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Block Krylov subspace methods for the computation of structural response to turbulent wind

In this paper the numerical computation of the dynamic response to turbulent wind excitations of slender structures is addressed. A numerical procedure capable to effectively estimate the three-dimensional structural behavior is proposed, based on a direct frequency domain approach. A probabilistic...

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Published in:Computer methods in applied mechanics and engineering 2011-06, Vol.200 (23), p.2067-2082
Main Authors: Barbella, G., Perotti, F., Simoncini, V.
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Language:English
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description In this paper the numerical computation of the dynamic response to turbulent wind excitations of slender structures is addressed. A numerical procedure capable to effectively estimate the three-dimensional structural behavior is proposed, based on a direct frequency domain approach. A probabilistic description of the wind velocity field, accounting for the correlation between the turbulence components, is combined to a linearized fluid–structure interaction model, under the quasi-steady hypothesis. We propose robust implementations of multiple right-hand side and multiple shift Krylov subspace methods with deflation of basis vectors, which allow us to efficiently analyze the dynamic response for a wide range of frequency values and wind time histories. Numerical experiments are reported with data stemming from real structure modeling.
doi_str_mv 10.1016/j.cma.2011.02.017
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1879-2138
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subjects Block methods
Deflation techniques
Dynamic response
Earth, ocean, space
Exact sciences and technology
External geophysics
Fluid-structure interaction
Frequency domain analysis
Frequency domains
Fundamental areas of phenomenology (including applications)
Iterative nonsymmetric solvers
Mathematical models
Meteorology
Physics
Solid mechanics
Stemming
Structural and continuum mechanics
Subspace methods
Turbulent flow
Turbulent wind
Vibration, mechanical wave, dynamic stability (aeroelasticity, vibration control...)
Winds and their effects
title Block Krylov subspace methods for the computation of structural response to turbulent wind
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