Spectrometers for the solar patrol of extreme ultraviolet and soft x-ray radiation

Details Spectrometers for the solar patrol of extreme ultraviolet and soft x-ray radiation Spectrometers for the solar patrol of extreme ultraviolet and soft x-ray radiation

Jul 1997

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1997spie.3113..404a&link_type=abstract

Proc. SPIE Vol. 3113, p. 404-410, Grazing Incidence and Multilayer X-Ray Optical Systems, Richard B. Hoover; Arthur B. Walker; E

Computer Science

Scientific paper

The variations of the intensity and spectral distribution of the EUV and x-ray solar fluxes from the whole disk in the wavelength range 0.1 - 134 nm are the main reason of changes in all upper atmospheric and ionospheric parameters and one of the principal factors in the solar-terrestrial relation changes. However the permanent monitoring of the solar EUV and soft x-ray radiation (0.8 - 120 nm) is absent at present. In this paper the recent advances in the elaboration of the topical-electronic apparatus complex for the permanent space patrol of EUV and soft x-ray solar radiation are discussed and optical schemes of solar spectrometers of grazing and normal incidence with diffraction gratings and also their energetic characteristics are presented.

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