Abstract
In X ray region, the supermirror can provide better optical performance than metal substrate or two-layer mirror. W/Si supermirrors are designed in 0.2–10 keV by block method. These mirrors have big grazing incidence angles of 1.0, 1.4, and 1.7 degrees, which is the most important characteristic in our job. Compared with two-layer mirror, our design provides a significant improvement of reflectance in 5–10 keV, and it also gives a good initial one for further optimization by other algorithms. Our job has a potential application in X ray astronomical imaging detection missions.
Sign-in/Register to access full text options 
Talk to us
Join us for a 30 min session where you can share your feedback and ask us any queries you have
Schedule a callMore From: Nuclear Instruments and Methods in Physics Research Section A: Accelerators, Spectrometers, Detectors and Associated Equipment
Disclaimer: All third-party content on this website/platform is and will remain the property of their respective owners and is provided on "as is" basis without any warranties, express or implied. Use of third-party content does not indicate any affiliation, sponsorship with or endorsement by them. Any references to third-party content is to identify the corresponding services and shall be considered fair use under The CopyrightLaw.
