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
Cattaneo F
(2014)
ON LARGE-SCALE DYNAMO ACTION AT HIGH MAGNETIC REYNOLDS NUMBER
in The Astrophysical Journal
Welsh S
(2014)
Compressible Taylor-Couette flow - instability mechanism and codimension 3 points
in Journal of Fluid Mechanics
Teed R
(2014)
The dynamics and excitation of torsional waves in geodynamo simulations
in Geophysical Journal International
Pittard J
(2016)
Numerical simulations of a shock-filament interaction
in Monthly Notices of the Royal Astronomical Society
Wareing C
(2016)
Magnetohydrodynamical simulation of the formation of clumps and filaments in quiescent diffuse medium by thermal instability
in Monthly Notices of the Royal Astronomical Society
Hughes DW
(2016)
Strong-field dynamo action in rapidly rotating convection with no inertia.
in Physical review. E
Barker A
(2016)
Non-linear tides in a homogeneous rotating planet or star: global simulations of the elliptical instability
in Monthly Notices of the Royal Astronomical Society
Burge C
(2016)
Ambipolar diffusion regulated collapse of filaments threaded by perpendicular magnetic fields
in Astronomy & Astrophysics
Kondic T
(2016)
THE DECAY OF A WEAK LARGE-SCALE MAGNETIC FIELD IN TWO-DIMENSIONAL TURBULENCE
in The Astrophysical Journal
Pittard J
(2016)
The turbulent destruction of clouds - III. Three-dimensional adiabatic shock-cloud simulations
in Monthly Notices of the Royal Astronomical Society
| 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 |