Other
Scientific paper
Nov 1992
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992georl..19.2203l&link_type=abstract
Geophysical Research Letters (ISSN 0094-8276), vol. 19, no. 22, p. 2203-2206.
Other
25
Irradiance, Solar Activity Effects, Solar Cycles, Solar Flux, Solar Spectra, Ultraviolet Spectra, Ultraviolet Spectroscopy, Upper Atmosphere Research Satellite (Uars), Variability
Scientific paper
Since October 1991, the Solar Ultraviolet Spectral Irradiance Monitor on board the Upper Atmosphere Research Satellite has been measuring the solar spectral irradiance from 120 to 400 nm with low (5 nm) and moderate (1.1 nm) resolution on a daily basis. By scaling the modulation measured over four solar rotations to proxy indicators of solar activity, we estimate the amplitude of the solar ultraviolet irradiance variation during the 11-year activity cycle, extending the wavelength coverage of existing empirical variability models to 120 nm and distinguishing the variability of the emission lines from that of the underlying solar continuum. These estimates are compared with results from another empirical variability model and from direct measurements.
Brueckner Guenter
Edlow Kenneth
Floyd Linton
Lean Judith
Prinz Dianne
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