North African mineral dust sources: New insights from a combined analysis based on 3D dust aerosol distributions, surface winds and ancillary soil parameters

Mineral dust aerosol is a key player in the climate system. Determining dust sources and the spatio-temporal variability of dust emission fluxes is essential for estimating the impact of dust on the atmospheric radiation budget, cloud and precipitation formation processes, the bio-productivity and, ultimately, the carbon cycle. Although much effort has been put into determining dust sources from satellite observations, geo-locating active dust sources is still challenging and uncertainties in space and time are evident. One major source of uncertainty is the lack of clear differentiation between near-source dust aerosol and transported dust aerosol. In order to reduce this uncertainty, we use 3D information on the distribution of dust aerosol suspended in the atmosphere calculated from spectral measurements obtained by the Infrared Atmospheric Sounding Interferometer (IASI) by using the Mineral Aerosols Profiling from Infrared Radiance (MAPIR) algorithm. In addition to standard dust products from satellite observations, which provide 2D information on the horizontal distribution of dust, MAPIR allows for the retrieval of additional information on the vertical distribution of dust plumes. This ultimately enables us to separate between near-source and transported dust plumes. Combined with information on near-surface wind speed and surface properties, low-altitude dust plumes can be assigned to dust emission events and low-altitude transport regimes can be excluded. Consequently, this technique will reduce the uncertainty in automatically geo-locating active dust sources. The findings of our study illustrate the spatio-temporal distribution of North African dust sources based on 9 years of data, allowing for the observation of a full seasonal cycle of dust emissions, differentiating morning and afternoon/evening emissions and providing a first glance at long-term changes. In addition, we compare the results of this new method to the results from Schepanski et al. (2012), who manually identified dust sources from Spinning Enhanced Visible and InfraRed Imager (SEVIRI) red-green-blue (RGB) images. The comparison illustrates that each method has its strengths and weaknesses that must be taken into account when using the results. This study is of particular importance for understanding future environmental changes due to a changing climate. © Author(s) 202

Observing mineral dust in northern Africa, the middle east and Europe: current capabilities and challenges ahead for the development of dust services

Mineral dust produced by wind erosion of arid and semi-arid surfaces is a major component of atmospheric aerosol that affects climate, weather, ecosystems, and socio-economic sectors such as human health, transportation, solar energy, and air quality. Understanding these effects and ultimately improving the resilience of affected countries requires a reliable, dense, and diverse set of dust observations, fundamental for the development and the provision of skillful dust forecasts tailored products. The last decade has seen a notable improvement of dust observational capabilities in terms of considered parameters, geographical coverage, and delivery times, as well as of tailored products of interest to both the scientific community and the various end-users. Given this progress, here we review the current state of observational capabilities including in-situ, ground-based and satellite remote sensing observations, in Northern Africa, the Middle East and Europe for the provision of dust information considering the needs of various users. We also critically discuss observational gaps and related unresolved questions while providing suggestions for overcoming the current limitations. Our review aims to be a milestone for discussing dust observational gaps at a global level to address the needs of users, from research communities to nonscientific stakeholders

Multi-sectoral Impact Assessment of an Extreme African Dust Episode in the Eastern Mediterranean in March 2018

