Impact of Atmospheric Turbulence on Dynamic Wind Loads on Heliostats

This study analyses the turbulent wind properties in the lower 10 m of the atmospheric surface layer close to the ground where heliostats are located. Power spectral densities of streamwise and vertical components of wind are analysed, and the frequencies associated with the peak of the spectra are determined using field data collected at two open-country terrains in addition to spectral models of ESDU85020. Variations of the peak frequencies with height from the ground, terrain type and average wind speed are discussed and the impact on heliostat wind loads are described. It is found that while the peak frequency of the streamwise turbulence is between 0.01–0.1 Hz, the peak of the vertical turbulence occurs at frequencies in the range of 0.1–1 Hz. It is shown that smaller heliostats that are located closer to the ground are exposed to turbulent wind fluctuations at a higher frequency and are thus expected to experience wind loads with a higher dominant frequency compared to larger heliostats located higher above the ground. These frequencies need to be considered in design of heliostat drives and structural components

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Publication Details

Journal
SolarPACES Conference Proceedings
Published
2024-09-16
DOI
https://doi.org/10.52825/solarpaces.v2i.835
Primary Topic
Wind and Air Flow Studies
Type
article
Field-Weighted Citation Impact
0.00

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article

Impact of Atmospheric Turbulence on Dynamic Wind Loads on Heliostats

Azadeh Jafari, Matthew J. Emes, Maziar Arjomandi
SolarPACES Conference Proceedings
Wind and Air Flow Studies
article

Impact of Atmospheric Turbulence on Dynamic Wind Loads on Heliostats

Azadeh Jafari, Matthew J. Emes, Maziar Arjomandi
article en

Abstract

This study analyses the turbulent wind properties in the lower 10 m of the atmospheric surface layer close to the ground where heliostats are located. Power spectral densities of streamwise and vertical components of wind are analysed, and the frequencies associated with the peak of the spectra are determined using field data collected at two open-country terrains in addition to spectral models of ESDU85020. Variations of the peak frequencies with height from the ground, terrain type and average wind speed are discussed and the impact on heliostat wind loads are described. It is found that while the peak frequency of the streamwise turbulence is between 0.01–0.1 Hz, the peak of the vertical turbulence occurs at frequencies in the range of 0.1–1 Hz. It is shown that smaller heliostats that are located closer to the ground are exposed to turbulent wind fluctuations at a higher frequency and are thus expected to experience wind loads with a higher dominant frequency compared to larger heliostats located higher above the ground. These frequencies need to be considered in design of heliostat drives and structural components

SolarPACES Conference ProceedingsVol. 2
The University of Adelaide (AU)
U.S. Department of Energy, Australian Solar Thermal Research Institute, Solar Energy Technologies Office
Openalex Percentile: Top 85%
Wind and Air Flow Studies
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Impact of Atmospheric Turbulence on Dynamic Wind Loads on Heliostats — Azadeh Jafari, Matthew J. Emes, et al. · SolarPACES Conference Proceedings (2024) | TGRS Research Map | TGRS