2004
DOI: 10.1364/ao.43.001835
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Experimental comparison of extreme-ultraviolet multilayers for solar physics

Abstract: We compare the reflectance and stability of multilayers comprising either Si/Mo, Si/Mo2C, Si/B4C, Si/C, or Si/SiC bilayers, designed for use as extreme-ultraviolet (EUV) reflective coatings. The films were deposited by using magnetron sputtering and characterized by both x-ray and EUV reflectometry. We find that the new Si/SiC multilayer offers the greatest spectral selectivity at the longer wavelengths, as well as the greatest thermal stability. We also describe the optimization of multilayers designed for th… Show more

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Cited by 61 publications
(33 citation statements)
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“…In addition to this, Mg/SiC possesses several other favorable properties: near-zero film stress, good spectral selectivity and thermal stability up to about 350° C [17,18]. This unique combination of properties is highly desirable for mirror multilayer coatings in solar physics instrumentation and is unmatched by any of the other multilayer material pairs operating in the > 25 nm wavelength region such as Mo/Si [19], SiC/Si [19], Sc/Si [20], B 4 C/Si [19], Al/SiC [21], other Mg-based multilayers such as Mg/Co [22], and rare-earth based multilayers [23][24][25][26]. Despite the superior optical performance of Mg/SiC multilayers in the EUV region when compared to other material pairs, their use as coatings in applications that require long-term stability, such as for example the EUV imaging telescopes aboard NASA's Solar Dynamics Observatory mission [14], has been hindered by Mg corrosion [15,27].…”
Section: Introductionmentioning
confidence: 99%
“…In addition to this, Mg/SiC possesses several other favorable properties: near-zero film stress, good spectral selectivity and thermal stability up to about 350° C [17,18]. This unique combination of properties is highly desirable for mirror multilayer coatings in solar physics instrumentation and is unmatched by any of the other multilayer material pairs operating in the > 25 nm wavelength region such as Mo/Si [19], SiC/Si [19], Sc/Si [20], B 4 C/Si [19], Al/SiC [21], other Mg-based multilayers such as Mg/Co [22], and rare-earth based multilayers [23][24][25][26]. Despite the superior optical performance of Mg/SiC multilayers in the EUV region when compared to other material pairs, their use as coatings in applications that require long-term stability, such as for example the EUV imaging telescopes aboard NASA's Solar Dynamics Observatory mission [14], has been hindered by Mg corrosion [15,27].…”
Section: Introductionmentioning
confidence: 99%
“…The SiC/Mg structure could be another possible structure for multilayers working at 30.4nm [11]. As can be seen in figure 5 this kind of multilayer shows a better reflectivity than the standard Mo/Si and the Si/B 4 C structure.…”
Section: Sic/mgmentioning
confidence: 97%
“…Until recently, most reflective EUV coatings for space and other applications at wavelengths longer than 12.4 nm (the Si L absorption edge) and up to approximately 40 nm were fabricated of multilayer structures containing silicon as a low absorbing material. 17 However, at wavelengths beyond the Al L edge (λ > 17.1 nm), aluminum provides for higher theoretical peak reflectance since it is less absorbing than silicon. The question about aluminum was a technological feasibility of high-reflecting and stable multilayers containing this material, which is known for its chemical reactivity with oxygen and other materials as well as for high roughness of films obtained during the growth as a result of crystallization.…”
Section: Tri-component Al-based Multilayers For Euvmentioning
confidence: 99%