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
Dritschel D
(2012)
Two-dimensional magnetohydrodynamic turbulence in the small magnetic Prandtl number limit
in Journal of Fluid Mechanics
Aluzas R
(2012)
Numerical simulations of shocks encountering clumpy regions Simulations of shocks encountering clumpy regions
in Monthly Notices of the Royal Astronomical Society
Favier B
(2013)
On the problem of large-scale magnetic field generation in rotating compressible convection
in Journal of Fluid Mechanics
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
Cattaneo F
(2013)
On the measurement of turbulent magnetic diffusivities: the three-dimensional case
in Journal of Fluid Mechanics
Favier B
(2013)
Growth rate degeneracies in kinematic dynamos.
in Physical review. E, Statistical, nonlinear, and soft matter physics
Mizerski K
(2013)
SHORT-WAVELENGTH MAGNETIC BUOYANCY INSTABILITY
in The Astrophysical Journal Supplement Series
Hughes D
(2013)
The effect of velocity shear on dynamo action due to rotating convection
in Journal of Fluid Mechanics
Hubber D
(2013)
Convergence of AMR and SPH simulations - I. Hydrodynamical resolution and convergence tests
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
Favier B
(2013)
Kinematic dynamo action in square and hexagonal patterns.
in Physical review. E, Statistical, nonlinear, and soft matter physics
Tobias S
(2013)
On the measurement of the turbulent diffusivity of a large-scale magnetic field
in Journal of Fluid Mechanics
Van Loo S
(2013)
Sputtering in oblique C-type shocks
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
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
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
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
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
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 |