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dc.contributor.authorGhosh, Supriyo
dc.contributor.authorBoonsri, Chantira
dc.contributor.authorMartin, William
dc.contributor.authorJones, Hugh R. A.
dc.contributor.authorChoochalerm, Piyamas
dc.contributor.authorUsher, Sarah
dc.contributor.authorYerolatsitis, Stephanos
dc.contributor.authorWocial, Thomas
dc.contributor.authorWright, Thomas
dc.date.accessioned2024-01-12T09:30:03Z
dc.date.available2024-01-12T09:30:03Z
dc.date.issued2024-01-02
dc.identifier.citationGhosh , S , Boonsri , C , Martin , W , Jones , H R A , Choochalerm , P , Usher , S , Yerolatsitis , S , Wocial , T & Wright , T 2024 , ' Mitigating Modal Noise in Multimode Circular Fibres by Optical Agitation using a Galvanometer ' , RAS Techniques and Instruments , vol. 3 , no. 1 , pp. 8-18 . https://doi.org/10.1093/rasti/rzad059
dc.identifier.issn2752-8200
dc.identifier.otherArXiv: http://arxiv.org/abs/2312.16996v1
dc.identifier.urihttp://hdl.handle.net/2299/27406
dc.description© 2024 The Author(s). Published by Oxford University Press on behalf of Royal Astronomical Society. This is an open access article distributed under the terms of the Creative Commons Attribution License (CC BY), https://creativecommons.org/licenses/by/4.0/
dc.description.abstractModal noise appears due to the non-uniform and unstable distribution of light intensity among the finite number of modes in multimode fibres. It is an important limiting factor in measuring radial velocity precisely by fibre-fed high-resolution spectrographs. The problem can become particularly severe as the fibre's core become smaller and the number of modes that can propagate reduces. Thus, mitigating modal noise in relatively small core fibres still remains a challenge. We present here a novel technique to suppress modal noise. Two movable mirrors in the form of a galvanometer reimage the mode-pattern of an input fibre to an output fibre. The mixing of modes coupled to the output fibre can be controlled by the movement of mirrors applying two sinusoidal signals through a voltage generator. We test the technique for four multimode circular fibres: 10 and 50 micron step-index, 50 micron graded-index, and a combination of 50 micron graded-index and 5:1 tapered fibres (GI50t). We present the results of mode suppression both in terms of the direct image of the output fibre and spectrum of white light obtained with the high-resolution spectrograph. We found that the galvanometer mitigated modal noise in all the tested fibres, but was most useful for smaller core fibres. However, there is a trade-off between the modal noise reduction and light-loss. The GI50t provides the best result with about 60% mitigation of modal noise at a cost of about 5% output light-loss. Our solution is easy to use and can be implemented in fibre-fed spectrographs.en
dc.format.extent11
dc.format.extent4120656
dc.language.isoeng
dc.relation.ispartofRAS Techniques and Instruments
dc.subjectastro-ph.IM
dc.subjectastro-ph.EP
dc.subjectastro-ph.SR
dc.titleMitigating Modal Noise in Multimode Circular Fibres by Optical Agitation using a Galvanometeren
dc.contributor.institutionDepartment of Physics, Astronomy and Mathematics
dc.contributor.institutionCentre for Astrophysics Research (CAR)
dc.contributor.institutionSchool of Physics, Engineering & Computer Science
dc.contributor.institutionUniversity of Hertfordshire
dc.description.statusPeer reviewed
rioxxterms.versionofrecord10.1093/rasti/rzad059
rioxxterms.typeJournal Article/Review
herts.preservation.rarelyaccessedtrue


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