Translator Disclaimer
1 September 1995 Shielding simulations for the Advanced X-Ray Astrophysics Facility (AXAF)
Author Affiliations +
The Advanced X ray Astrophysics Facility (AXAF) contains two focal-plane science instruments -- the microchannel-plate high-resolution camera (HRC) and the AXAF CCD imaging spectrometer (ACIS). Each of these instruments provides two low-internal- background detectors, one for imaging and the other for reading out AXAF's objective transmission gratings. Taking maximum advantage of the low internal background of these instruments requires shielding against external electromagnetic and particle radiation. To optimize the shielding within weight constraints, we performed extensive numerical simulations of the photon transport and of the particle transport and activation within the AXAF. We discuss the simulations and report the results of the shielding study. With the adopted shielding design, the particle-induced background and the x-ray-induced background are each comparable to or less than the anticipated internal background of AXAF's imaging detectors (HRC and ACIS). Thus, the predicted total non-imaged background is very low -- less than 0.2 counts arcsec-2 day-1 for the HRC and even lower for the ACIS half-arcsec angular resolution, this low background has negligible effect upon point-source detection, for reasonable observation durations.
© (1995) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Kurtis L. Dietz, Ronald F. Elsner, Marshall K. Joy, Stephen L. O'Dell, Brian D. Ramsey, Martin C. Weisskopf, Anthony W. Armstrong, Bonnie L. Colborn, and Nina Kanvec "Shielding simulations for the Advanced X-Ray Astrophysics Facility (AXAF)", Proc. SPIE 2518, EUV, X-Ray, and Gamma-Ray Instrumentation for Astronomy VI, (1 September 1995);


HEXIT SAT a mission concept for x ray grazing...
Proceedings of SPIE (October 11 2004)
X-ray evolving universe spectroscopy mission (XEUS)
Proceedings of SPIE (September 29 1999)
New x-ray telescope mission (NeXT)
Proceedings of SPIE (October 11 2004)
The SWIFT Gamma-Ray Burst Observatory
Proceedings of SPIE (October 11 2004)

Back to Top