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Proceedings Paper

Advances In Photographic X-Ray Imaging For Solar Astronomy
Author(s): D. Moses; R. Schueller; K. Waljeski; J. M. Davis
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Paper Abstract

The technique of obtaining quantitative data from high resolution soft X-ray photographic images produced by grazing incidence optics was successfully developed to a high degree during the AS&E Solar Research Sounding Rocket Program and the S-054 X-Ray Spectrographic Telescope Experiment Program on Skylab. Continued use of soft X-ray photographic imaging in sounding rocket flights of the AS&E High Resolution Solar Soft X-Ray Imaging Payload has provided opportunities to further develop these techniques. The developments discussed include: (1) The calibration and use of an inexpensive, commercially available microprocessor controlled drum type film processor for photometric film development. (2) The use of Kodak Techni-cal Pan 2415 film and Kodak SO-253 High Speed Holographic film for improved resolu-tion. (3) The application of a technique described by Cook, Ewing, and Sutton(1) for determining the film characteristics curves from density histograms of the flight film. Although the superior sensitivity, noise level, and linearity of microchannel plate and CCD detectors attracts the development efforts of many groups working in soft X-ray imaging, the high spatial resolution and dynamic range as well as the reliability and ease of application of photographic media assures the continued use of these techniques in solar X-ray astronomy observations.

Paper Details

Date Published: 27 November 1989
PDF: 14 pages
Proc. SPIE 1159, EUV, X-Ray, and Gamma-Ray Instrumentation for Astronomy and Atomic Physics, (27 November 1989); doi: 10.1117/12.962610
Show Author Affiliations
D. Moses, American Science and Engineering, Inc. (United States)
R. Schueller, American Science and Engineering, Inc. (United States)
K. Waljeski, Brandeis University (United States)
J. M. Davis, NASA, Marshall Space Flight Center (United States)

Published in SPIE Proceedings Vol. 1159:
EUV, X-Ray, and Gamma-Ray Instrumentation for Astronomy and Atomic Physics
Charles J. Hailey; Oswald H. W. Siegmund, Editor(s)

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