SPLASH: An Interactive Visualisation Tool for Smoothed Particle Hydrodynamics Simulations. 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.

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  1. Holmes, David W.; Pivonka, Peter: Novel pressure inlet and outlet boundary conditions for smoothed particle hydrodynamics, applied to real problems in porous media flow (2021)
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  3. David A. Hubber, Giovanni P. Rosotti, Richard A. Booth: GANDALF - Graphical Astrophysics code for N-body Dynamics And Lagrangian Fluids (2017) arXiv
  4. Duan, Guangtao; Chen, Bin: Large eddy simulation by particle method coupled with sub-particle-scale model and application to mixing layer flow (2015)
  5. Stasyszyn, Federico A.; Elstner, Detlef: A vector potential implementation for smoothed particle magnetohydrodynamics (2015)
  6. Adami, S.; Hu, X. Y.; Adams, N. A.: A transport-velocity formulation for smoothed particle hydrodynamics (2013)
  7. Price, Daniel J.: Smoothed particle hydrodynamics and magnetohydrodynamics (2012)
  8. Corrigan, Andrew; Wallin, John; Vesenjak, Matej: Visualization of meshless simulations using Fourier volume rendering (2009)
  9. Lorén-Aguilar, P.; Isern, J.; García-Berro, E.: High-resolution smoothed particle hydrodynamics simulations of the merger of binary white dwarfs (2009)
  10. Vanaverbeke, S.; Keppens, R.; Poedts, S.; Boffin, H.: GRADSPH: A parallel smoothed particle hydrodynamics code for self-gravitating astrophysical fluid dynamics (2009)
  11. Price, Daniel J.: Modelling discontinuities and Kelvin-Helmholtz instabilities in SPH (2008)