NASA Logo

NTRS

NTRS - NASA Technical Reports Server

Back to Results
Enhanced Far Ultra-Violet Optical Properties of Physical Vapor Deposited Aluminum Mirrors Through Fluorination Astronomical instrumentation for measurements in the Far Ultra-Violet (FUV, 90-200 nm) typically use aluminum (Al) thin films due to their high reflectance over this wavelength range. However, the native aluminum oxide layer that forms on Al upon exposure to the atmosphere is strongly absorbing in this wavelength range, requiring that the films be protected with a dielectric that inhibits oxidation. Typically, magnesium fluoride (MgF2) or lithium fluoride (LiF) coatings are used as protective layers, but each has shortcomings. For example, MgF2 has an absorption cutoff at 115 nm reducing performance in a critical part of the FUV spectrum of observational interest. A viable option to access these lower wavelengths could be the use of the LiF overcoat as it has a lower absorption cutoff at 102.5 nm, but it is hygroscopic and thus susceptible to degradation in humid conditions. An approach to reduce the hygroscopic nature of LiF would be to implement a passivation process during the deposition of both Al+LiF coatings. Our team at GSFC has developed a new reactive Physical Vapor Deposition (rPVD) process that consists of a fluorination process with XeF2 gas combined with our traditional PVD process. We have found that this new rPVD coating process offers a protected version of Al+LiF with a more environmentally stable and more transparent LiF layer, along with unprecedent reflectivity. The process starts with a bare optically smooth substrate that is coated with Al in an ultra-high vacuum (UHV) chamber by the conventional PVD process. Then, the bare Al mirror is immediately exposed to a reactive XeF2 gas before and after the application of the flash PVD evaporated LiF layer. We have also been investigating the use of this rPVD coating process for potential efficiency enhancements of Si-based gratings. Since it is known that the XeF2 vapor is a strong Si etchant, we are investigating if the native SiO2 layer on Si is sufficient to protect the groove profile of e-beam-ruled Si gratings from degradation. We will report on the characterization of various Al+LiF witness mirror coatings (both on borosilicate and Si) performed under various deposition conditions using the XeF2 passivation process. These tests include XPS to determine film stoichiometry and AFM/SEM to measure surface roughness and any etching on the Si substrate. We will also report on FUV reflectance and spectroscopic ellipsometry to characterize optical constants of these passivated films in the UV/Visible/NIR spectral ranges.
Document ID
20240000047
Acquisition Source
Goddard Space Flight Center
Document Type
Poster
Authors
M. A. Quijada
(Goddard Space Flight Center Greenbelt, Maryland, United States)
J. G. del Hoyo
(Goddard Space Flight Center Greenbelt, Maryland, United States)
L. V. Rodriguez de Marcos
(Catholic University of America Washington D.C., District of Columbia, United States)
D. M. Lewis
(Brigham Young University Provo, Utah, United States)
E. J. Wollack
(Goddard Space Flight Center Greenbelt, Maryland, United States)
T. D. Rydalch
(Brigham Young University Provo, Utah, United States)
D. D. Allred
(Brigham Young University Provo, Utah, United States)
Date Acquired
January 2, 2024
Subject Category
Chemistry and Materials (General)
Meeting Information
Meeting: 243rd American Astronomical Society Meeting
Location: New Orleans, LA
Country: US
Start Date: January 7, 2024
End Date: January 11, 2024
Sponsors: American Astronomical Society
Funding Number(s)
WBS: 141108.04.02.01.66
CONTRACT_GRANT: 21-SAT21-0027 A
Distribution Limits
Public
Copyright
Use by or on behalf of the US Gov. Permitted.
Technical Review
Single Expert
Keywords
Engineering (General)
No Preview Available