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
Pagano P
(2021)
Modelling of asymmetric nanojets in coronal loops
in Astronomy & Astrophysics
Pagano P
(2018)
Contribution of phase-mixing of Alfvén waves to coronal heating in multi-harmonic loop oscillations
in Astronomy & Astrophysics
Saavedra-Bastidas J
(2024)
Gravitational collapse at low to moderate Mach numbers: The relationship between star formation efficiency and the fraction of mass in the massive object
in Astronomy & Astrophysics
Pagano P
(2020)
Effect of coronal loop structure on wave heating through phase mixing
in Astronomy & Astrophysics
Pagano P
(2019)
MHD simulations of the in situ generation of kink and sausage waves in the solar corona by collision of dense plasma clumps
in Astronomy & Astrophysics
Galbiati M
(2024)
MUSE Analysis of Gas around Galaxies (MAGG) VI. The cool and enriched gas environment of z ? 3 Ly a emitters
in Astronomy & Astrophysics
Maccagni F
(2024)
MHONGOOSE discovery of a gas-rich low surface brightness galaxy in the Dorado group
in Astronomy & Astrophysics
Johnston C
(2021)
A fast multi-dimensional magnetohydrodynamic formulation of the transition region adaptive conduction (TRAC) method
in Astronomy & Astrophysics
MartÃnez-Delgado D
(2023)
Hidden depths in the local Universe: The Stellar Stream Legacy Survey
in Astronomy & Astrophysics
Scholtz J
(2024)
GN-z11: The environment of an active galactic nucleus at z = 10.603 New insights into the most distant Ly a detection
in Astronomy & Astrophysics
Mercier W
(2024)
The COSMOS-Web ring: In-depth characterization of an Einstein ring lensing system at z ~ 2
in Astronomy & Astrophysics
Howson T
(2021)
Magnetic reconnection and the Kelvin-Helmholtz instability in the solar corona
in Astronomy & Astrophysics
Morello G
(2023)
Spitzer thermal phase curve of WASP-121 b
in Astronomy & Astrophysics
Pagano P
(2017)
Contribution of mode-coupling and phase-mixing of Alfvén waves to coronal heating
in Astronomy & Astrophysics
Fenton A
(2024)
The 3D structure of disc-instability protoplanets
in Astronomy & Astrophysics
Prole L
(2024)
Heavy black hole seed formation in high- z atomic cooling halos
in Astronomy & Astrophysics
Witstok J
(2021)
Prospects for observing the low-density cosmic web in Lyman- a emission
in Astronomy & Astrophysics
Andrassy R
(2022)
Dynamics in a stellar convective layer and at its boundary: Comparison of five 3D hydrodynamics codes
in Astronomy & Astrophysics
Pagano P
(2020)
Hydrogen non-equilibrium ionisation effects in coronal mass ejections
in Astronomy & Astrophysics
Horst L
(2021)
Multidimensional low-Mach number time-implicit hydrodynamic simulations of convective helium shell burning in a massive star
in Astronomy & Astrophysics
Bemporad A
(2018)
Measuring the electron temperatures of coronal mass ejections with future space-based multi-channel coronagraphs: a numerical test
in Astronomy & Astrophysics
Hausammann L
(2022)
Continuous Simulation Data Stream: A dynamical timescale-dependent output scheme for simulations
in Astronomy and Computing
Radia M
(2022)
Lessons for adaptive mesh refinement in numerical relativity
in Classical and Quantum Gravity
Adamek J
(2020)
Numerical solutions to Einstein's equations in a shearing-dust universe: a code comparison
in Classical and Quantum Gravity
Hoy C
(2024)
A rapid multi-modal parameter estimation technique for LISA
in Classical and Quantum Gravity
| 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 |