660 postdoctoral-soil-structure-interaction-fem-dynamics Postdoctoral positions in United Kingdom
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—to investigate magnetization dynamics. The goal is to precisely resolve the static and layer specific dynamic modes of topological magnetic textures—like chiral domain walls, skyrmions, hopfions, and more.
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About the role Non-equilibrium expanding flows are generated when shocked gas crosses expansion waves, e.g. at the rear of hypersonic vehicles or in ground-based facilities. The effect
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-scale structures in different regions of space. The key data comes from recent missions (SolarOrbiter, ParkerSolarProbe, BepiColombo) and databases of MagnetosphericMultiScale and Messenger. About You The
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characterise the internal dynamics of neural networks. Topological approach – based on metrics derived from topological data analysis to capture qualitative structural changes in the neural network configuration
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imagination for atomistic structure and dynamics; an interest in fundamental science with real-world applications; and both the initiative to work independently and the skill to collaborate in a
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Department of Chemistry. It is one of five schools in the Faculty of Science and Engineering. The School is an exciting and dynamic environment, home to over 530 undergraduate students, 70 postgraduate taught
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Department of Chemistry. It is one of five schools in the Faculty of Science and Engineering. The School is an exciting and dynamic environment, home to over 530 undergraduate students, 70 postgraduate taught
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About the Role A postdoctoral researcher is being recruited to work with Dr Andrew Winter, as an observational astronomer in a primarily theory-oriented group. The high-level goal is to connect
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developing formalisms for their interpretation (GMC structure, dynamical state, lifetime, formation, evolution), and/or ii) weighing the supermassive black holes lurking at galaxy centres using molecular gas
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developing formalisms for their interpretation (GMC structure, dynamical state, lifetime, formation, evolution), and/or ii) weighing the supermassive black holes lurking at galaxy centres using molecular gas