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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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tightly embedded into an interdisciplinary and inter-institutional network. As a postdoctoral researcher in coupled hydrodynamic-ecological modeling (24 months, 100%), you will fill a central position to
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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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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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journals Excellent command of written and spoken English Proficiency with structured coastal ocean models (e.g., ROMS, GETM, CROCO) Familiarity with the hydrodynamics specific to the Baltic Sea region (also