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atmospheres. Research areas include hydrodynamic atmospheric escape from rocky exoplanets, nitrogen and sulfur cycling on early Mars and Earth, chemical kinetics of early Earth, Venus, Mars, and analogous
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the formation of planets and planetary systems. His research combines planet formation simulations, the study of dust chemistry, and hydrodynamic modelling of protoplanetary discs to constrain the conditions that
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atmospheres. Research areas include hydrodynamic atmospheric escape from rocky exoplanets, nitrogen and sulfur cycling on early Mars and Earth, chemical kinetics of early Earth, Venus, Mars, and analogous
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of Civil and Mechanical Engineering , section for Fluid Mechanics, Coastal and Maritime Engineering (FVM). The position will play an integral part of the project “SHORE: Simulating coastal HydrOdynamics and
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how the interplay between organisms, hydrodynamics, sediment dynamics and chemistry shapes the estuarine and delta environment in the context of natural and human-induced environmental changes
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candidates will focus on developing integrated hydrodynamic and larval transport models to enhance our understanding of circulation dynamics, water quality, and the potential dispersal routes of bivalve larvae
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astronomy, physics, computer science or equivalent degree Solid background in star and planet formation or small bodies of the solar system Experience in hydrodynamics and/or N-body simulations in the star
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part of the project “SHORE: Simulating coastal HydrOdynamics and particle tRansport procEsses”, financed by the European Research Council. The SHORE project is briefly described below: Beaches
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nonlinear, hydrodynamic, thermodynamic and continuity equations of the neutral gas, the ion and electron energy equations, the O+ continuity equation and ion chemistry, and the neutral wind dynamo. The lower
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hydrodynamic stability analysis that has applications in the study of the development of singularities, the long-time behavior of complex systems, the formation of spatial patterns, the transition between