Paper
1 October 1990 Polarization analysis of the advanced x-ray astrophysical facility telescope assembly
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Abstract
The Advanced X-ray Astrophysical Facility (AXAF) telescope consists of six concentric paraboloid-hyperboloid pairs of mirrors operating near grazing incidence. Because of the substantial polarization effects at large angles of incidence, there is concern about the feasibility of polarimetry near the focal plane. The primary mirror acts as a tangentially directed half-wave linear retarder and nearly completely depolarizes the linearly polarized component of the light. The secondary mirror introduces an additional half wave of linear retardance. The tangentially directed one-wave linear retarder leaves the transmitted beam in the incident polarization state. The net instrumental polarization effects are small, and polarimetry is feasible with the AXAF.
© (1990) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Daniel M. Brown and Russell A. Chipman "Polarization analysis of the advanced x-ray astrophysical facility telescope assembly", Proc. SPIE 1317, Polarimetry: Radar, Infrared, Visible, Ultraviolet, and X-Ray, (1 October 1990); https://doi.org/10.1117/12.22075
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KEYWORDS
Polarization

Mirrors

Telescopes

X-rays

Polarimetry

Infrared radiation

Radar

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