Shear- and Self-Noise Sources
The main sources of aerodynamically generated sound can be decomposed into a shear-noise term (generated by the interaction between the mean shear velocities and turbulent velocity components of the flow) and self-noise term (generated by turbulence-turbulence interactions). Simcenter STAR-CCM+ allows you to compute these noise source terms from a synthetic turbulent velocity field.
The synthetic turbulent velocity field is generated from a steady-state Reynolds-Averaged Navier-Stokes (RANS) flow solution using random Fourier modes. This method, called the Stochastic Noise Generation and Radiation (SNGR) model, was proposed by Kraichnan [847] and Karweit et al.[845], and afterward developed by Bailly and Juve [824], Bechara et al.[825].
The following noise source models allow you to compute shear- and self-noise sources from the synthetic turbulent velocity field:
Note | These models solve for noise sources only—not for acoustic wave propagation. |
- Lilley Sources
- The Lilley Sources model uses a nonlinear function to compute shear- and self-noise sources.
- LEE Sources
- The Linearized Euler Equation (LEE) Sources model accounts for refraction and convection effects in any sheared mean flows. The equations can be used for a wider range of conditions than the Lilley equation, where the associated source term is a nonlinear function of the fluctuating velocity flow field. See [42].