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Improving sodium laser guide star brightness by polarization switching

Optical pumping with circularly polarized light has been used to enhance the brightness of sodium laser guide star. But the benefit is reduced substantially due to the precession of sodium atoms in geomagnetic field. Switching the laser between left and right circular polarization at the Larmor freq...

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Detalles Bibliográficos
Autores principales: Fan, Tingwei, Zhou, Tianhua, Feng, Yan
Formato: Online Artículo Texto
Lenguaje:English
Publicado: Nature Publishing Group 2016
Materias:
Acceso en línea:https://www.ncbi.nlm.nih.gov/pmc/articles/PMC4750368/
https://www.ncbi.nlm.nih.gov/pubmed/26797503
http://dx.doi.org/10.1038/srep19859
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author Fan, Tingwei
Zhou, Tianhua
Feng, Yan
author_facet Fan, Tingwei
Zhou, Tianhua
Feng, Yan
author_sort Fan, Tingwei
collection PubMed
description Optical pumping with circularly polarized light has been used to enhance the brightness of sodium laser guide star. But the benefit is reduced substantially due to the precession of sodium atoms in geomagnetic field. Switching the laser between left and right circular polarization at the Larmor frequency is proposed to improve the return. With ESO’s laser guide star system at Paranal as example, numerical simulation shows that the return flux is increased when the angle between geomagnetic field and laser beam is larger than 60°, as much as 50% at 90°. The proposal is significant since most astronomical observation is at angle between 60° and 90° and it only requires a minor addition to the delivery optics of present laser system.
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spelling pubmed-47503682016-02-18 Improving sodium laser guide star brightness by polarization switching Fan, Tingwei Zhou, Tianhua Feng, Yan Sci Rep Article Optical pumping with circularly polarized light has been used to enhance the brightness of sodium laser guide star. But the benefit is reduced substantially due to the precession of sodium atoms in geomagnetic field. Switching the laser between left and right circular polarization at the Larmor frequency is proposed to improve the return. With ESO’s laser guide star system at Paranal as example, numerical simulation shows that the return flux is increased when the angle between geomagnetic field and laser beam is larger than 60°, as much as 50% at 90°. The proposal is significant since most astronomical observation is at angle between 60° and 90° and it only requires a minor addition to the delivery optics of present laser system. Nature Publishing Group 2016-01-22 /pmc/articles/PMC4750368/ /pubmed/26797503 http://dx.doi.org/10.1038/srep19859 Text en Copyright © 2016, Macmillan Publishers Limited http://creativecommons.org/licenses/by/4.0/ This work is licensed under a Creative Commons Attribution 4.0 International License. The images or other third party material in this article are included in the article’s Creative Commons license, unless indicated otherwise in the credit line; if the material is not included under the Creative Commons license, users will need to obtain permission from the license holder to reproduce the material. To view a copy of this license, visit http://creativecommons.org/licenses/by/4.0/
spellingShingle Article
Fan, Tingwei
Zhou, Tianhua
Feng, Yan
Improving sodium laser guide star brightness by polarization switching
title Improving sodium laser guide star brightness by polarization switching
title_full Improving sodium laser guide star brightness by polarization switching
title_fullStr Improving sodium laser guide star brightness by polarization switching
title_full_unstemmed Improving sodium laser guide star brightness by polarization switching
title_short Improving sodium laser guide star brightness by polarization switching
title_sort improving sodium laser guide star brightness by polarization switching
topic Article
url https://www.ncbi.nlm.nih.gov/pmc/articles/PMC4750368/
https://www.ncbi.nlm.nih.gov/pubmed/26797503
http://dx.doi.org/10.1038/srep19859
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