Wide field-of-view Hadamard X-ray spectrometer

Details Wide field-of-view Hadamard X-ray spectrometer Wide field-of-view Hadamard X-ray spectrometer

Dec 1977

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1977ssi.....3..483m&link_type=abstract

Space Science Instrumentation, vol. 3, Dec. 1977, p. 483-489.

Mathematics

1

Signal To Noise Ratios, Transformations (Mathematics), X Ray Sources, X Ray Spectroscopy, Bragg Angle, Crystals, Line Spectra, Masking, X Ray Telescopes

Scientific paper

A new type of spectrometer consisting of a flat Bragg crystal and a Hadamard transform X-ray telescope is described. It has a wide field of view and is suitable to observe line spectrum features of widely extended X-ray sources. The signal to noise ratio advantage of this spectrometer is almost the same as that of the curved Bragg crystal spectrometer proposed by Borken and Kraushaar, but its wave length resolution and spatial resolution are better than for the curved crystal spectrometer.

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