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
Tobias S
(2013)
On the measurement of the turbulent diffusivity of a large-scale magnetic field
in Journal of Fluid Mechanics
Dallas V
(2016)
Forcing-dependent dynamics and emergence of helicity in rotating turbulence
in Journal of Fluid Mechanics
Welsh S
(2014)
Compressible Taylor-Couette flow - instability mechanism and codimension 3 points
in Journal of Fluid Mechanics
Dritschel D
(2012)
Two-dimensional magnetohydrodynamic turbulence in the small magnetic Prandtl number limit
in Journal of Fluid Mechanics
Vetrov A. A.
(2009)
Comparing thermal and electrical methods for controlling the wavelength of semiconductor-laser radiation
in JOURNAL OF OPTICAL TECHNOLOGY
Komissarov Serguei S.
(2009)
Blandford-Znajek Mechanism versus Penrose Process
in JOURNAL OF THE KOREAN PHYSICAL SOCIETY
Pittard J
(2016)
Numerical simulations of a shock-filament interaction
in Monthly Notices of the Royal Astronomical Society
Komissarov S
(2012)
Shock dissipation in magnetically dominated impulsive flows Shock dissipation
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
Komissarov S
(2009)
Activation of the Blandford-Znajek mechanism in collapsing stars
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
Goldsmith K
(2017)
A comparison of shock-cloud and wind-cloud interactions: the longer survival of clouds in winds
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
Komissarov S
(2009)
Magnetic acceleration of ultrarelativistic jets in gamma-ray burst sources
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
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
Hubber D
(2013)
Convergence of AMR and SPH simulations - I. Hydrodynamical resolution and convergence tests
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
Rogers H
(2013)
Feedback from winds and supernovae in massive stellar clusters - I. Hydrodynamics
in Monthly Notices of the Royal Astronomical Society
Pittard J
(2016)
The turbulent destruction of clouds - III. Three-dimensional adiabatic shock-cloud simulations
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
Close J
(2017)
Hydrodynamic ablation of protoplanetary discs via supernovae
in Monthly Notices of the Royal Astronomical Society
Wareing C
(2017)
Magnetohydrodynamic simulations of mechanical stellar feedback in a sheet-like molecular cloud
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
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 |