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Analysis of Wind Influence to Radio Astronomy Observations at Irbene Radio-telescope Complex Cover

Analysis of Wind Influence to Radio Astronomy Observations at Irbene Radio-telescope Complex

Open Access
|Jan 2012

Abstract

The results of modelling wind-related deformations in an RT-16 radio telescope (located at Irbene, Latvia) mirror system are presented. The Finite Volume method is used for the development of a Computational Fluid Dynamic model of turbulent airflow around the telescope. An open sourced Computational Fluid Dynamic toolkit OpenFOAM is used for the solution of Partial Different Equations. Notable model difficulties arise due to the open nature of the air flow leading to unknown far field turbulence parameters. Our future plans are to create a unified, coupled, liquid-solid interaction model for RT-32/RT-16 antennas.

DOI: https://doi.org/10.2478/v10145-011-0017-z | Journal eISSN: 2255-8837 | Journal ISSN: 1691-5208
Language: English
Page range: 118 - 126
Published on: Jan 13, 2012
In partnership with: Paradigm Publishing Services
Publication frequency: 2 issues per year

© 2012 Sabine Upnere, Normunds Jekabsons, Roberts Joffe, Valerijs Bezrukovs, Vladislavs Bezrukovs, published by Riga Technical University
This work is licensed under the Creative Commons License.

Volume 6 (2011): Issue -1 (June 2011)