Research on Wind Flow Control by Windbreak Fence for a Large Radio Telescope Site Based on Numerical Simulations

The higher the pointing accuracy of the radio telescope, the more obvious the influence of wind disturbance on antenna performance. Taking the site of the 110 m aperture QiTai radio Telescope (QTT) as an example, the terrain and air flow characteristics of the site are studied. It is found that the...

Full description

Saved in:
Bibliographic Details
Main Authors: Feilong He, Qian Xu, Na Wang
Format: Article
Language:English
Published: Wiley 2023-01-01
Series:Advances in Astronomy
Online Access:http://dx.doi.org/10.1155/2023/5257749
Tags: Add Tag
No Tags, Be the first to tag this record!
_version_ 1850120791481384960
author Feilong He
Qian Xu
Na Wang
author_facet Feilong He
Qian Xu
Na Wang
author_sort Feilong He
collection DOAJ
description The higher the pointing accuracy of the radio telescope, the more obvious the influence of wind disturbance on antenna performance. Taking the site of the 110 m aperture QiTai radio Telescope (QTT) as an example, the terrain and air flow characteristics of the site are studied. It is found that the wind direction with high incoming wind frequency and relatively high speed is mostly located in the mountain gap on the periphery of the antenna. If the wind resistance facilities are precisely arranged in the upstream tuyere, the wind speed in the antenna area can be effectively reduced. This study proposes a method to control the wind flow at a telescope site based on the precise arrangement of the windbreak fence. The windbreak fence simulation model is constructed using the theory of porous jump. The mean error of the simulation results is less than 14% compared to the wind tunnel measured data, indicating that the constructed windbreak fence model has high reliability. The computational domain model of the working conditions for the site is constructed. The extreme condition of the windbreak fence arrangement is considered, and the simulation results show that the wind speed in the antenna area can be reduced by more than 30% through the control of the windbreak fence. It verifies the feasibility of the method of controlling the wind flow by the windbreak fence for the site which provides a reference for the subsequent research on the precise arrangement of the windbreak fence.
format Article
id doaj-art-63c4df80d7294d7f8d79b7b6c5d06c58
institution OA Journals
issn 1687-7977
language English
publishDate 2023-01-01
publisher Wiley
record_format Article
series Advances in Astronomy
spelling doaj-art-63c4df80d7294d7f8d79b7b6c5d06c582025-08-20T02:35:16ZengWileyAdvances in Astronomy1687-79772023-01-01202310.1155/2023/5257749Research on Wind Flow Control by Windbreak Fence for a Large Radio Telescope Site Based on Numerical SimulationsFeilong He0Qian Xu1Na Wang2Xinjiang Astronomical ObservatoryXinjiang Astronomical ObservatoryXinjiang Astronomical ObservatoryThe higher the pointing accuracy of the radio telescope, the more obvious the influence of wind disturbance on antenna performance. Taking the site of the 110 m aperture QiTai radio Telescope (QTT) as an example, the terrain and air flow characteristics of the site are studied. It is found that the wind direction with high incoming wind frequency and relatively high speed is mostly located in the mountain gap on the periphery of the antenna. If the wind resistance facilities are precisely arranged in the upstream tuyere, the wind speed in the antenna area can be effectively reduced. This study proposes a method to control the wind flow at a telescope site based on the precise arrangement of the windbreak fence. The windbreak fence simulation model is constructed using the theory of porous jump. The mean error of the simulation results is less than 14% compared to the wind tunnel measured data, indicating that the constructed windbreak fence model has high reliability. The computational domain model of the working conditions for the site is constructed. The extreme condition of the windbreak fence arrangement is considered, and the simulation results show that the wind speed in the antenna area can be reduced by more than 30% through the control of the windbreak fence. It verifies the feasibility of the method of controlling the wind flow by the windbreak fence for the site which provides a reference for the subsequent research on the precise arrangement of the windbreak fence.http://dx.doi.org/10.1155/2023/5257749
spellingShingle Feilong He
Qian Xu
Na Wang
Research on Wind Flow Control by Windbreak Fence for a Large Radio Telescope Site Based on Numerical Simulations
Advances in Astronomy
title Research on Wind Flow Control by Windbreak Fence for a Large Radio Telescope Site Based on Numerical Simulations
title_full Research on Wind Flow Control by Windbreak Fence for a Large Radio Telescope Site Based on Numerical Simulations
title_fullStr Research on Wind Flow Control by Windbreak Fence for a Large Radio Telescope Site Based on Numerical Simulations
title_full_unstemmed Research on Wind Flow Control by Windbreak Fence for a Large Radio Telescope Site Based on Numerical Simulations
title_short Research on Wind Flow Control by Windbreak Fence for a Large Radio Telescope Site Based on Numerical Simulations
title_sort research on wind flow control by windbreak fence for a large radio telescope site based on numerical simulations
url http://dx.doi.org/10.1155/2023/5257749
work_keys_str_mv AT feilonghe researchonwindflowcontrolbywindbreakfenceforalargeradiotelescopesitebasedonnumericalsimulations
AT qianxu researchonwindflowcontrolbywindbreakfenceforalargeradiotelescopesitebasedonnumericalsimulations
AT nawang researchonwindflowcontrolbywindbreakfenceforalargeradiotelescopesitebasedonnumericalsimulations