In late March 2018, a large part of the Eastern Mediterranean experienced an extraordinary episode of African dust, one of the most intense in recent years, here referred to as the “Minoan Red” event. The episode mainly affected the Greek island of Crete, where the highest aerosol concentrations over the past 15 yeas were recorded, although impacts were also felt well beyond this core area. Our study fills a gap in dust research by assessing the multi-sectoral impacts of sand and dust storms and their socioeconomic implications. Specifically, we provide a multi-sectoral impact assessment of Crete during the occurrence of this exceptional African dust event. During the day of the occurrence of the maximum dust concentration in Crete, i.e. March 22nd, 2018, we identified impacts on meteorological conditions, agriculture, transport, energy, society (including closing of schools and cancellation of social events), and emergency response systems. As a result, the event led to a 3-fold increase in daily emergency responses compare to previous days associated with urban emergencies and wildfires, a 3.5-fold increase in hospital visits and admissions for Chronic Obstructive Pulmonary Disease (COPD) exacerbations and dyspnoea, a reduction of visibility causing aircraft traffic disruptions (eleven cancellations and seven delays), and a reduction of solar energy production. We estimate the cost of direct and indirect effects of the dust episode, considering the most affected socio-economic sectors (e.g. civil protection, aviation, health and solar energy production), to be between 3.4 and 3.8 million EUR for Crete. Since such desert dust transport episodes are natural, meteorology-driven and thus to a large extent unavoidable, we argue that the efficiency of actions to mitigate dust impacts depends on the accuracy of operational dust forecasting and the implementation of relevant early warning systems for social awareness

Nitrous Oxide Profiling from Infrared Radiances (NOPIR): Algorithm Description, Application to 10 Years of IASI Observations and Quality Assessment

Nitrous oxide (N$_{2}$O) is the third most abundant anthropogenous greenhouse gas (after carbon dioxide and methane), with a long atmospheric lifetime and a continuously increasing concentration due to human activities, making it an important gas to monitor. In this work, we present a new method to retrieve N$_{2}$O concentration profiles (with up to two degrees of freedom) from each cloud-free satellite observation by the Infrared Atmospheric Sounding Interferometer (IASI), using spectral micro-windows in the N$_{2}$O ν$_{3}$ band, the Radiative Transfer for TOVS (RTTOV) tools and the Tikhonov regularization scheme. A time series of ten years (2011–2020) of IASI N$_{2}$O profiles and integrated partial columns has been produced and validated with collocated ground-based Network for the Detection of Atmospheric Composition Change (NDACC) and Total Carbon Column Observing Network (TCCON) data. The importance of consistency in the ancillary data used for the retrieval for generating consistent time series has been demonstrated. The Nitrous Oxide Profiling from Infrared Radiances (NOPIR) N$_{2}$O partial columns are of very good quality, with a positive bias of 1.8 to 4% with respect to the ground-based data, which is less than the sum of uncertainties of the compared values. At high latitudes, the comparisons are a bit worse, due to either a known bias in the ground-based data, or to a higher uncertainty in both ground-based and satellite retrievals

Multi-sectoral impact assessment of an extreme African dust episode in the Eastern Mediterranean in March 2018

In late March 2018, a large part of the Eastern Mediterranean experienced an extraordinary episode of African dust, one of the most intense in recent years, here referred to as the “Minoan Red” event. The episode mainly affected the Greek island of Crete, where the highest aerosol concentrations over the past 15 yeas were recorded, although impacts were also felt well beyond this core area. Our study fills a gap in dust research by assessing the multi-sectoral impacts of sand and dust storms and their socioeconomic implications. Specifically, we provide a multi-sectoral impact assessment of Crete during the occurrence of this exceptional African dust event. During the day of the occurrence of the maximum dust concentration in Crete, i.e. March 22nd, 2018, we identified impacts on meteorological conditions, agriculture, transport, energy, society (including closing of schools and cancellation of social events), and emergency response systems. As a result, the event led to a 3-fold increase in daily emergency responses compare to previous days associated with urban emergencies and wildfires, a 3.5-fold increase in hospital visits and admissions for Chronic Obstructive Pulmonary Disease (COPD) exacerbations and dyspnoea, a reduction of visibility causing aircraft traffic disruptions (eleven cancellations and seven delays), and a reduction of solar energy production. We estimate the cost of direct and indirect effects of the dust episode, considering the most affected socio-economic sectors (e.g. civil protection, aviation, health and solar energy production), to be between 3.4 and 3.8 million EUR for Crete. Since such desert dust transport episodes are natural, meteorology-driven and thus to a large extent unavoidable, we argue that the efficiency of actions to mitigate dust impacts depends on the accuracy of operational dust forecasting and the implementation of relevant early warning systems for social awareness.Thanks are due to FCT/MCTES for the financial support to CESAM (UIDP/50017/2020+UIDB/50017/2020) through national funds, and also to the Icelandic Research Fund for the grant no. 207057-051. Authors S. Kazadzis and P. Kosmopoulos would like to acknowledge the European Commission project EuroGEO e-shape (grant agreement No 820852). Also, International Cooperative for Aerosol Prediction (ICAP) and NASA mission researchers are gratefully for providing aerosol data for this study. Aurelio Tobias was supported by MCIN/AEI/10.13039/501100011033 (grant CEX2018-000794-S). S. Kutuzov acknowledges the Megagrant project (agreement No. 075-15-2021-599, 8.06.2021)

