Performance characterization of hard X-ray imaging instruments at synchrotron radiation facility SPring-8

Yasushi Ogasaka, Keisuke Tamura, Ryo Shibata, Akihiro Furuzawa, Tomokazu Nakamura, Masataka Naitou, Takuya Miyazawa, Kenta Shimoda, Katsuhiko Onishi, Yoshihiro Fukaya, Tomonaga Iwahara, Yasushi Kanou, Hideyo Kunieda, Koujun Yamashita, Emi Miyata, Kenji Mukai, Kazuhiro Ikegami, Michihiko Aono, Hiroshi Tsunemi, Kentaro UesugiYoshio Suzuki

Research output: Chapter in Book/Report/Conference proceedingConference contribution

1 Citation (Scopus)

Abstract

The relevance of pre-flight calibration of space-born instruments is widely recognized. As an energy region of interest shifts to hard X-rays in these years, measurement setup becomes difficult to be afforded or maintained by a laboratory- or small-collaboration-based resources. In 10 to 100 keV region X-ray source that is bright and monochromatic enough to calibrate optics in detail is no longer available other than at synchrotron facility. Focal length becomes longer and this is another aspect that is beyond capabilities of soft-X-ray-oriented facilities. The hard X-ray instruments for balloon program have been characterized at synchrotron facility SPring-8/BL20B2 in Japan. SPring-8 is one of the world's brightest third generation synchrotron radiation facility. BL20B2 is specialized for medical and imaging experiment, and has 200m-long transport tube. Measurement at BL20B2 has great advantages such as extremely high flux, large sized and less divergent beam, and monochromatic beam covering entire hard X-ray region from 8 to 120keV. 16m-long experiment hutch is capable of long focal length of hard X-ray telescope. Pt/C multilayer-supermirror hard X-ray telescopes, position-sensitive scintillation counter and scintillator-deposited CCD, have been characterized at the facility. Instrumentation of the facility and some of measurement results are presented.

Original languageEnglish
Title of host publicationSpace Telescopes and Instrumentation II
Subtitle of host publicationUltraviolet to Gamma Ray
DOIs
Publication statusPublished - 2006
EventSpace Telescopes and Instrumentation II: Ultraviolet to Gamma Ray - Orlando, FL, United States
Duration: 24-05-200631-05-2006

Publication series

NameProceedings of SPIE - The International Society for Optical Engineering
Volume6266 II
ISSN (Print)0277-786X

Other

OtherSpace Telescopes and Instrumentation II: Ultraviolet to Gamma Ray
CountryUnited States
CityOrlando, FL
Period24-05-0631-05-06

All Science Journal Classification (ASJC) codes

  • Electronic, Optical and Magnetic Materials
  • Condensed Matter Physics
  • Computer Science Applications
  • Applied Mathematics
  • Electrical and Electronic Engineering

Fingerprint Dive into the research topics of 'Performance characterization of hard X-ray imaging instruments at synchrotron radiation facility SPring-8'. Together they form a unique fingerprint.

  • Cite this

    Ogasaka, Y., Tamura, K., Shibata, R., Furuzawa, A., Nakamura, T., Naitou, M., Miyazawa, T., Shimoda, K., Onishi, K., Fukaya, Y., Iwahara, T., Kanou, Y., Kunieda, H., Yamashita, K., Miyata, E., Mukai, K., Ikegami, K., Aono, M., Tsunemi, H., ... Suzuki, Y. (2006). Performance characterization of hard X-ray imaging instruments at synchrotron radiation facility SPring-8. In Space Telescopes and Instrumentation II: Ultraviolet to Gamma Ray [62663T] (Proceedings of SPIE - The International Society for Optical Engineering; Vol. 6266 II). https://doi.org/10.1117/12.671232