Aeroacoustics Your title goes here Methodologies, Validations and - - PowerPoint PPT Presentation
Aeroacoustics Your title goes here Methodologies, Validations and - - PowerPoint PPT Presentation
Aeroacoustics Your title goes here Methodologies, Validations and Continuing Outlook Your subtitle goes here Fred Mendona Some Characteristic Flow Noise Issues Autom omotiv otive e extern ernal, al, sunroof of buffet eting,
Some Characteristic Flow Noise Issues
- Autom
- motiv
- tive
e – extern ernal, al, sunroof
- f buffet
eting, ing, HVAC
- Aerospace – airframe noise, jets, ECS
Industry and Expert Collaborations
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DESTINY Aeroacoustics Projects (2002 - 2005)
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German Auto manufacturers – Aeroacoustics Working Group (2005-7 and 2009-11)
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Daimler, BMW, Audi, VW, Porsche
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Acoustic partner collaborations
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LMS through BEM codes SYSNOISE and V.Lab.Acoustics
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FFT’s FEA code, ACTRAN
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ESI’s SEA code, VA-One
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Aero-Vibroacoustics
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External flow excitation, internal structural noise transmission
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Internal flow excitation, external structural noise transmission
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One of the originators in the field, Paul Bremner, expert advisor to CD-adapco
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LES for Acoustics, Cambridge University Press
http://www.cambridge.org/us/catalogue/catalogue.asp?isbn=0521871441
Introduction
– CFD, with the correct physical models…. » Is very capable of simulating the sources of aeroacoustic noise
- Directly (LES) for applications in the low Reynolds number range
- Indirectly (RANS) using broadband syntesization models
» Also possible to propagate the noise – STAR-CCM+ provides the software tools to extract the maximum
value from the CFD process in Aeroacoustics CAE
» Dedicated Training programme for Aeroacoustics – CD-adapco sees as its responsibility to deliver the validated tools,
with the best-practice advice; stating value and limitations
Aeroacoustics Overview: v6.04 and beyond
Ae Aeroacous roacoustics ics Sim Simula lations ions Optio ions ns Steady ady state Transient ansient
Broad
- adban
band d Correla rrelatio ions ns Synt nthe hesized ized Fluc uctua uatio ions ns SNGR CURLE surf rfac ace PROUDMAN AN volume lume GOLD LDST STEI EIN 2D-ax axi LEE LEE Lille ley Mesh Freque equenc ncy Cut-off LES LES DES Trans ansien ient RANS Point int and d Surface FFTs Auto
- and Cross Spectra
ra – cohere herenc nce e and phas ase FW FW-H Direc ect Export
- rt to
ACTRAN AN / V.Lab ab.Ac Acou
- ustics
ics / VA-One One Expor port to Propa
- pagat
gation ion codes des Direc ect Noise e Propa
- paga
gatio ion Direc ect Export
- rt to
SEA for r inter ernal nal nois ise e charac haracter eris isatio ion
Process
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Steady-state: Model Optimisation
»
Source Locations (Broadband correlations, Lilley, Curle, Proudman)
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Mesh requirements (Mesh frequency cut-off estimator)
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Assess time-step requirements – Transient: Direct Source Capture
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Advanced turbulence models
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Advanced boundary conditions
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Compressible solutions
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Direct Propagation (in STAR-CCM+)
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Propagation via coupling to:
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SYSNOISE / V.Lab.Acoustics
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FFT-ACTRAN
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VA-One
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VibroAcoustics transmission via SEA, FEA
250 Hz 500 Hz 1000 Hz 2000 Hz
Steady-state: Broadband correlations for AAC sources
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Quadrupole-like sources re-synthesized from steady-state RANS result
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STAR 1st commercial CFD code to introduce Lilley source visualisation (2000)
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Curle surface noise correlation
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Proudman volume correlation
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Locates maximum noise sources quickly
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Adds value for
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Parametric design changes
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Locates regions for mesh refinement
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Locates regions for data output
Steady-state: Broadband correlations - Examples
Surface (Curle) Volume (Proudman)
Steady-state: Mesh Frequency Cut-off Estimator
– Unique to STAR – Estimates the resolvable frequency from steady-state results – Informs user of CFD grid suitability early in the process – E.g. Frequency of up to1000Hz in mirror wake example
Transient capabilities
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LES-type turbulence model
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DES (options of Spalart-Allmaras, k-ε, k-ωSST)
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DES advection scheme blending
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Full LES (wall resolved or unresolved)
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Advanced wall treatment
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y+ insensitive
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Non-reflecting conditions for
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Inflow and outflow boundaries
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Full Compressibility
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Interaction between the flow and acoustics
- Especially for cavity resonance
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Most efficient commercial transient solver
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2nd order space and time discretisation
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Spectral Analysis
» FFT at points and surfaces »
Auto and Cross spectra – coherence and phase
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Frequency and Wave Number Fourier analysis
Validated Methodology
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Monitor point in mirror wake
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Tail-off in predicted spectrum at mesh cut-off frequency of ~1000 Hz STAR Experiment
Validated Methodology
Surface FFT (dB) at 500Hz (top) and 1000Hz (bottom)
Direct Propagation in STAR-CCM+
– Mesh requirement » 20 cells per acoustic wavelength ( λ= c / f )
- In ambient conditions, you need cells of ~15mm to propagate a signal at
1000Hz
- Domain size = 1000D, (~10 λ )
– Non-reflective in/outflow boundaries
100 0 Hz 500 0 Hz 3150 50 Hz Over erall all
Propagation – FW-H and 3rd party code export
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STAR results capture the acoustic sources for propagation via
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Ffowcs Williams-Hawkings (far-field propagation of compact sources without internal reflections)
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STAR offers coupling to 3rd party propagation codes:
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FFT, ACTRAN
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LMS, Virtual.Lab.Acoustics
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ESI, VA-One
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VibroAcoustics
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Using FVS in STAR-CCM+
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Export to SEA and FEA
Industrial examples with Validations
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Resonance Effects
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Slat / Cavity /Flap
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HVAC duct: Dipole Sources
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Fan Noise
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Side-view mirror: External Aero
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