Room temperature plasma-etching and surface passivation of far-ultraviolet Al mirrors using electron beam generated plasmas

The development of optical systems operating in the far ultraviolet range (FUV, λ=100-200 nm) is limited by the efficiency of passivated aluminum (Al) mirrors. Although it is presently possible to obtain high-reflectivity FUV mirrors through physical vapor deposition, the process involves deposition...

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Veröffentlicht in:Optical materials express 2021-03, Vol.11 (3), p.740
Hauptverfasser: Rodriguez de Marcos, Luis V., Boris, David R., Gray, Emrold, del Hoyo, Javier G., Kozen, Alexander C., Richardson, Joseph G., Rosenberg, Samantha G., Walton, Scott G., Wheeler, Virginia, Wollack, Edward J., Woodward, Jeffrey M., Quijada, Manuel A.
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Sprache:eng
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Zusammenfassung:The development of optical systems operating in the far ultraviolet range (FUV, λ=100-200 nm) is limited by the efficiency of passivated aluminum (Al) mirrors. Although it is presently possible to obtain high-reflectivity FUV mirrors through physical vapor deposition, the process involves deposition with substrates at high temperatures, which is technically challenging for large optical elements. A novel passivation procedure for bare Al mirrors is reported. The treatment consisted of using a low-temperature electron-beam generated plasma produced in a gas mixture of Ar and SF 6 to etch away the native oxide layer from the Al film, while simultaneously promoting the generation of a thin aluminum tri-fluoride (AlF 3 ) layer on the Al surface. In the first section we analyze the effect of varying both ion energy and SF 6 concentration on the FUV reflectance, thickness, composition, and surface morphology of the resulting AlF 3 protective layers. In the second section, the reflectivity of samples is optimized at selected important FUV wavelengths for astronomical observations. Notably, samples attained state-of-the-art reflectances of 75% at 108.5 nm (He Lyman γ), 91% at 121.6 nm (H Lyman α), 90% at 130.4 nm (OI), and of 95% at 155.0 nm (C IV). The stability over time of these passivated mirrors is also investigated.
ISSN:2159-3930
2159-3930
DOI:10.1364/OME.417475