standard for such measurements but, despite the range of pollen taxa that can be identified, these techniques suffer from a range of drawbacks. This includes being available at low temporal resolution (usually daily averages) and with a delay (usually 3-9 days from the measurement). Recent technological developments have made possible automatic pollen measurements, which are available at high temporal resolution and in real time, although currently only scattered in a few locations across Europe., Materials & Methods: To promote the development of an extensive network across Europe and to ensure that this network will respond to end user needs, a stakeholder workshop was organised under the auspices of the EUMETNET AutoPollen Programme. Participants discussed requirements for the groups they represented, ranging from the need for information at various spatial scales, at high temporal resolution, and for targeted services to be developed., Results: The provision of real-time information is likely to lead to a notable decrease in the direct and indirect health costs associated with allergy in Europe, currently estimated between €50-150 billion/year.
1 DISCUSSION & CONCLUSION: A European measurement network to meet end user requirements would thus more than pay for itself in terms of potential annual savings and provide significant impetus to research across a range of disciplines from climate science and public health to agriculture and environmental management., (© 2021 The Authors. Clinical and Translational Allergy published by John Wiley and Sons Ltd on behalf of European Academy of Allergy and Clinical Immunology.)- Published
- 2021
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46. Tropospheric ozone in CCMI models and Gaussian process emulation to understand biases in the SOCOLv3 chemistry-climate model.
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Revell LE, Stenke A, Tummon F, Feinberg A, Rozanov E, Peter T, Abraham NL, Akiyoshi H, Archibald AT, Butchart N, Deushi M, Jöckel P, Kinnison D, Michou M, Morgenstern O, O'Connor FM, Oman LD, Pitari G, Plummer DA, Schofield R, Stone K, Tilmes S, Visioni D, Yamashita Y, and Zeng G
- Abstract
Previous multi-model intercomparisons have shown that chemistry-climate models exhibit significant biases in tropospheric ozone compared with observations. We investigate annual-mean tropospheric column ozone in 15 models participating in the SPARC/IGAC (Stratosphere-troposphere Processes and their Role in Climate/International Global Atmospheric Chemistry) Chemistry-Climate Model Initiative (CCMI). These models exhibit a positive bias, on average, of up to 40-50% in the Northern Hemisphere compared with observations derived from the Ozone Monitoring Instrument and Microwave Limb Sounder (OMI/MLS), and a negative bias of up to ~30% in the Southern Hemisphere. SOCOLv3.0 (version 3 of the Solar-Climate Ozone Links CCM), which participated in CCMI, simulates global-mean tropospheric ozone columns of 40.2 DU - approximately 33% larger than the CCMI multi-model mean. Here we introduce an updated version of SOCOLv3.0, "SOCOLv3.1", which includes an improved treatment of ozone sink processes, and results in a reduction in the tropospheric column ozone bias of up to 8 DU, mostly due to the inclusion of N
2 O5 hydrolysis on tropospheric aerosols. As a result of these developments, tropospheric column ozone amounts simulated by SOCOLv3.1 are comparable with several other CCMI models. We apply Gaussian process emulation and sensitivity analysis to understand the remaining ozone bias in SOCOLv3.1. This shows that ozone precursors (nitrogen oxides (NOx ), carbon monoxide, methane and other volatile organic compounds) are responsible for more than 90% of the variance in tropospheric ozone. However, it may not be the emissions inventories themselves that result in the bias, but how the emissions are handled in SOCOLv3.1, and we discuss this in the wider context of the other CCMI models. Given that the emissions data set to be used for phase6 of the Coupled Model Intercomparison Project includes approximately 20% more NOx than the data set used for CCMI, further work is urgently needed to address the challenges of simulating sub-grid processes of importance to tropospheric ozone in the current generation of chemistry-climate models.- Published
- 2018
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47. Deriving Global OH Abundance and Atmospheric Lifetimes for Long-Lived Gases: A Search for CH 3 CCl 3 Alternatives.
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Liang Q, Chipperfield MP, Fleming EL, Abraham NL, Braesicke P, Burkholder JB, Daniel JS, Dhomse S, Fraser PJ, Hardiman SC, Jackman CH, Kinnison DE, Krummel PB, Montzka SA, Morgenstern O, McCulloch A, Mühle J, Newman PA, Orkin VL, Pitari G, Prinn RG, Rigby M, Rozanov E, Stenke A, Tummon F, Velders GJM, Visioni D, and Weiss RF
- 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 (CH
3 CCl3 ) (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 (CH2 F2 ), HFC-134a (CH2 FCF3 , HFC-152a (CH3 CHF2 ), 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
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