Soft X-ray spectrographs for solar observations

Details Soft X-ray spectrographs for solar observations Soft X-ray spectrographs for solar observations

Jan 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988spie..982..299b&link_type=abstract

IN: X-ray instrumentation in astronomy II; Proceedings of the Meeting, San Diego, CA, Aug. 15-17, 1988 (A89-40276 17-35). Bellin

Physics

Atomic Physics

2

Gratings (Spectra), Solar Maximum Mission, Solar Observatories, X Ray Spectroscopy, Atomic Physics, Charge Coupled Devices

Scientific paper

Recent advances in soft X-ray spectrometery are reviewed, with emphasis on techniques for studying the windowless region from roughly 1-100 A. Recent technological developments considered include multilayer mirrors, large-format CCD detectors which are sensitive to X-rays, position-sensitive photon counting detectors, new kinds of X-ray films, and optical systems based on gratings with nonuniform ruling spacings. Improvements in the extent and accuracy of the atomic physics data sets on which the analysis of spectroscopic observatons depend are also discussed.

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