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
Tsiklauri D
(2011)
Heating of solar chromosphere by electromagnetic wave absorption in a plasma slab model
in Physics of Plasmas
Gruszecki M
(2011)
Magnetoacoustic shock formation near a magnetic null point
in Astronomy & Astrophysics
Hughes D
(2011)
The a-effect in rotating convection: a comparison of numerical simulations
in Monthly Notices of the Royal Astronomical Society: Letters
Jones C
(2011)
Planetary Magnetic Fields and Fluid Dynamos
in Annual Review of Fluid Mechanics
Mizerski K
(2011)
The effect of stratification and compressibility on anelastic convection in a rotating plane layer
in Geophysical & Astrophysical Fluid Dynamics
Parkin E
(2011)
SPIRALING OUT OF CONTROL: THREE-DIMENSIONAL HYDRODYNAMICAL MODELING OF THE COLLIDING WINDS IN ? CARINAE
in The Astrophysical Journal
Jones C
(2011)
Anelastic convection-driven dynamo benchmarks
in Icarus
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
Komissarov S
(2011)
3+1 magnetodynamics
in Monthly Notices of the Royal Astronomical Society: Letters
Komissarov S
(2011)
On the origin of variable gamma-ray emission from the Crab nebula Gamma-ray emission from the Crab nebula
in Monthly Notices of the Royal Astronomical Society
Weliwita JA
(2011)
Skew-varicose instability in two-dimensional generalized Swift-Hohenberg equations.
in Physical review. E, Statistical, nonlinear, and soft matter physics
Komissarov S
(2012)
Shock dissipation in magnetically dominated impulsive flows Shock dissipation
in Monthly Notices of the Royal Astronomical Society
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
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
Botha G
(2012)
OBSERVATIONAL SIGNATURES OF THE CORONAL KINK INSTABILITY WITH THERMAL CONDUCTION
in The Astrophysical Journal
Van Loo S
(2012)
Magnetic fields and star formation
in Astronomy & Geophysics
Teed R
(2012)
On the necessary conditions for bursts of convection within the rapidly rotating cylindrical annulus
in Physics of Fluids
Threlfall J
(2012)
Nonlinear wave propagation and reconnection at magnetic X-points in the Hall MHD regime
in Astronomy & Astrophysics
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
Hughes D
(2012)
Introduction
in Geophysical & Astrophysical Fluid Dynamics
Mizerski K
(2012)
Large-scale convective dynamos in a stratified rotating plane layer
in Geophysical & Astrophysical Fluid Dynamics
Gruszecki M
(2012)
Intensity variations associated with fast sausage modes
in Astronomy & Astrophysics
Pechhacker R
(2012)
The effect of electron beam pitch angle and density gradient on solar type III radio bursts
in Physics of Plasmas
Bushby P
(2012)
Convectively driven dynamo action in the quiet Sun
in Geophysical & Astrophysical Fluid Dynamics
Tsiklauri D
(2012)
Three dimensional particle-in-cell simulation of particle acceleration by circularly polarised inertial Alfven waves in a transversely inhomogeneous plasma
in Physics of Plasmas
| 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 |