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Volumn 5193, Issue , 2004, Pages 191-203

A Comparison of Uranium Oxide and Nickel as Single-layer Reflectors from 2.7 to 11.6 Nanometers

Author keywords

EUV; EUV soft X ray astronomy; Low angle reflector; Nickel; Soft x ray; Synchrotron; Uranium oxide

Indexed keywords

ASTRONOMY; EVAPORATION; MAGNETRONS; MATHEMATICAL MODELS; MIRRORS; NICKEL; REFLECTION; REFRACTIVE INDEX; THIN FILMS; X RAYS;

EID: 1942453812     PISSN: 0277786X     EISSN: None     Source Type: Conference Proceeding    
DOI: 10.1117/12.523478     Document Type: Conference Paper
Times cited : (8)

References (22)
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    • David D. Allred, Matthew B. Squires, R. Steven Turley, Webster Cash, and Ann Shipley, "Highly Reflective Uranium Mirrors for Astrophysics Applications," in X-ray Mirrors, Crystals and Multilayers, Andreas K. Freund, Albert T. Macrander, Tetsuya Ishikawa, and James. T. Wood, Editors, Proc. SPIE 4782, pp. 212-223, SPIE, Bellingham, WA, 2002.
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    • The curves for these plots were computed at the CXRO website http://www-cxro.lbl.gov/optical_constants/mirror2.html (June-July, 2003) using the option "thick mirrors", that is, single surface mirrors with zero surface roughness. The refractive indices, which are needed for the calculation, were calculated using the atomic scattering factor model using densities which we supplied the program. We used the CRC Handbook of Chemistry and Physics for densities. That is, there was no effort made to obtain the actual densities of the films. Densities: David R. Lide, Ed., CRC Handbook of Chemistry and Physics, 71st edition, CRC Press. Boca Raton, 1990-91
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* 이 정보는 Elsevier사의 SCOPUS DB에서 KISTI가 분석하여 추출한 것입니다.