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
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
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 |