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
Aluzas R
(2012)
Numerical simulations of shocks encountering clumpy regions Simulations of shocks encountering clumpy regions
in Monthly Notices of the Royal Astronomical Society
Arber T
(2009)
THERMAL FRONTS IN FLARING MAGNETIC LOOPS
in The Astrophysical Journal
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
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
Barkov M
(2010)
Close binary progenitors of gamma-ray bursts
in Monthly Notices of the Royal Astronomical Society
Botha G
(2010)
Thermal conduction effects on the kink instability in coronal loops
in Astronomy & Astrophysics
Botha G
(2011)
CHROMOSPHERIC RESONANCES ABOVE SUNSPOT UMBRAE
in The Astrophysical Journal
Botha G
(2012)
OBSERVATIONAL SIGNATURES OF THE CORONAL KINK INSTABILITY WITH THERMAL CONDUCTION
in The Astrophysical Journal
Bowker J
(2014)
Incorporating velocity shear into the magneto-Boussinesq approximation
in Geophysical & Astrophysical Fluid Dynamics
Burge C
(2016)
Ambipolar diffusion regulated collapse of filaments threaded by perpendicular magnetic fields
in Astronomy & Astrophysics
Bushby P
(2012)
Convectively driven dynamo action in the quiet Sun
in Geophysical & Astrophysical Fluid Dynamics
Calkins M
(2016)
Convection-driven kinematic dynamos at low Rossby and magnetic Prandtl numbers
in Physical Review Fluids
Cattaneo F
(2013)
On the measurement of turbulent magnetic diffusivities: the three-dimensional case
in Journal of Fluid Mechanics
Cattaneo F
(2014)
ON LARGE-SCALE DYNAMO ACTION AT HIGH MAGNETIC REYNOLDS NUMBER
in The Astrophysical Journal
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
Close J
(2017)
Hydrodynamic ablation of protoplanetary discs via supernovae
in Monthly Notices of the Royal Astronomical Society
Dallas V
(2016)
Forcing-dependent dynamics and emergence of helicity in rotating turbulence
in Journal of Fluid Mechanics
Davies C
(2011)
THE MEAN ELECTROMOTIVE FORCE RESULTING FROM MAGNETIC BUOYANCY INSTABILITY
in The Astrophysical Journal
Dritschel D
(2012)
Two-dimensional magnetohydrodynamic turbulence in the small magnetic Prandtl number limit
in Journal of Fluid Mechanics
Falle S
(2017)
The interaction of hydrodynamic shocks with self-gravitating clouds
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
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
Favier B
(2013)
Growth rate degeneracies in kinematic dynamos.
in Physical review. E, Statistical, nonlinear, and soft matter physics
Favier B
(2013)
Kinematic dynamo action in square and hexagonal patterns.
in Physical review. E, Statistical, nonlinear, and soft matter physics
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 |