Published July 18, 2000
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X-ray multilayer coatings for use at energies above 100 keV
Abstract
We discuss the development of X-ray multilayer coatings for use as broad-band reflectors operating at energies above 100 keV. Such coatings can be used to produce hard X-ray telescopes that will make possible a variety of entirely new astronomical observations. We summarize our recent investigation into the growth, structure and hard X-ray performance of depth-graded W/Si multilayers, present follow-up information on Cu/Si multilayers, and discuss preliminary results obtained with Ni/Si, Ni._8Cr._2/Si, and Ni._(93)V._(07)/Si multilayers.
Additional Information
© 2000 Society of Photo-Optical Instrumentation Engineers (SPIE). The authors are grateful to E. Ziegler, V. Honkimaki, M. S. Del Rio, A. Souvorov, A. Freund, M. Ohler, and R. Hustache for their help and support in facilitating the high-energy reflectance measurements made at ESRF. This research was supported in part by NASA under grant no. NAG-5-5128, and by the U.S. Dept. of Energy, Office of Science, Laboratory Technology Division under contract DE-AC5-96OR22464 with Lockheed Martin Energy Research Corp. and contract DE-ACO5-760R00033 with Oak Ridge Associated Universities.Attached Files
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Additional details
- Eprint ID
- 84255
- Resolver ID
- CaltechAUTHORS:20180111-115315911
- NASA
- NAG-5-5128
- Department of Energy (DOE)
- DE-AC05-96OR22464
- Department of Energy (DOE)
- DE-ACO5-760OR00033
- Created
-
2018-01-11Created from EPrint's datestamp field
- Updated
-
2021-11-15Created from EPrint's last_modified field
- Caltech groups
- Space Radiation Laboratory
- Series Name
- Proceedings of SPIE
- Series Volume or Issue Number
- 4012