Development, Production and Evaluation of Aerosol Climate Data Records from European Satellite Observations (Aerosol_cci)

Producing a global and comprehensive description of atmospheric aerosols requires integration of ground-based, airborne, satellite and model datasets. Due to its complexity, aerosol monitoring requires the use of several data records with complementary information content. This paper describes the lessons learned while developing and qualifying algorithms to generate aerosol Climate Data Records (CDR) within the European Space Agency (ESA) Aerosol_cci project. An iterative algorithm development and evaluation cycle involving core users is applied. It begins with the application-specific refinement of user requirements, leading to algorithm development, dataset processing and independent validation followed by user evaluation. This cycle is demonstrated for a CDR of total Aerosol Optical Depth (AOD) from two subsequent dual-view radiometers. Specific aspects of its applicability to other aerosol algorithms are illustrated with four complementary aerosol datasets. An important element in the development of aerosol CDRs is the inclusion of several algorithms evaluating the same data to benefit from various solutions to the ill-determined retrieval problem. The iterative approach has produced a 17-year AOD CDR, a 10-year stratospheric extinction profile CDR and a 35-year Absorbing Aerosol Index record. Further evolution cycles have been initiated for complementary datasets to provide insight into aerosol properties (i.e., dust aerosol, aerosol absorption).Peer reviewe

Origine de l'homochiralité de la terre: investigations théoriques et expérimentales

