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SPLASH: An Interactive Visualisation Tool for Smoothed Particle Hydrodynamics Simulations

Published online by Cambridge University Press:  05 March 2013

Daniel J. Price
Daniel J. Price*
Affiliation:
School of Physics, University of Exeter, Exeter EX4 4QL, UK. Email: [email protected]
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Abstract

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This paper presents SPLASH, a publicly available interactive visualisation tool for Smoothed Particle Hydrodynamics (SPH) simulations. Visualisation of SPH data is more complicated than for grid-based codes because the data are defined on a set of irregular points and therefore requires a mapping procedure to a two dimensional pixel array. This means that, in practise, many authors simply produce particle plots which offer a rather crude representation of the simulation output. Here we describe the techniques and algorithms which are utilised in SPLASH in order to provide the user with a fast, interactive and meaningful visualisation of one, two and three dimensional SPH results.

Keywords

hydrodynamicsmethods: numerical
Type
Research Article
Information
Publications of the Astronomical Society of Australia , Volume 24 , Issue 3 , 2007 , pp. 159 - 173
Copyright
Copyright © Astronomical Society of Australia 2007

References

Barnes, D. G., Fluke, C. J., Bourke, P. D. & Parry, O. T., 2006, PASA, 23, 82 CrossRefGoogle Scholar
Bate, M. R., Bonnell, I. A. & Bromm, V., 2003, MNRAS, 339, 577 CrossRefGoogle Scholar
Bate, M. R. B., 1995, PhD thesis, University of Cambridge, Cambridge, UK Google Scholar
Benz, W., Cameron, A. G. W., Press, W. H. & Bowers, R. L., 1990, ApJ, 348, 647 Google Scholar
Dale, J. E. & Davies, M. B., 2006, MNRAS, 366, 1424 Google Scholar
Freitag, M. & Benz, W., 2005, MNRAS, 358, 1133 Google Scholar
Frenk, C. S., et al., 1999, ApJ, 525, 554 CrossRefGoogle Scholar
Hernquist, L. & Katz, N., 1989, ApJS, 70, 419 Google Scholar
Mayer, L., Quinn, T., Wadsley, J. & Stadel, J., 2002, Sci, 298, 1756 CrossRefGoogle Scholar
Monaghan, J. J., 1992, ARA&A, 30, 543 Google Scholar
Monaghan, J. J., 2002, MNRAS, 335, 843 CrossRefGoogle Scholar
Monaghan, J. J., 2005, Rep. Prog. Phys., 68, 1703 CrossRefGoogle Scholar
Price, D. J., 2004, PhD thesis, University of Cambridge, Cambridge, UK, astro-ph/0507472 Google Scholar
Price, D. J. & Monaghan, J. J., 2004, MNRAS, 348, 139 Google Scholar
Price, D. J. & Monaghan, J. J., 2007, MNRAS, 374, 1347 Google Scholar
Price, D. J. & Rosswog, S., 2006, Sci, 312, 719 CrossRefGoogle Scholar
Smith, A. J., Haswell, C. A., Murray, J. R., Truss, M. R. & Foulkes, S. B., 2007, MNRAS, 378, 785 CrossRefGoogle Scholar
Springel, V., 2005, MNRAS, 364, 1105 CrossRefGoogle Scholar
Springel, V. & Hernquist, L., 2002, MNRAS, 333, 649 CrossRefGoogle Scholar