W/SiC x-ray multilayers optimized for use above 100 keV

被引:42
作者
Windt, DL
Donguy, S
Hailey, CJ
Koglin, J
Honkimaki, V
Ziegler, E
Christensen, FE
Chen, H
Harrison, FA
Craig, WW
机构
[1] Columbia Astrophys Lab, New York, NY 10027 USA
[2] European Synchrotron Radiat Facil, F-38043 Grenoble, France
[3] Danish Space Res Inst, DK-2100 Copenhagen, Denmark
[4] CALTECH, Pasadena, CA 91125 USA
[5] Lawrence Livermore Natl Lab, Livermore, CA 94550 USA
关键词
D O I
10.1364/AO.42.002415
中图分类号
O43 [光学];
学科分类号
070207 ; 0803 ;
摘要
We have developed a new depth-graded multilayer system comprising W and SiC layers, suitable for use as hard x-ray reflective coatings operating in the energy range 100-200 keV. Grazing-incidence x-ray reflectance at E = 8 keV was used to characterize the interface widths, as well as the temporal and thermal stability in both periodic and depth-graded W/SiC structures, whereas synchrotron radiation was used to measure the hard x-ray reflectance of a depth-graded multilayer designed specifically for use in, the range Esimilar to150-170 keV. We have modeled the hard x-ray reflectance using newly derived optical constants, which we determined from reflectance versus incidence angle measurements also made using synchrotron radiation, in the range E = 120-180 keV. We describe our experimental investigation in detail, compare the new W/SiC multilayers with both W/Si and W/B4C films that have been studied previously, and discuss the significance of these results with regard to the eventual development of a hard x-ray nuclear line telescope. (C) 2003 Optical Society of America.
引用
收藏
页码:2415 / 2421
页数:7
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