Chirality is the property of objects, including molecules, which are not superimposable on their materialized mirror image. Chiral molecules are omnipresent in living organisms and the constituents of biological macromolecules (proteins and nucleic acids) are chiral. Amino-acids (constituting proteins), ribose and 2-deoxy-ribose (the only chiral constituent of RNA and DNA nucleotides respectively) are furthermore generally present in living organisms only under one of their enantiomeric forms. This is referred to as the homochirality of the living world. The origin of this homochirality is still unexplained, even if many partial scenarios have been proposed in the literature. All scenarios involve the creation of a small enantiomeric excess for certain molecules, amplification of this excess and chirality transfer to other chiral molecules. The origin of homochirality on Earth is closely related to the origin of life, and is currently supposed to have preceded life. As no-one will ever be able to directly observe the phenomena which lead to homochirality, and life, on our planet, the only scientific approach to try and help explain how this occurred is to build scenarios, and test them taking into account all available information on the physical and chemical conditions on the primitive Earth (Earth before life appeared). In our work, we investigated three scenarios related to the origin of homochirality on Earth. One of these scenarios also relates to a very precise step of the origin of life: the selection of beta-d-ribofuranose as component of RNA nucleotides.Enantiomeric excesses (up to 15 %) of alpha-methylated alpha-amino-acids have been detected in meteorites which fell on Earth during the 20th century. No enantiomeric excess is detected for the corresponding alpha-hydroxy-acids in the same meteoritic samples and small (2% at most) or no enantiomeric excesses have been measured for non-methylated alpha-amino-acids. In the first part of our work, we investigated if photolysis by circularly polarized light (CPL) in space could be at the origin of the presence (or absence) of an enantiomeric excess for these compounds. Experiments to reproduce UV-CPL photolysis are difficult to undertake: they require high-energy circularly polarized photons, hence the use of a synchrotron. In our work, we used quantum mechanical calculations to obtain the electronic circular dichroïsm (ECD) spectra of two -methylated -amino-acids, their corresponding alpha-hydroxy-acids and one non-methylated alpha-amino-acid. Differences are observed between these spectra, and we propose a scenario to explain the experimental measurements reported here above: the enantioselective photolysis, in the gas phase at low temperatures (20K at most), of the alpha-amino-acids by UV-CPL with lambda>210 nm. Under these conditions no photolysis of the alpha-hydroxy-acids would occur. This scenario concerns the first step in the origin of homochirality on Earth: the creation of a small enantiomeric excess for some chiral molecules.The second scenario that we investigated relates to the enantiomeric amplification step of the origin of homochirality on Earth, for which the role of the alpha-amino-acid serine has been suggested in the literature. Serine clusters have been observed in the gas phase by mass spectrometry. Among these clusters the octamer has been shown to be a magic number cluster and to have a preference for homochirality. An enantiomeric amplification via cycles of formation and dissociation of the octamer has been suggested. No complete scenario has however been proposed in the literature to explain how this could have occurred on the primitive Earth, but any scenario would most probably include an aqueous phase. We aimed at determining if the homochiral preference of serine octamers also exists in solution and therefore we first investigated if serine octamers exist in solution. For this study, we used nuclear magnetic resonance and infrared spectroscopies, which are well-adapted to the study of molecular assemblies in solution. We were able to demonstrate that most probably serine clusters are not present in solution, and if they are it could only be in extremely low concentration. The scenario suggested in the literature is discussed in the light of our results and of literature data on serine clusters.As last hypothesis, we investigated a possible scenario for the selection of beta-d-ribofuranose as component of RNA nucleotides. The currently known prebiotic synthesis pathways to ribose also lead to the formation of many other carbohydrates, and ribose is only a minor product of these syntheses. Our hypothesis is that beta-d-ribofuranose could have been selected through favorable interactions with alpha-amino-acids already present on the primitive Earth under one enantiomeric form. Indeed, it is plausible that a peptidic world emerged before the presence of RNA and that homochiral alpha-amino-acids were present on Earth when RNA was synthesized. Under this hypothesis, we investigated the role that alpha-l-amino-acids could have played in the selection of alpha-d-ribofuranose as component of RNA nucleotides. This work is related to the last step of the origin of homochirality: chirality transfer. Our scenario was investigated via nuclear magnetic resonance studies of the interaction between alpha-amino-acids and carbohydrates. We were able to show that, in the systems that we studied, when an interaction occurs it is very weak (affinity constant less than 1M−1) and non enantioselective. Our results most probably discard the role that alpha-amino-acids alone could have played in the selection of beta-d-ribofuranose as component of RNA nucleotides, but does not discard the role that peptides could have played in this selection.Doctorat en Sciences de l'ingénieurinfo:eu-repo/semantics/nonPublishe

Origine de l'homochiralité de la terre: investigations théoriques et expérimentales

