Unsteady RANS and DES for simulating flow and tonal noise in centrifugal fans
Title: |
Unsteady RANS and DES for simulating flow and tonal noise in centrifugal fans |
DNr: |
SNIC 2018/3-437 |
Project Type: |
SNIC Medium Compute |
Principal Investigator: |
Alf-Erik Almstedt <affe@chalmers.se> |
Affiliation: |
Chalmers tekniska högskola |
Duration: |
2018-10-01 – 2019-10-01 |
Classification: |
20306 |
Keywords: |
|
Abstract
Tonal noise from an isolated centrifugal fan is investigated using unsteady Reynolds-averaged Navier-Stokes (URANS) simulations. Isolated
centrifugal fans are often used in ventilation systems and play an important role in producing tonal and broadband noise. The broadband noise can be reduced when
the fan efficiency is optimized. However, the tonal noise cannot be effectively reduced. It is therefore of great interest to identify and reduce the tonal noise
for this type of fans operating in public environment. The noise is predicted by coupling the URANS and the Ffowcs Williams and Hawkings acoustic analogy. The
numerical methodology and mesh generation methods are validated. Numerical simulation is a more convenient way to identify tonal noise than experiments. However,
simulation of the noise using advanced computational fluid dynamics (CFD) methods (e.g., large eddy simulation) requires many computational resources. To predict
the tonal noise, a convenient method is the URANS. The method can simulate characteristic unsteady structures, which are responsible for the tonal
noise generation, with low computational costs. Though it has a drawback to provide the fluctuations that are important for the broadband noise generation. The
aerodynamic properties obtained from RANS and URANS are consistent with the experimental data. The magnitudes of the tonal noise at the blade passing frequencies
are well predicted. Moreover, the broadband noise below 350 Hz agrees with the measurement although obvious discrepancies are found at high frequencies, which
cannot be resolved by URANS.