The MIRACLE Consortium: Modelling the Universe - From Atomic to Large Scales Structures
Lead Research Organisation:
University College London
Department Name: Physics and Astronomy
Abstract
The MIRACLE High Performance Computing supports high-end computing in astrophysics, covering the following projects: * the optical properties of small molecules; * 3D radiative (magneto)-hydro-dynamical simulations of stellar formation, * stellar structure and evolution; * astrochemical simulations in 3D physical simulations, especially the polymerization of astrophysical dust particles; * catalytic and optical properties of astronomical dust candidates; * 3D spectral line and continuum radiative transfer; * 3D simulations of planetary atmospheres and extra-solar planetary atmospheres and * full hydro-dynamical simulation of the intra-cluster medium.
Organisations
Publications
Ercolano B
(2009)
Gas phase diagnostics of protoplanetary disc extension
in Astronomy & Astrophysics
Royer P
(2010)
PACS and SPIRE spectroscopy of the red supergiant VY CMa
in Astronomy and Astrophysics
Decin L
(2010)
Silicon in the dust formation zone of IRC +10216
in Astronomy and Astrophysics
Bastian N
(2009)
Hierarchical star formation in M33: properties of the star-forming regions
in Astrophysics and Space Science
Ercolano B
(2009)
The effects of spatially distributed ionisation sources on the temperature structure of H ii regions
in Astrophysics and Space Science
Miller S
(2010)
H3+ cooling in planetary atmospheres.
in Faraday discussions
Achilleos N
(2010)
Influence of hot plasma pressure on the global structure of Saturn's magnetodisk
in Geophysical Research Letters
Dubernet M. L.
(2010)
Virtual atomic and molecular data centre
in JOURNAL OF QUANTITATIVE SPECTROSCOPY & RADIATIVE TRANSFER
Tennyson J
(2010)
IUPAC critical evaluation of the rotational-vibrational spectra of water vapor. Part II
in Journal of Quantitative Spectroscopy and Radiative Transfer
Rothman L
(2010)
HITEMP, the high-temperature molecular spectroscopic database
in Journal of Quantitative Spectroscopy and Radiative Transfer