Development of high throughput X-ray telescopes for X-ray imaging and dispersive spectrometers

Details Development of high throughput X-ray telescopes for X-ray imaging and dispersive spectrometers Development of high throughput X-ray telescopes for X-ray imaging and dispersive spectrometers

Aug 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986sao..rept.....g&link_type=abstract

Semiannual Report, 1 Jul. 1985 - 30 Jun. 1986 Smithsonian Astrophysical Observatory, Cambridge, MA.

Statistics

Methodology

Image Processing, Mirrors, Numerical Control, Spectrometers, Structural Design, X Ray Telescopes, All Sky Photography, Angular Resolution, Glass, Ray Tracing, Surface Finishing, Surface Properties

Scientific paper

During the past year the technical approach to the realization of a high throughput Kirkpatrick-Baez X-ray mirror became better defined in terms of construction methodology and factors which affect maximum size. More progress was made than anticipated in the area of automatic figure formation. However, effort to improve the resolution of float glass by simple techniques were not successful. Mirror development, spectroscopy, all sky telescope, and explorer concept studies are discussed.

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