Solar spectroscopy in the far-ultraviolet-X-ray wavelength regions - Status and prospects

Details Solar spectroscopy in the far-ultraviolet-X-ray wavelength regions - Status and prospects Solar spectroscopy in the far-ultraviolet-X-ray wavelength regions - Status and prospects

Oct 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988josab...5.2237f&link_type=abstract

Optical Society of America, Journal, B: Optical Physics (ISSN 0740-3224), vol. 5, Oct. 1988, p. 2237-2251. NASA-supported resear

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21

Extreme Ultraviolet Radiation, Far Ultraviolet Radiation, Solar Atmosphere, Solar Spectra, X Ray Spectra, Bragg Angle, Line Spectra, Rocket Sounding, Satellite Imagery, Solar Instruments

Scientific paper

The authors review the status and prospects of solar spectroscopy in the far-UV - X-ray wavelength regions between approximately 1.7 and 2000 Å. They divide the solar spectrum into a number of wavelength regions, determined by characteristics of spectroscopic instrumentation. The quality of the available spectra obtained in each region is discussed, concentrating on spectral resolution, wavelength coverage and accuracy, and line intensity and line-profile information.

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