The forgotten role of the ground state in atmospheric photochemistry. This project aims to provide novel solutions to two deficiencies in current atmospheric chemistry models. That is, molecular hydrogen (H2) is underestimated by up to a factor of two, and in polluted areas, HO2 concentrations are underestimated by up to a factor of ten. The project will investigate these solutions and assess their local and global atmospheric impact. By better characterising the atmospheric H2 budget, and the r ....The forgotten role of the ground state in atmospheric photochemistry. This project aims to provide novel solutions to two deficiencies in current atmospheric chemistry models. That is, molecular hydrogen (H2) is underestimated by up to a factor of two, and in polluted areas, HO2 concentrations are underestimated by up to a factor of ten. The project will investigate these solutions and assess their local and global atmospheric impact. By better characterising the atmospheric H2 budget, and the role of ground state reactions in general, the predictive ability of atmospheric models will be improved. This will allow, for example, the outcomes of any change in atmospheric H2 concentration, potentially as part of any future hydrogen economy, to be predicted before they occur. The benefits of this project are global: they allow us to better predict the impact of changes to atmospheric composition – before they occur, and local: Australia’s strengths in physical, theoretical and atmospheric chemistry are reinforced.Read moreRead less
Cause and effect: new mechanisms of particles formation in thunderstorms. This project aims to identify meaningful and specific indicators for predicting particle formation and alteration during thunderstorms. How thunderstorms develop is well-understood. However, identifying meaningful and specific indicators for predicting particle alteration during a thunderstorm is still not clear. This project will practically contribute to the evidence of the impact of air particulates, thereby having dire ....Cause and effect: new mechanisms of particles formation in thunderstorms. This project aims to identify meaningful and specific indicators for predicting particle formation and alteration during thunderstorms. How thunderstorms develop is well-understood. However, identifying meaningful and specific indicators for predicting particle alteration during a thunderstorm is still not clear. This project will practically contribute to the evidence of the impact of air particulates, thereby having direct implications for meteorological, and air pollution policy in Australia and worldwide. This project will allow researchers to understand the impact of these factors on the escalation of the causative effects, and to find a way to prevent unnecessary fatal outcomes.Read moreRead less
Discovery Early Career Researcher Award - Grant ID: DE180101194
Funder
Australian Research Council
Funding Amount
$353,700.00
Summary
A chirped pulse microwave spectrometer for studying atmospheric chemistry. This project aims to construct a microwave spectrometer with a unique molecular source to study atmospheric chemistry. Criegee intermediates formed by the ozonolysis of terpenes are key species in atmospheric chemical processes. Only very recently have small Criegee intermediates been detected by various spectroscopic methods. In this project a purpose-built chirped, pulsed Fourier transform microwave spectrometer will be ....A chirped pulse microwave spectrometer for studying atmospheric chemistry. This project aims to construct a microwave spectrometer with a unique molecular source to study atmospheric chemistry. Criegee intermediates formed by the ozonolysis of terpenes are key species in atmospheric chemical processes. Only very recently have small Criegee intermediates been detected by various spectroscopic methods. In this project a purpose-built chirped, pulsed Fourier transform microwave spectrometer will be coupled with a specialised molecular source that will enable their direct observation and characterisation by rotational spectroscopy. This will allow the structure of these molecules to be determined, which will provide insights into their reaction mechanisms.Read moreRead less
Molecular signatures of complex photodissociation reactions. All energy on earth comes from the sun, either directly (e.g photosynthesis) or indirectly (e.g fossil fuels). Photochemistry is the study of how this light is absorbed and what happens to a molecule afterwards. Despite significant experimental and theoretical advances in the past decade (some in our lab), scientists still cannot predict the outcomes of most photochemical reactions. In this project we will determine the reactivity o ....Molecular signatures of complex photodissociation reactions. All energy on earth comes from the sun, either directly (e.g photosynthesis) or indirectly (e.g fossil fuels). Photochemistry is the study of how this light is absorbed and what happens to a molecule afterwards. Despite significant experimental and theoretical advances in the past decade (some in our lab), scientists still cannot predict the outcomes of most photochemical reactions. In this project we will determine the reactivity of several small, fundamental organic molecules. Not only are these molecules pollutants around our cities, but discovery of how they react in the presence of light will allow us to understand and predict the photochemistry of a much wider range of organic species.Read moreRead less
Reactive Intermediates in Atmospheric and Combustion Chemistry. Reactive intermediates are the key species that determine outcomes of the chemical reaction networks in atmospheric and combustion chemistry. However, most reactive intermediates remain undiscovered. The project aims to discover these intermediates using laser spectroscopy. Current models of atmospheric chemistry cannot account for the carbon balance over forests, nor the formation of secondary organic aerosols. Combustion models st ....Reactive Intermediates in Atmospheric and Combustion Chemistry. Reactive intermediates are the key species that determine outcomes of the chemical reaction networks in atmospheric and combustion chemistry. However, most reactive intermediates remain undiscovered. The project aims to discover these intermediates using laser spectroscopy. Current models of atmospheric chemistry cannot account for the carbon balance over forests, nor the formation of secondary organic aerosols. Combustion models struggle to predict how next-generation fuels burn in modern engines. The successful discovery of these intermediates would allow models to be more accurate and predictive. This will allow scientists, engineers and policy makers to make more informed decisions about atmospheric processes and design more efficient new fuels.Read moreRead less
