28 coding-"https:"-"FEMTO-ST"-"CSIC" "https:" "https:" "https:" "https:" "https:" "https:" "Dr" Fellowship positions in Norway
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for Early Career Scientists (FRIPRO) ReCon²: “Resolving the Solar Convective Conundrum: A Full-Physics Approach to Solar Convection” (project period 01.04.2026–01.10.2029) and led by Dr. Andrius Popovas
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/InstituteDepartment of Physics and TechnologyCountryNorwayGeofield Contact State/Province Troms City Tromsø Website https://en.uit.no/startsida Street Hansine Hansens veg 18 Postal Code 9019 STATUS: EXPIRED X (formerly
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Environment. Dr Rosa Cheesman (PROMENTA, University of Oslo) will serve as primary supervisor with overall responsibility for the PhD project. Dr Nicolai Borgen and Prof Astrid Sandsør (Centre for Research
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be embedded in the SCML research group and contribute to its ongoing interdisciplinary work at the intersection of machine learning and life sciences. Dr. Milena Pavlović will serve as a primary
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(NELO), revealing the branchial cavity as an important region of the fish immune system. (https://www.science.org/doi/10.1126/sciadv.adj0101 ) (https://www.frontiersin.org/journals/immunology/articles
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institutions. Position 1 – Origins: Constraining the cosmic infrared background and interplanetary dust emission using multi-generational data, supervised by Dr. Duncan Watts (duncanwa@astro.uio.no ) and Prof
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the interdisciplinary NeuroPathways Convergence Environment. Dr Rosa Cheesman (PROMENTA, University of Oslo) will serve as primary supervisor with overall responsibility for the PhD project. Dr Nicolai Borgen and Prof
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Model) simulations with realistic freshwater fluxes from the Greenland ice sheet. The PhD candidate will be supervised by Dr. Marius Årthun. The PhD candidate will be connected to “Arctic Ocean 2050 ”, a
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learning and life sciences. Dr. Milena Pavlović will serve as a primary supervisor for the project, with professors Anne-Marie George, Pooya Zakeri, and Torbjørn Rognes serving as co-supervisors
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van der Voort and Dr. Reetika Joshi. AEPIC. This project focuses on advancing our hybrid PIC and MHD code to enable fully adaptable and self-consistent simulations of the solar atmosphere and solar