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Coming clean: understanding and mitigating optical contamination and laser induced damage in advanced LIGO

Gushwa, Kaitlin E. and Torrie, Calum I. (2014) Coming clean: understanding and mitigating optical contamination and laser induced damage in advanced LIGO. In: Laser-Induced Damage in Optical Materials: 2014. Proceedings of SPIE. No.9237. Society of Photo-optical Instrumentation Engineers (SPIE) , Bellingham, WA, Art. No. 923702. ISBN 978-1-62841-300-7. http://resolver.caltech.edu/CaltechAUTHORS:20150311-104401320

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Abstract

The cleanliness of optical surfaces is of great concern as the Advanced Laser Interferometer Gravitational-Wave Observatory (LIGO) project transitions from installation to operation at full power. More particulates than expected were observed on and near the core optics as a result of assembly and installation work, prompting a re-evaluation of longheld contamination control practices. Even low particulate levels can potentially damage the fused silica optics and reduce overall interferometer sensitivity. These risks are mitigated from a combination of the following approaches: quantifying the extent of the contamination, identifying its sources, improving practices to reduce the generation of particulates, introducing a non-contact in-situ cleaning technique for suspended optics in air, qualifying cleanliness levels against induced damage, and developing methods for remotely measuring and cleaning suspended optics under vacuum. While significant progress has been made in understanding and mitigating contamination, and thus, protecting the optics from losses and damage, there is still more work to be done to reach ultimate performance requirements.


Item Type:Book Section
Related URLs:
URLURL TypeDescription
http://dx.doi.org/10.1117/12.2066909DOIArticle
http://proceedings.spiedigitallibrary.org/proceeding.aspx?articleid=1921817PublisherArticle
Additional Information:© 2014 SPIE. The authors gratefully acknowledge the support of the United States National Science Foundation (award No. PHY-0757058). LIGO was constructed by the California Institute of Technology and Massachusetts Institute of Technology with funding from the National Science Foundation, and operates under cooperative agreement PHY-0107417. Caltech also acknowledges financial support from the Science and Technology Facilities Council of the United Kingdom. This paper filed internally under LIGO document number LIGO- P1400205. LIGO Internal Reports may be accessed at https://dcc.ligo.org/cgi-bin/DocDB/DocumentDatabase. The authors wish to acknowledge the many colleagues in LIGO and the LIGO Scientific Collaboration who have supported this work. In particular, the authors would like to thank Jeff Bartlett, Garilynn Billingsley, Dennis Coyne, Eric Gustafson, Matthew Heintze, Norna Robertson, Betsy Weaver and Liyuan Zhang within LIGO. In addition, the authors would like to thank all of the excellent contacts they now have within the National Ignition Facility.
Funders:
Funding AgencyGrant Number
NSFPHY-0757058
NSFPHY-0107417
Science and Technology Facilities Council (STFC)UNSPECIFIED
Subject Keywords:LIGO; gravitational waves; ultra-high vacuum system; coated fused silica optics; damage, absorption and scatter; contamination control; particulate cleanliness level; obscuration ratio
Other Numbering System:
Other Numbering System NameOther Numbering System ID
LIGO Document NumberLIGO-P1400205
Record Number:CaltechAUTHORS:20150311-104401320
Persistent URL:http://resolver.caltech.edu/CaltechAUTHORS:20150311-104401320
Official Citation:Kaitlin E. Gushwa and Calum I. Torrie "Coming clean: understanding and mitigating optical contamination and laser induced damage in advanced LIGO", Proc. SPIE 9237, Laser-Induced Damage in Optical Materials: 2014, 923702 (October 31, 2014); doi:10.1117/12.2066909; http://dx.doi.org/10.1117/12.2066909
Usage Policy:No commercial reproduction, distribution, display or performance rights in this work are provided.
ID Code:55699
Collection:CaltechAUTHORS
Deposited By: Jason Perez
Deposited On:11 Mar 2015 23:17
Last Modified:11 Mar 2015 23:17

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