Formation, photochemistry and fate of gas-phase peroxyl radicals. This project aims to understand how peroxyl radical reactions modulate the composition of air. The gas-phase chemical reactions of organic peroxyl radicals contribute to air quality in clean and polluted environments. However, experimental observations of these reaction intermediates and the complex mechanisms governing their formation and fate are limited. This project will use mass spectrometry and laser-based methods to interro ....Formation, photochemistry and fate of gas-phase peroxyl radicals. This project aims to understand how peroxyl radical reactions modulate the composition of air. The gas-phase chemical reactions of organic peroxyl radicals contribute to air quality in clean and polluted environments. However, experimental observations of these reaction intermediates and the complex mechanisms governing their formation and fate are limited. This project will use mass spectrometry and laser-based methods to interrogate the chemical and photochemical reactions of peroxyl radicals in the gas phase. This project expects to understand the composition and dynamics of the troposphere and inform strategies to improve air quality.Read moreRead less
Vibrational Spectroscopy and Imaging from Interstellar Dust to Life. The outcome of this project will result in a more thorough understanding of the role of water in the atmosphere and in the Greenhouse effect, and will provide information leading to more accurate modelling of Global warming. The results will also lead to new insights into interstellar chemistry, the chemistry of cometary dust and the origins of life.
Sulfuric acid formation from atmospheric sulfur trioxide and disulfur oxide: is one water molecule enough? Sulfate aerosols significantly affect the amount of solar radiation reaching the Earth, influencing the nett energy balance, and mitigating the greenhouse effect. A major source of these aerosols is sulfuric acid. Understanding the sources and formation rates of sulfuric acid production is of considerable importance for global climate models. This project will provide significant insight in ....Sulfuric acid formation from atmospheric sulfur trioxide and disulfur oxide: is one water molecule enough? Sulfate aerosols significantly affect the amount of solar radiation reaching the Earth, influencing the nett energy balance, and mitigating the greenhouse effect. A major source of these aerosols is sulfuric acid. Understanding the sources and formation rates of sulfuric acid production is of considerable importance for global climate models. This project will provide significant insight into the sulfur oxides and their water clusters, relevant to sulfuric acid formation, providing data applicable to the modelling of planetary atmospheres, especially timely for the Venus Express mission, and more importantly, the building of comprehensive climate models.Read moreRead less
New insights into free radical reactivity via gas phase studies of radical anions. Free radicals are known to be critical reactive intermediates in chemical processes ranging from the formation of photochemical smog, through combustion to the onset of age-related diseases. This research increases our understanding of how free radicals react and will thus allow for more accurate prediction, and in some instances greater control, of the outcomes of chemical reactions and their health and environme ....New insights into free radical reactivity via gas phase studies of radical anions. Free radicals are known to be critical reactive intermediates in chemical processes ranging from the formation of photochemical smog, through combustion to the onset of age-related diseases. This research increases our understanding of how free radicals react and will thus allow for more accurate prediction, and in some instances greater control, of the outcomes of chemical reactions and their health and environmental consequences. New instrumental technologies will be developed and young Australian researchers will be trained here, and with collaborators in the USA, in state-of-the-art techniques (particularly in mass spectrometry) that are essential to our emerging technology-based economy.Read moreRead less
Discovery Early Career Researcher Award - Grant ID: DE150100301
Funder
Australian Research Council
Funding Amount
$335,000.00
Summary
Planetary Nitrile Chemistry: Synchrotron Spectroscopic Investigations. Observed in planetary atmospheres such as Saturn's moon Titan, cyanide-based aerosols undergo photolytic processing to generate complex organic material of prebiotic interest. However, dedicated spectroscopic experiments directed at nitrile aerosol analogues have not been performed to date. To bridge this gap, a custom cooling cell at the Australian Synchrotron will be used to investigate condensed-phase nitriles at Titan con ....Planetary Nitrile Chemistry: Synchrotron Spectroscopic Investigations. Observed in planetary atmospheres such as Saturn's moon Titan, cyanide-based aerosols undergo photolytic processing to generate complex organic material of prebiotic interest. However, dedicated spectroscopic experiments directed at nitrile aerosol analogues have not been performed to date. To bridge this gap, a custom cooling cell at the Australian Synchrotron will be used to investigate condensed-phase nitriles at Titan conditions. Laser irradiation of nitrile ice particles will then follow; designed to simulate photochemical processes in the Titan atmosphere. The project aims to use data compiled for nitrile aerosols and their photolytic products to assist in assigning these species to unconfirmed bands within infrared surveys of planetary environments.Read moreRead less