M-Star CFD Capabilities
Time-Accurate CFD
Large Eddy Simulation means no guessing on turbulence models
No Meshing
Save time with minimal pre-processing
Complex Physics
Model custom chemical reaction rates, heat transfer, and more
Cloud Enabled
Submit jobs directly to secure cloud provider
M-Star CFD is a general-purpose solver for modeling three-dimensional, time-varying fluid flow, chemical reactions, heat transfer, and particle dynamics. The software is developed aggressively; users are supported energetically. Contact us today to get started.
Fluid Models
- Newtonian
- Power law
- Carreau fluids
- Herschel-Bulkley
- Thixotropic fluids
- User defined viscosity-strain relationships
Multi-phase Physics
- Free surface flows
- Lagrangian particle and bubble tracking
- Bubble and particle break-up/coalescence
- Immissible fluid interactions
- Miscible fluids and stratified systems
- One and two-way particle and bubble coupling
Scalar Transport
- Thermal transport
- Scalar field transport
- Multi-species reactions
- Exothermic/endothermic reactions
- Viscous heating and softening
- Sub-grid mixing
- Fast reaction treatment
Momentum Transport
- Direct numerical simulation
- Smagorinsky large eddy simulation (LES)
- Time-averaged flow field
- Frozen turbulent flow field
In-Situ Analysis
- Custom plugin support (User Defined Functions)
- Blending/mean-age
- Residence time distribution
- Recirculation loops
- Static/moving probes
Geometry
- Windows-based GUI
- Import IGES, STEP, STL files
- Built-in parametric geometry
- No user meshing
Computational Backend
- MPI support for Windows and Linux
- Self-optimizing block generation
- Variable mesh support (coming 2018)
- GPU support (coming 2018)
Post-Processing
- Open source 2D/3D VTK output
- One-click post-processing in ParaView
- User-defined post-processing scripts
Support
- Virtual via screen sharing and phone
- Email support
- On-site training available