Anomalous isotope effects in atmospheric ozone and carbon dioxide. The anomalous isotopic composition of atmospheric ozone, which has been a puzzle for over twenty years, will be investigated by laboratory and atmospheric measurements. An understanding of the source of this anomaly and its effect on the isotopic composition of other trace atmospheric gases, especially CO2, would provide unique opportunities for constraining the tropospheric and stratospheric ozone budgets and determining the his ....Anomalous isotope effects in atmospheric ozone and carbon dioxide. The anomalous isotopic composition of atmospheric ozone, which has been a puzzle for over twenty years, will be investigated by laboratory and atmospheric measurements. An understanding of the source of this anomaly and its effect on the isotopic composition of other trace atmospheric gases, especially CO2, would provide unique opportunities for constraining the tropospheric and stratospheric ozone budgets and determining the history of a particular air mass. The method of detection will be high resolution FTIR spectroscopy which, in contrast to traditional mass-spectrometric methods, provides information about the position of the heavy atom in an enriched ozone molecule and requires no sample preparation.Read moreRead less
The energetics and dynamics of chemical reactions of polyatomic molecules involving multiple electronic states. This project will produce, from first principles, the first quantitatively accurate computer simulations of chemical reactions which involve several atoms and multiple electronic states. Many of the most important chemical reactions in the atmosphere (and elsewhere) involve changing both the shape of the molecules and their electronic structure. Many of these reactions are difficult to ....The energetics and dynamics of chemical reactions of polyatomic molecules involving multiple electronic states. This project will produce, from first principles, the first quantitatively accurate computer simulations of chemical reactions which involve several atoms and multiple electronic states. Many of the most important chemical reactions in the atmosphere (and elsewhere) involve changing both the shape of the molecules and their electronic structure. Many of these reactions are difficult to study in the laboratory, and consequently computer simulation is an essential component of the study of such reactions. U nderstanding how these reactions occur, and how fast they proceed, are important to our understanding of the dynamics of the atmosphere and other large scale reactors.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
Isotopic fractionation in planetary atmospheres. Ongoing changes in the Earth's atmosphere, such as ozone depletion, demonstrate the need to understand atmospheric photochemical processes. Isotopic fractionation is one vehicle for obtaining
detailed insight into these processes. The proposed research will
increase our understanding of fundamental molecular processes and use these new results to improve our knowledge of isotopic fractionation in planetary atmospheres. The resulting models wil ....Isotopic fractionation in planetary atmospheres. Ongoing changes in the Earth's atmosphere, such as ozone depletion, demonstrate the need to understand atmospheric photochemical processes. Isotopic fractionation is one vehicle for obtaining
detailed insight into these processes. The proposed research will
increase our understanding of fundamental molecular processes and use these new results to improve our knowledge of isotopic fractionation in planetary atmospheres. The resulting models will lead to new insight into the Earth's ozone chemistry and the recent evolution of Titan's and Venus' atmospheres, including how much water may have been present on Venus in the recent past. The research program also enables Australian participation in three international spacecraft
missions.
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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.
Photochemistry of the Middle Atmospheres of Venus and the Earth. Ongoing changes in the Earth's atmosphere, such as ozone depletion, demonstrate the need to understand the processes that control atmospheric chemistry. The proposed research will improve the fidelity of photochemical models, provide additional insight into the recent evolution of the Venus atmosphere, and examine how atmospheric chemistry and climate change interact(ed) on Venus. This research will improve our understanding of l ....Photochemistry of the Middle Atmospheres of Venus and the Earth. Ongoing changes in the Earth's atmosphere, such as ozone depletion, demonstrate the need to understand the processes that control atmospheric chemistry. The proposed research will improve the fidelity of photochemical models, provide additional insight into the recent evolution of the Venus atmosphere, and examine how atmospheric chemistry and climate change interact(ed) on Venus. This research will improve our understanding of long-standing issues, such as how much water might have been present on Venus in the recent past. The research program will provide an opportunity for Australian science to participate in at least one spacecraft mission to Venus. Read moreRead less
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
Quantum Mechanics and Planetary Atmospheres. The project will increase the visibility and status of Australian research, by the participation of researchers and students in a wide international collaboration, covering experiments, theory, and computation, which will solve a fundamental research problem that has previously defied understanding. The resulting nitrogen model will be relevant to the important fields of global and planetary atmospheric change, and will find immediate application in t ....Quantum Mechanics and Planetary Atmospheres. The project will increase the visibility and status of Australian research, by the participation of researchers and students in a wide international collaboration, covering experiments, theory, and computation, which will solve a fundamental research problem that has previously defied understanding. The resulting nitrogen model will be relevant to the important fields of global and planetary atmospheric change, and will find immediate application in the analysis of results from the NASA missions, Voyager, Cassini, and (later) New Horizons. In the experimental part of the project, an Australian-first extreme-ultraviolet laser facility will be developed which will provide research opportunities complementary to the Australian Synchrotron.Read moreRead less
Understanding the chemistry and evolution of planets and their atmospheres: Integrating experiments, observations, and quantum mechanical models. Ongoing changes in the Earth's atmosphere, demonstrate the need to understand photochemical processes and their role in atmospheric evolution. The proposed research will increase our understanding of the evolution of planetary atmospheres, with concomitant insight into the Earth's evolution. This proposal will greatly enhance the visibility of Australi ....Understanding the chemistry and evolution of planets and their atmospheres: Integrating experiments, observations, and quantum mechanical models. Ongoing changes in the Earth's atmosphere, demonstrate the need to understand photochemical processes and their role in atmospheric evolution. The proposed research will increase our understanding of the evolution of planetary atmospheres, with concomitant insight into the Earth's evolution. This proposal will greatly enhance the visibility of Australian research, through formal, direct connections to NASA and ESA (European Space Agency) planetary exploration missions, along with publications in Nature, Science, and/or PNAS (Proceedings of the National Academy of Sciences) that will likely result from the high-profile problems to be studied. Furthermore, as a result of this collaboration, Australian students and postdoctoral researchers will benefit from interactions with top international scientists.Read moreRead less