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Your Job: This PhD project focuses on modelling and simulating future gas grids, exploring transformation pathways, and developing cross-sectoral simulation frameworks to support informed decision
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single fluid vortex and a liquid/gas interface in various configurations through theoretical/numerical modelling and stability analyses. The following configurations will be analysed : - a horizontal fluid
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-dimensional atmospheric chemical transport modeling. PREFERRED: Experience using these models together with observations to optimally estimate trace gas sources and sinks (i.e.,inverse modeling). In
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inviting dynamic young scientists, capable of theoretical fracture mechanics and related modeling techniques, to join our team to probe cutting edge issues in fatigue and fracture. Some examples of research
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traditional (hydrothermal quartz, barites etc.) paleo-atmospheric proxies via noble gas and noble gas-nitrogen static mass spectrometry. The main goal of the project is to identify new geological areas as
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of experimental studies of gas-cooled plasma-facing components in fusion technology under the direction of Dr. Minami Yoda. The primary responsibilities of the position will be to reassemble and
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, https://doi.org/10.1016/j.ijhydene.2025.151376 . Mayank Kamboj, Donatella Cirrone, Dmitriy Makarov, Vladimir Molkov, Modelling Radiative Heat Transfer to Closed LH2 Storage and Its Effect on Storage
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Role: Research Associate in Novel Optical Sources Based on Gas-Filled Hollow-Fibers Grade and Salary: Grade 7, £37,694 - £47,389 per annum FTE and working pattern: 1FTE, 35hrs per week, Monday
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design Desirable Qualifications Experience with or interest in gas-phase fragmentation mechanisms and ion chemistry Interest in computational proteomics, spectral library development, or fragmentation
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Identification and classification of coherent flow structures in the plasma of the Sun’s photosphere
of magnetic field production in the Sun is not fully understood, although several models based on dynamo theory have been proposed to describe the characteristic features of the solar magnetic field, such as