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
(2013)
Growth rate degeneracies in kinematic dynamos.
in Physical review. E, Statistical, nonlinear, and soft matter physics
Tsiklauri D
(2011)
Heating of solar chromosphere by electromagnetic wave absorption in a plasma slab model
in Physics of Plasmas
Sreenivasan B
(2011)
Helicity generation and subcritical behaviour in rapidly rotating dynamos
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
Close J
(2017)
Hydrodynamic ablation of protoplanetary discs via supernovae
in Monthly Notices of the Royal Astronomical Society
Wareing C
(2017)
Hydrodynamic simulations of mechanical stellar feedback in a molecular cloud formed by thermal instability
in Monthly Notices of the Royal Astronomical Society
Bowker J
(2014)
Incorporating velocity shear into the magneto-Boussinesq approximation
in Geophysical & Astrophysical Fluid Dynamics
Gruszecki M
(2012)
Intensity variations associated with fast sausage modes
in Astronomy & Astrophysics
Hughes D
(2012)
Introduction
in Geophysical & Astrophysical Fluid Dynamics
Favier B
(2013)
Kinematic dynamo action in square and hexagonal patterns.
in Physical review. E, Statistical, nonlinear, and soft matter physics
Mizerski K
(2012)
Large-scale convective dynamos in a stratified rotating plane layer
in Geophysical & Astrophysical Fluid Dynamics
Guervilly C
(2017)
Large-scale-vortex dynamos in planar rotating convection
in Journal of Fluid Mechanics
Komissarov S
(2009)
Magnetic acceleration of ultrarelativistic jets in gamma-ray burst sources
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
Gourgouliatos KN
(2016)
Magnetic field evolution in magnetar crusts through three-dimensional simulations.
in Proceedings of the National Academy of Sciences of the United States of America
Van Loo S
(2012)
Magnetic fields and star formation
in Astronomy & Geophysics
Gruszecki M
(2011)
Magnetoacoustic shock formation near a magnetic null point
in Astronomy & Astrophysics
Wareing C
(2017)
Magnetohydrodynamic simulations of mechanical stellar feedback in a sheet-like molecular cloud
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
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
Threlfall J
(2012)
Nonlinear wave propagation and reconnection at magnetic X-points in the Hall MHD regime
in Astronomy & Astrophysics
Pittard J
(2016)
Numerical simulations of a shock-filament interaction
in Monthly Notices of the Royal Astronomical Society
Aluzas R
(2012)
Numerical simulations of shocks encountering clumpy regions Simulations of shocks encountering clumpy regions
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
Cattaneo F
(2014)
ON LARGE-SCALE DYNAMO ACTION AT HIGH MAGNETIC REYNOLDS NUMBER
in The Astrophysical Journal
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 |