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
Rogers H
(2013)
Feedback from winds and supernovae in massive stellar clusters - I. Hydrodynamics
in Monthly Notices of the Royal Astronomical Society
Tobias SM
(2013)
Shear-driven dynamo waves at high magnetic Reynolds number.
in Nature
Mizerski K
(2013)
SHORT-WAVELENGTH MAGNETIC BUOYANCY INSTABILITY
in The Astrophysical Journal Supplement Series
Tobias S
(2013)
On the measurement of the turbulent diffusivity of a large-scale magnetic field
in Journal of Fluid Mechanics
Favier B
(2013)
On the problem of large-scale magnetic field generation in rotating compressible convection
in Journal of Fluid Mechanics
Tobias SM
(2013)
Direct statistical simulation of out-of-equilibrium jets.
in Physical review letters
Vaidya B
(2013)
The responses of magnetically subcritical cores to shocks
in Monthly Notices of the Royal Astronomical Society
Van Loo S
(2013)
Sputtering in oblique C-type shocks
in Monthly Notices of the Royal Astronomical Society
Favier B
(2013)
Kinematic dynamo action in square and hexagonal patterns.
in Physical review. E, Statistical, nonlinear, and soft matter physics
| 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 |