Physics
Scientific paper
Aug 1976
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1976ssi.....2..289t&link_type=abstract
(Science Research Council, Symposium on the Techniques of Solar and Cosmic X-Ray Spectroscopy, Dorking, Surrey, England, May 22,
Physics
Far Ultraviolet Radiation, Solar Instruments, Ultraviolet Spectroscopy, X Ray Spectroscopy, Channel Multipliers, Chromosphere, Grazing Incidence Telescopes, Photomultiplier Tubes, Plasma Diagnostics, Solar Spectra, Spectroheliographs
Scientific paper
The solar extreme ultraviolet and soft X-ray (XUV) spectrum at wavelengths between 20 and 300 A contains a wealth of emission lines from ions formed at temperatures from 10 to the 5th K to greater than 2 x 10 to the 7th K. The requirements for high resolution spectrophotometric instrumentation are discussed in the light of data obtained with extreme ultraviolet and X-ray telescopes flown on Skylab. The design of a grazing-incidence spectroheliometer for active region and flare studies over the wavelength range from 40 to 630 A is presented and recently developed high-efficiency detectors and detector-arrays for use at XUV wavelengths are described.
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