Dr Andrei Igoshev
Dr Toby Wood
| A connection between proto-neutron star Tayler-Spruit dynamos and low-field magnetars | 2025 |
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Dr Craig Duguid
Professor Paul Bushby
Dr Toby Wood
| Shear-driven magnetic buoyancy in the solar tachocline: Dependence of the mean electromotive force on diffusivity and latitude | 2024 |
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Scott Hopper
Dr Toby Wood
Professor Paul Bushby
| Stratified Resistive Tearing Instability | 2024 |
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Dr Gary Liu
Dr Andrew Baggaley
Professor Carlo Barenghi
Dr Toby Wood
| Vortex Depinning in a Two-Dimensional Superfluid | 2024 |
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Dr John Moss
Dr Toby Wood
Professor Paul Bushby
| Self-adjointness of sound-proof models for magnetic buoyancy | 2023 |
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Dr Craig Duguid
Professor Paul Bushby
Dr Toby Wood
| Shear-driven magnetic buoyancy in the solar tachocline: The mean electromotive force due to rotation | 2023 |
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Dr Andrew Snodin
Dr Toby Wood
| A hybrid pseudo-incompressible–hydrostatic model | 2022 |
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Jordan Day
Dr Elizabeth Heidrich
Dr Toby Wood
| A scalable model of fluid flow, substrate removal and current production in microbial fuel cells | 2022 |
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Professor Jenny Read
Dr Christos Kaspiris-Rousellis
Dr Toby Wood
| Seeing the future: Predictive control in neural models of ocular accommodation | 2022 |
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Dr Toby Wood
| Superconducting Phases in Neutron Star Cores | 2022 |
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Dr Toby Wood
| Three-dimensional Magnetothermal Simulations of Magnetar Outbursts | 2022 |
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Dr John Moss
Dr Toby Wood
Professor Paul Bushby
| Validity of sound-proof approximations for magnetic buoyancy | 2022 |
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Dr Andrei Igoshev
Dr Toby Wood
| 3D Magnetothermal Simulations of Tangled Crustal Magnetic Field in Central Compact Objects | 2021 |
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Dr Toby Wood
| Modelling Magnetar Behaviour with 3D Magnetothermal Simulations | 2021 |
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Dr Andrei Igoshev
Dr Toby Wood
| Strong toroidal magnetic fields required by quiescent X-ray emission of magnetars | 2021 |
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Dr Toby Wood
| X-Ray Emission from Isolated Neutron Stars Revisited: 3D Magnetothermal Simulations | 2021 |
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Dr Toby Wood
| 3D modelling of magneto-thermal evolution of neutron stars: method and test cases | 2020 |
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Amit Seta
Professor Paul Bushby
Professor Anvar Shukurov
Dr Toby Wood
| On the saturation mechanism of the fluctuation dynamo at PrM >= 1 | 2020 |
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Dr Toby Wood
Mae Mesgarnezhad
Dr George Stagg
Professor Carlo Barenghi
| Quasiperiodic boundary conditions for three-dimensional superfluids | 2019 |
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Dr Toby Wood
| A self-consistent model of the solar tachocline | 2018 |
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Amit Seta
Professor Anvar Shukurov
Dr Toby Wood
Professor Paul Bushby
Andrew Snodin
et al. | Relative distribution of cosmic rays and magnetic fields | 2018 |
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Professor Anvar Shukurov
Andrew Snodin
Amit Seta
Professor Paul Bushby
Dr Toby Wood
et al. | Cosmic rays in intermittent magnetic fields | 2017 |
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Dr Toby Wood
| Magnetic field evolution in magnetar crusts through three-dimensional simulations | 2016 |
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Dr Toby Wood
Professor Paul Bushby
| Oscillatory convection and limitations of the Boussinesq approximation | 2016 |
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Dr Toby Wood
| Three Dimensional Simulation of the Magnetic Stress in a Neutron Star Crust | 2015 |
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Dr Toby Wood
| Density-shear instability in electron magneto-hydrodynamics | 2014 |
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Dr Toby Wood
| A new model for mixing by double-diffusive convection (semi-convection): II. The transport of heat and composition through layers | 2013 |
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Dr Celine Guervilly
Dr Toby Wood
| Effect of metallic walls on dynamos generated by laminar boundary-driven flow in a spherical domain | 2013 |
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