A high resolution solar atlas for fluorescence calculations

Details A high resolution solar atlas for fluorescence calculations A high resolution solar atlas for fluorescence calculations

Jul 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983stin...8420465h&link_type=abstract

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Physics

Fluorescence, High Resolution, Irradiance, Line Spectra, Solar Spectra, Spectral Resolution, Sun, Calibrating, Correlation, Errors, Tables (Data), Ultraviolet Spectra, Variability, Wavelengths

Scientific paper

The characteristics required of a solar atlas to be used for studying the fluorescence process in comets are examined. Several sources of low resolution data were combined to provide an absolutely calibrated spectrum from 2250 A to 7000A. Three different sources of high resolution data were also used to cover this same spectral range. The low resolution data were then used to put each high resolution spectrum on an absolute scale. The three high resolution spectra were then combined in their overlap regions to produce a single, absolutely calibrated high resolution spectrum over the entire spectral range.

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