DiRAC-2.5 - the pathway to DiRAC Phase 3
Lead Research Organisation:
Durham University
Department Name: Physics
Abstract
We request funding to relocate the Blue Wonder HPC cluster and associated storage, currently at the Hartree Centre at Daresbury, to Durham, together with installation and hardware maintenance costs. This move would enable DiRAC to expand the current DiRAC-2 Data centric service, managed by Durham, by a factor of two in both computing power and data storage capacity. The new service would be called the DiRAC-2.5 Data Centric service.
Planned Impact
DiRAC would seek to continue to engage with industry at various levels, from the
provision of computing cycles for industrial applications to the
exchange of technical knowledge and shared training programmes. The
facility will serve to train young scientists in the most advanced
techniques for supercomputing. These have extensive applications beyond
academia, for example in industry and finance. Finally, output from Dirac-based
projects will be used for science outreach activities.
provision of computing cycles for industrial applications to the
exchange of technical knowledge and shared training programmes. The
facility will serve to train young scientists in the most advanced
techniques for supercomputing. These have extensive applications beyond
academia, for example in industry and finance. Finally, output from Dirac-based
projects will be used for science outreach activities.
Organisations
Publications
Givans J
(2022)
Non-linearities in the Lyman-a forest and in its cross-correlation with dark matter halos
in Journal of Cosmology and Astroparticle Physics
Glasscock K
(2024)
Statistical estimation of full-sky radio maps from 21 cm array visibility data using Gaussian constrained realizations
in RAS Techniques and Instruments
Glowacki M
(2021)
The redshift evolution of the baryonic Tully-Fisher relation in SIMBA
in Monthly Notices of the Royal Astronomical Society
Glowacki M
(2021)
The redshift evolution of the baryonic Tully-Fisher relation in SIMBA
in Monthly Notices of the Royal Astronomical Society
Glowacki M
(2022)
ASymba: H i global profile asymmetries in the simba simulation
in Monthly Notices of the Royal Astronomical Society
Glowacki M
(2020)
The redshift evolution of the baryonic Tully-Fisher relation in Simba
Glowacki M
(2020)
The baryonic Tully-Fisher relation in the simba simulation
in Monthly Notices of the Royal Astronomical Society
Glowacki M
(2022)
ASymba: HI global profile asymmetries in the Simba simulation
Glowacki M
(2020)
The baryonic Tully-Fisher relation in the Simba simulation
Goater A
(2024)
EDGE: The direct link between mass growth history and the extended stellar haloes of the faintest dwarf galaxies
in Monthly Notices of the Royal Astronomical Society
Goldstraw E
(2018)
Comparison of methods for modelling coronal magnetic fields
in Astronomy & Astrophysics
Gonzalez-Perez V
(2020)
Do model emission line galaxies live in filaments at z ~ 1?
in Monthly Notices of the Royal Astronomical Society
Gonzalez-Perez V
(2017)
The host dark matter haloes of [O II] emitters at 0.5 < z < 1.5
in Monthly Notices of the Royal Astronomical Society
Gonzalez-Perez V
(2020)
Do model emission line galaxies live in filaments at z~1?
Gonzalo T
(2024)
PEANUTS: a software for the automatic computation of solar neutrino flux and its propagation within Earth
in The European Physical Journal C
Gourgouliatos K
(2020)
Nonaxisymmetric Hall instability: A key to understanding magnetars
Gourgouliatos K
(2019)
Nonaxisymmetric Hall instability: A key to understanding magnetars
in Physical Review Research
Grand R
(2018)
Aurigaia: mock Gaia DR2 stellar catalogues from the auriga cosmological simulations
in Monthly Notices of the Royal Astronomical Society
Grand R
(2021)
Determining the full satellite population of a Milky Way-mass halo in a highly resolved cosmological hydrodynamic simulation
in Monthly Notices of the Royal Astronomical Society
Grand R
(2024)
Overview and public data release of the augmented Auriga Project: cosmological simulations of dwarf and Milky Way-mass galaxies
in Monthly Notices of the Royal Astronomical Society
Granelli A
(2023)
ULYSSES, universal LeptogeneSiS equation solver: Version 2
in Computer Physics Communications
Granelli A
(2023)
ULYSSES, Universal LeptogeneSiS Equation Solver: version 2
Gray A
(2021)
Uncertainty Propagation in SINBAD Fusion Benchmarks with Total Monte Carlo and Imprecise Probabilities
in Fusion Science and Technology
Grove C
(2022)
The DESI N -body simulation project - I. Testing the robustness of simulations for the DESI dark time survey
in Monthly Notices of the Royal Astronomical Society
| Description | See Dirac annual report https://dirac.ac.uk |
| Exploitation Route | See Dirac annual report https://dirac.ac.uk |
| Sectors | Digital/Communication/Information Technologies (including Software) Education |
| URL | https://dirac.ac.uk |