File:Reflectivity angular spectrum at different wavelengths.png
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Reflectivity_angular_spectrum_at_different_wavelengths.png (568 × 311 pixels, file size: 28 KB, MIME type: image/png)
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[edit]DescriptionReflectivity angular spectrum at different wavelengths.png |
English: The measured EUV multilayer reflectance is shown above as a function of incident angle for 13.3-13.7 nm wavelength range.[1] ASML's NXE EUV tool's broadband spectrum reflectance is also shown as the dashed curve.[2] The incident angle is defined with respect to the normal to the multilayer surface. The EUV source output is mostly concentrated between 13.3 nm and 13.7 nm.[3] The reflectance integrated over the range of angles is also comparable for the wavelengths of this range, but the dropoff for larger angles is faster for the longer wavelengths.[1] This trend is expected from the condition of Bragg's law.[4][5] A change in the cosine of the incident angle on the order of 1/(# of layer periods) ~2-3% is sufficient to reduce the wavelength's reflectance significantly.[6][7] Inset: the impact of the angular dependence of reflectance on the wavelength distribution in the pupil, also known as apodization. The longest wavelengths are brighter at smaller angles, while the shortest wavelengths are brighter at larger angles. [8]
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Author | Guiding light |
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References
[edit]- ↑ a b http://www.eecs.berkeley.edu/Pubs/TechRpts/2013/EECS-2013-56.html R. Chao et al., Measurement and characterization of EUV mask performance at high-NA, EECS Department, Univ. of California, Berkeley Technical Report No. UCB/EECS-2013-56, 5/10/2013, Figure 5.
- ↑ N. Davydova et al., Proc. SPIE 8352, 835208 (2012).
- ↑ I. Fomenkov et al., Adv. Opt. Techn. 6, 173 (2017).
- ↑ F. Scholze et al., Proc. SPIE 6151, 615137 (2006).
- ↑ The Very Different Wavelengths of EUV Lithography
- ↑ D. Attwood, Soft X-rays and Extreme Ultraviolet Radiation: Principles and Applications, Cambridge University Press, 2000, Ch. 5.
- ↑ B. E. A. Salah and M. C. Teich, Fundamentals of Photonics, Wiley, 1991, p. 805ff.
- ↑ J. Ruoff, Proc. SPIE 7823, 78231N (2010).
File history
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Date/Time | Thumbnail | Dimensions | User | Comment | |
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current | 12:25, 20 August 2019 | 568 × 311 (28 KB) | Guiding light (talk | contribs) | larger fonts | |
12:22, 20 August 2019 | 568 × 311 (27 KB) | Guiding light (talk | contribs) | clearer labels of shortest and longest wavelength zones | ||
12:35, 19 August 2019 | 569 × 311 (26 KB) | Guiding light (talk | contribs) | Added inset for wavelength distribution in pupil | ||
15:32, 31 July 2019 | 569 × 311 (26 KB) | Guiding light (talk | contribs) | enlarged graph | ||
14:56, 31 July 2019 | 566 × 309 (20 KB) | Guiding light (talk | contribs) | The actual spectrum's reflectance is added as dashed curve. | ||
06:28, 20 July 2019 | 762 × 454 (97 KB) | Guiding light (talk | contribs) | Remove inset | ||
06:23, 20 July 2019 | 761 × 454 (110 KB) | Guiding light (talk | contribs) | Show individual wavelengths only; effective illumination for 13.55 nm only. | ||
14:46, 19 July 2019 | 711 × 422 (97 KB) | Guiding light (talk | contribs) | weighted average corrected | ||
20:17, 18 July 2019 | 746 × 446 (109 KB) | Guiding light (talk | contribs) | "weighted average" changed to "weighted sum" the correct term | ||
11:58, 18 July 2019 | 758 × 452 (110 KB) | Guiding light (talk | contribs) | corrected weighted average |
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