Chirality is the property of objects, including molecules, which are not superimposable on their materialized mirror image. Chiral molecules are omnipresent in living organisms and the constituents of biological macromolecules (proteins and nucleic acids) are chiral. Amino-acids (constituting proteins), ribose and 2-deoxy-ribose (the only chiral constituent of RNA and DNA nucleotides respectively) are furthermore generally present in living organisms only under one of their enantiomeric forms. This is referred to as the homochirality of the living world. The origin of this homochirality is still unexplained, even if many partial scenarios have been proposed in the literature. All scenarios involve the creation of a small enantiomeric excess for certain molecules, amplification of this excess and chirality transfer to other chiral molecules. The origin of homochirality on Earth is closely related to the origin of life, and is currently supposed to have preceded life. As no-one will ever be able to directly observe the phenomena which lead to homochirality, and life, on our planet, the only scientific approach to try and help explain how this occurred is to build scenarios, and test them taking into account all available information on the physical and chemical conditions on the primitive Earth (Earth before life appeared). In our work, we investigated three scenarios related to the origin of homochirality on Earth. One of these scenarios also relates to a very precise step of the origin of life: the selection of beta-d-ribofuranose as component of RNA nucleotides.Enantiomeric excesses (up to 15 %) of alpha-methylated alpha-amino-acids have been detected in meteorites which fell on Earth during the 20th century. No enantiomeric excess is detected for the corresponding alpha-hydroxy-acids in the same meteoritic samples and small (2% at most) or no enantiomeric excesses have been measured for non-methylated alpha-amino-acids. In the first part of our work, we investigated if photolysis by circularly polarized light (CPL) in space could be at the origin of the presence (or absence) of an enantiomeric excess for these compounds. Experiments to reproduce UV-CPL photolysis are difficult to undertake: they require high-energy circularly polarized photons, hence the use of a synchrotron. In our work, we used quantum mechanical calculations to obtain the electronic circular dichroïsm (ECD) spectra of two -methylated -amino-acids, their corresponding alpha-hydroxy-acids and one non-methylated alpha-amino-acid. Differences are observed between these spectra, and we propose a scenario to explain the experimental measurements reported here above: the enantioselective photolysis, in the gas phase at low temperatures (20K at most), of the alpha-amino-acids by UV-CPL with lambda>210 nm. Under these conditions no photolysis of the alpha-hydroxy-acids would occur. This scenario concerns the first step in the origin of homochirality on Earth: the creation of a small enantiomeric excess for some chiral molecules.The second scenario that we investigated relates to the enantiomeric amplification step of the origin of homochirality on Earth, for which the role of the alpha-amino-acid serine has been suggested in the literature. Serine clusters have been observed in the gas phase by mass spectrometry. Among these clusters the octamer has been shown to be a magic number cluster and to have a preference for homochirality. An enantiomeric amplification via cycles of formation and dissociation of the octamer has been suggested. No complete scenario has however been proposed in the literature to explain how this could have occurred on the primitive Earth, but any scenario would most probably include an aqueous phase. We aimed at determining if the homochiral preference of serine octamers also exists in solution and therefore we first investigated if serine octamers exist in solution. For this study, we used nuclear magnetic resonance and infrared spectroscopies, which are well-adapted to the study of molecular assemblies in solution. We were able to demonstrate that most probably serine clusters are not present in solution, and if they are it could only be in extremely low concentration. The scenario suggested in the literature is discussed in the light of our results and of literature data on serine clusters.As last hypothesis, we investigated a possible scenario for the selection of beta-d-ribofuranose as component of RNA nucleotides. The currently known prebiotic synthesis pathways to ribose also lead to the formation of many other carbohydrates, and ribose is only a minor product of these syntheses. Our hypothesis is that beta-d-ribofuranose could have been selected through favorable interactions with alpha-amino-acids already present on the primitive Earth under one enantiomeric form. Indeed, it is plausible that a peptidic world emerged before the presence of RNA and that homochiral alpha-amino-acids were present on Earth when RNA was synthesized. Under this hypothesis, we investigated the role that alpha-l-amino-acids could have played in the selection of alpha-d-ribofuranose as component of RNA nucleotides. This work is related to the last step of the origin of homochirality: chirality transfer. Our scenario was investigated via nuclear magnetic resonance studies of the interaction between alpha-amino-acids and carbohydrates. We were able to show that, in the systems that we studied, when an interaction occurs it is very weak (affinity constant less than 1M−1) and non enantioselective. Our results most probably discard the role that alpha-amino-acids alone could have played in the selection of beta-d-ribofuranose as component of RNA nucleotides, but does not discard the role that peptides could have played in this selection.Doctorat en Sciences de l'ingénieurinfo:eu-repo/semantics/nonPublishe

An NMR Investigation of Serine Clustering in Solution: Implications for the Origin of Homochirality on Earth

info:eu-repo/semantics/nonPublishe

Etude de l'auto-assemblage des sérines en solutions

info:eu-repo/semantics/nonPublishe