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
Favier B
(2012)
How can large-scale twisted magnetic structures naturally emerge from buoyancy instabilities? Magnetic structures from buoyancy instability
in Monthly Notices of the Royal Astronomical Society
Hubber D
(2013)
Convergence of AMR and SPH simulations - I. Hydrodynamical resolution and convergence tests
in Monthly Notices of the Royal Astronomical Society
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
Rogers H
(2013)
Feedback from winds and supernovae in massive stellar clusters - I. Hydrodynamics
in Monthly Notices of the Royal Astronomical Society
Pittard J
(2016)
The turbulent destruction of clouds - III. Three-dimensional adiabatic shock-cloud simulations
in Monthly Notices of the Royal Astronomical Society
Barker A
(2012)
Magnetic buoyancy instabilities in the presence of magnetic flux pumping at the base of the solar convection zone Magnetic buoyancy and flux pumping
in Monthly Notices of the Royal Astronomical Society
Close J
(2017)
Hydrodynamic ablation of protoplanetary discs via supernovae
in Monthly Notices of the Royal Astronomical Society
Wareing C
(2017)
Magnetohydrodynamic simulations of mechanical stellar feedback in a sheet-like molecular cloud
in Monthly Notices of the Royal Astronomical Society
Pittard J
(2010)
The turbulent destruction of clouds - II. Mach number dependence, mass-loss rates and tail formation
in Monthly Notices of the Royal Astronomical Society
Goldsmith K
(2016)
The interaction of a magnetohydrodynamical shock with a filament
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 |