Absolute, Extreme-Ultraviolet Solar Spectral Irradiance Monitor (AESSIM)

Details Absolute, Extreme-Ultraviolet Solar Spectral Irradiance Monitor (AESSIM) Absolute, Extreme-Ultraviolet Solar Spectral Irradiance Monitor (AESSIM)

Nov 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992hco..rept.....p&link_type=abstract

Annual Report, 15 Nov. 1991 - 14 Nov. 1992 Harvard Coll. Observatory, Cambridge, MA.

Physics

Extreme Ultraviolet Radiation, Gas Ionization, Radiometers, Solar Radiation, Thin Films, Calibrating, Radiance, Rare Gases, Solar Spectra, Ultraviolet Spectra

Scientific paper

The goal of this research program is development of a method for obtaining daily, radiometrically accurate, solar spectral irradiance data at extreme-ultraviolet (EUV) wavelengths. In-orbit radiometric instrumentation recalibration is a fundamental requirement for such measurements. It was proposed to investigate, design, and test smaller and less massive, low power, in-space version of a 'standard' EUV radiance source, which was developed for laboratory use and to assess the merits of innovative combinations of rare-gas ionization cells and thin film filters to make absolute measurements of EUV radiation over a number of wavelength bands.

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