Astronomy and Astrophysics – Astronomy
Scientific paper
Oct 1996
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1996spie.2808..284a&link_type=abstract
Proc. SPIE Vol. 2808, p. 284-288, EUV, X-Ray, and Gamma-Ray Instrumentation for Astronomy VII, Oswald H. Siegmund; Mark A. Gummi
Astronomy and Astrophysics
Astronomy
Scientific paper
A novel form of thin-coated transparent polymer film undergoes a radiation-initiated solid-state polymerization reaction when irradiated with deep ultraviolet and x and gamma rays. It forms a permanent deep-blue high-resolution image, without the need for chemical, optical, or thermal processing. The increase in the optical density with absorbed dose, irradiance or photon fluence is a linear function with relatively high contrast and without appreciable reciprocity failure and has the same response in vacuum and in air. The sensor coating thickness on a polyester base is approximately 6 micrometer. It forms the radiation-induced image that can resolve 600 line pairs per millimeter. The ultraviolet sensitivity at 266 nm wavelength is such that the optical density produced by an irradiance of 30 mJ/cm2 is approximately 1.00 at the wavelength maximum of the absorption spectrum (670 nm). UV, low-energy x-ray (10 keV) and gamma-ray (660 keV) response characteristics are presented, which demonstrate the ability to evaluate and map radiation image distributions quantitatively. The films are useful to calibrate beam profiles, including the penumbra shapes, because of the wide dynamic range and linear response.
Al-Sheikhly Mohamad
Christou Aristos
Christou Chris A.
McLaughlin William L.
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