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
Barkov M
(2010)
Close binary progenitors of gamma-ray bursts
in Monthly Notices of the Royal Astronomical Society
Van Loo S
(2013)
Sputtering in oblique C-type shocks
in Monthly Notices of the Royal Astronomical Society
Vaidya B
(2013)
The responses of magnetically subcritical cores to shocks
in Monthly Notices of the Royal Astronomical Society
Wareing C
(2018)
A new mechanical stellar wind feedback model for the Rosette Nebula
in Monthly Notices of the Royal Astronomical Society
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
Close J
(2013)
Ram pressure stripping of the hot gaseous haloes of galaxies using the k?? sub-grid turbulence model
in Monthly Notices of the Royal Astronomical Society
Komissarov S
(2010)
Rarefaction acceleration of ultrarelativistic magnetized jets in gamma-ray burst sources Rarefaction acceleration of magnetized GRB jets
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
Falle S
(2017)
The interaction of hydrodynamic shocks with self-gravitating clouds
in Monthly Notices of the Royal Astronomical Society
Hughes D
(2011)
The a-effect in rotating convection: a comparison of numerical simulations
in Monthly Notices of the Royal Astronomical Society: Letters
| 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 |