122 parallel-computing-numerical-methods Postdoctoral research jobs at University of Oxford
Sort by
Refine Your Search
-
the EPSRC and is fixed-term for 1.5 years with the possibility of extension. The role is to lead the development of rotor CFD tools for tidal stream turbines. You will work on the EPSRC-funded programme
-
by ATi/Innovate UK and Rolls Royce and is fixed-term to June 2029. You will join a world‑leading programme advancing experimental and numerical methods to predict the impact performance of composite
-
The post holder will join the Physical Oceanography and Palaeoclimate groups in the Department of Earth Sciences and perform numerical model data analysis relevant to two projects: MEZCAL and
-
of reproducing aerodynamic loads in real time for physical experiments. The project combines numerical modelling, data-driven methods, and laboratory experimentation to advance next-generation real-time hybrid
-
temporal reasoning ultrasound AI tools. Thus, the work will involve both computational methods research and collaborating with clinical domain experts to design and evaluate models in simulated and real
-
responsible for the design and testing of original machine-learning based methods for fetal heart biomarker discovery from the CAIFE image and video dataset. The full-time post is funded by InnoHK and is fixed
-
department in its field, running a globally competitive programme of research and teaching. The Kennedy Institute is a biomedical research centre uniquely bringing together discovery science and early-stage
-
fluorescent microscopy approach undertaken in parallel inthe Uphoff lab. You will be working in a modern laboratory environment for protein purification, microbiology & molecular biology. Central Oxford cryo-EM
-
the lunar farside. The successful candidate will contribute to the development and scientific programme of the Lunar Farside Technosignature and Transients Telescope (LFT3; https://lft3.space). Lunar Farside
-
numerical cosmology. The successful candidate will lead the develop of realistic simulations of a galaxy, lensing, X-ray and CMB secondary observables. This will be built on the backlight simulations, a new