Parallel computing resources for the UK MHD community
Lead Research Organisation:
University of Leeds
Department Name: Applied Mathematics
Abstract
Abstracts are not currently available in GtR for all funded research. This is normally because the abstract was not required at the time of proposal submission, but may be because it included sensitive information such as personal details.
Organisations
People |
ORCID iD |
| Samuel Falle (Principal Investigator) |
Publications
Close J
(2013)
Ram pressure stripping of the hot gaseous haloes of galaxies using the k?? sub-grid turbulence model
in Monthly Notices of the Royal Astronomical Society
Pittard J
(2013)
Self-sealing shells: blowouts and blisters on the surfaces of leaky wind-blown bubbles and supernova remnants
in Monthly Notices of the Royal Astronomical Society
Schmitz H
(2013)
The effect of initial conditions on the electromagnetic radiation generation in type III solar radio bursts
in Physics of Plasmas
Hubber D
(2013)
Convergence of AMR and SPH simulations - I. Hydrodynamical resolution and convergence tests
in Monthly Notices of the Royal Astronomical Society
Favier B
(2013)
Growth rate degeneracies in kinematic dynamos.
in Physical review. E, Statistical, nonlinear, and soft matter physics
Cattaneo F
(2013)
On the measurement of turbulent magnetic diffusivities: the three-dimensional case
in Journal of Fluid Mechanics
Hughes D
(2013)
The effect of velocity shear on dynamo action due to rotating convection
in Journal of Fluid Mechanics
Rogers H
(2014)
Feedback from winds and supernovae in massive stellar clusters - II. X-ray emission
in Monthly Notices of the Royal Astronomical Society
Bowker J
(2014)
Incorporating velocity shear into the magneto-Boussinesq approximation
in Geophysical & Astrophysical Fluid Dynamics
Cattaneo F
(2014)
ON LARGE-SCALE DYNAMO ACTION AT HIGH MAGNETIC REYNOLDS NUMBER
in The Astrophysical Journal
| Description | The computations carried out with this equipment has shown us how magnetic fields play a crucial role in many astrophysical objects such as stars, accretion discs and galaxies. |
| Exploitation Route | Our work has stimulated others to use many of our computational techniques to study astrophysical magnetic fields. |
| Sectors | Aerospace Defence and Marine Energy Environment |
| Description | The numerical methods that have been developed during the project have been used in and industrial application: safety assessment of liquid carbon dioxide transport. |
| First Year Of Impact | 2012 |
| Sector | Aerospace, Defence and Marine,Energy,Environment |
| Impact Types | Cultural Economic |