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
Marston JB
(2016)
Generalized Quasilinear Approximation: Application to Zonal Jets.
in Physical review letters
Mizerski K
(2013)
SHORT-WAVELENGTH MAGNETIC BUOYANCY INSTABILITY
in The Astrophysical Journal Supplement Series
Mizerski K
(2012)
Large-scale convective dynamos in a stratified rotating plane layer
in Geophysical & Astrophysical Fluid Dynamics
Mizerski K
(2011)
The effect of stratification and compressibility on anelastic convection in a rotating plane layer
in Geophysical & Astrophysical Fluid Dynamics
Nigro G
(2017)
What is a large-scale dynamo?
in Monthly Notices of the Royal Astronomical Society: Letters
Parkin E
(2011)
SPIRALING OUT OF CONTROL: THREE-DIMENSIONAL HYDRODYNAMICAL MODELING OF THE COLLIDING WINDS IN ? CARINAE
in The Astrophysical Journal
Pascoe D
(2008)
Sausage oscillations in loops with a non-uniform cross-section
in Astronomy & Astrophysics
Pascoe D
(2008)
Sausage oscillations in loops with a non-uniform cross-section
in Astronomy & Astrophysics
Pechhacker R
(2012)
Electron cyclotron maser emission mode coupling to the z-mode on a longitudinal density gradient in the context of solar type III bursts
in Physics of Plasmas
Pechhacker R
(2012)
The effect of electron beam pitch angle and density gradient on solar type III radio bursts
in Physics of Plasmas
Pittard J
(2016)
Numerical simulations of a shock-filament interaction
in Monthly Notices of the Royal Astronomical Society
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
Pittard J
(2010)
The turbulent destruction of interstellar clouds
in Astrophysics and Space Science
Pittard J
(2016)
The turbulent destruction of clouds - III. Three-dimensional adiabatic shock-cloud simulations
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
Pittard J
(2011)
Tails of the unexpected: the interaction of an isothermal shell with a cloud
in Monthly Notices of the Royal Astronomical Society: Letters
Pongkitiwanichakul P
(2016)
SHEAR-DRIVEN DYNAMO WAVES IN THE FULLY NONLINEAR REGIME
in The Astrophysical Journal
Rogers H
(2014)
Feedback from winds and supernovae in massive stellar clusters - II. X-ray emission
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
Schmitz H
(2013)
The effect of initial conditions on the electromagnetic radiation generation in type III solar radio bursts
in Physics of Plasmas
Silvers L
(2009)
DOUBLE-DIFFUSIVE INSTABILITIES OF A SHEAR-GENERATED MAGNETIC LAYER
in The Astrophysical Journal
Sreenivasan B
(2011)
Helicity generation and subcritical behaviour in rapidly rotating dynamos
in Journal of Fluid Mechanics
Teed R
(2012)
On the necessary conditions for bursts of convection within the rapidly rotating cylindrical annulus
in Physics of Fluids
Teed R
(2014)
The dynamics and excitation of torsional waves in geodynamo simulations
in Geophysical Journal International
Threlfall J
(2012)
Nonlinear wave propagation and reconnection at magnetic X-points in the Hall MHD regime
in Astronomy & Astrophysics
| 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 |