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Review and Performance Testing of the Optical Power Monitor (PMON) The LISA mission requires a high precision optical power monitoring and control system that combines high reliability and measurement accuracy with extremely low disturbance to the core interferometric detection system. NASA is working with Avo Photonics to design and build this optical power monitor, known as PMON. The high-level design requirements take into account detector redundancy, mechanical rigidity, stability against temperature and input alignment changes, parasitic scatter and reflection artifacts, as well as low magnetic field. Gamma and Proton radiation tests have been performed on the photodiodes from a few vendors to verify radiation tolerance. Engineering development units of the PMON have been fabricated, delivered and evaluated at NASA.
Document ID
20240008319
Acquisition Source
Goddard Space Flight Center
Document Type
Poster
Authors
Hua Jiao
(Goddard Space Flight Center Greenbelt, United States)
Molly Fahey
(Goddard Space Flight Center Greenbelt, United States)
Kenji Numata
(Goddard Space Flight Center Greenbelt, United States)
Anthony W. Yu
(Goddard Space Flight Center Greenbelt, United States)
Aleksey Vasilyev
(System Science Applications (United States) Los Angeles, California, United States)
Wei Lu
(NOVA Federal LLC Arlington, Virginia, United States)
David Demmer
(AVO Photonics)
Will Drobnick
(AVO Photonics)
Rob Smith
(AVO Photonics)
Date Acquired
June 29, 2024
Publication Date
July 7, 2024
Publication Information
Publication: Journal of Physics
Publisher: IOP Science
Subject Category
Astronomy
Optics
Meeting Information
Meeting: 15th International LISA Symposium
Location: Dublin
Country: IE
Start Date: July 7, 2024
End Date: July 12, 2024
Sponsors: University College Dublin, UCD Centre for Space Research
Funding Number(s)
WBS: 244904.04.09.05.05.02.01
CONTRACT_GRANT: 80GSFC18C0120
Distribution Limits
Public
Copyright
Use by or on behalf of the US Gov. Permitted.
Technical Review
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