OpenSPH

Screenshots

See also the render gallery.

About

OpenSPH is a library and a GUI application for hydrodynamic and N-body simulations. It uses SPH discretization in space and currently is specialized for simulations of asteroid impacts. The code is being developed on Astronomical Institute of Charles University. It aims to provide a fast, versatile and easily extensible SPH solver utilizing modern CPU features (SSE/AVX instruction sets).

Quick start

Windows

OpenSPH can be easily installed using the MSI installer.

Debian and Ubuntu

The latest version can be downloaded as a Debian buster package. Install it via:

sudo dpkg -i opensph_0.4.1-1.deb

The package contains three executables:

• opensph - main program with graphical interface
• opensph-cli - command-line utility allowing to run simulations set up by opensph
• opensph-info - command-line utility for quick inspection of metadata of OpenSPH output files

Arch Linux

OpenSPH package can be build from AUR, using e.g. trizen:

trizen -S opensph

FreeBSD

The code is in the FreeBSD ports collection (big thanks to Yuri) and can be installed using:

pkg install OpenSPH

Getting the source code

The code can be downloaded from GitLab repository. Using git, you can clone the code with

git clone https://gitlab.com/sevecekp/sph.git
cd sph

To get the latest (experimental) version, switch to develomnent branch using

git checkout devel

Compilation

The code uses many c++14 features, so a reasonably new version of a C++ compiler is necessary. The compilation has been tested on gcc 6.3.1 and clang 4.0.0. Prerequisities of the code are:

• git (to get the code from the repository, skip if you already have the code)
• up-to-date version of gcc or clang compiler
• wxWidgets, needed for graphical interface of the code
• cmake (version >= 3.5)

Another optional dependencies of the code are:

• Intel Threading Building Blocks (version >= 2021.4) - generally improves performance of the code (enabled by -DWITH_TBB=ON)
• Eigen - provides additional methods for setting up initial conditions (enabled by -DWITH_EIGEN=ON)
• ChaiScript - allows to read and modify particle data from a script (enabled by -DWITH_CHAISCRIPT=ON)
• OpenVDB (version >= 8.1) - used for converting particles to volumetric data, usable by renderers (enabled by -DWITH_VDB=ON)

The compilation should be as easy as

mkdir build
cd build
cmake -DCMAKE_BUILD_TYPE=Release ..
make

By default, OpenSPH uses a custom thread pool for parallelization. It is possible to use Intel TBB library instead, using:

cmake -DCMAKE_BUILD_TYPE=Release -DWITH_TBB=ON ..

Alternatively, the code can be compiled using qmake build system.

Running a basic simulation

Simulations can be easily set up in the graphical application opensph, using a node-based editor. To use one of the simulation templates, click 'Project -> New session' and select one of the presets. Alternatively, see the category 'presets' on the right side of the editor. To start a simulation, either select 'Start run' from the 'Simulation' menu, or right-click any node and select 'Evaluate'.

For simulations of asteroid impacts, select the 'collision' or the 'fragmentation and reaccumulation' preset. The default simulation uses the following:

• Equation of motion consists of a stress tensor divergence (SolidStressForce) and an artifial viscosity term (StandardAV)
• Density evolution is solved using continuity equation (ContinuityEquation)
• Hooke's law as a constitutive equation
• von Mises criterion to account for plastic yield (VonMisesRheology)
• Grady-Kipp model of fragmentation with scalar damage quantity (ScalarDamage)
• Tillotson equation of state (TillotsonEos)
• Adaptive smoothing length (AdaptiveSmoothingLength)
• Basalt material parameters

Particle renderer

OpenSPH contains useful tools for visualization of particles. It allows rendering individual spherical particles as well as rendering of isosurface, reconstructed from particles. The color palette can be specified from arbitrary state quantities, making it easy to visualize particle velocities, internal energy, etc. The surface of bodies can be also textured with an arbitrary bitmap image.

Besides the orthographic and perspective projection, a fisheye camera for fulldome animations and a spherical 360° camera can be used.

Examples of library usage

It is certainly possible to use to library without the GUI executable and use the SPH or N-body solvers in other applications. There examples explain how to do that.

Code documentation

See documentation

Changelog

See changelog

Bug reports, ideas, question

Feel free to contact me at [email protected]. Any feedback is highly appreciated.