Intensity statistics of the solar spectrum

Details Intensity statistics of the solar spectrum Intensity statistics of the solar spectrum

Aug 1976

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1976azh....53..827i&link_type=abstract

Astronomicheskii Zhurnal, vol. 53, July-Aug. 1976, p. 827-830. In Russian.

Astronomy and Astrophysics

Astronomy

Line Spectra, Solar Flux Density, Solar Spectra, Spectral Line Width, Far Ultraviolet Radiation, Limb Darkening, Long Wave Radiation, Luminous Intensity, Optical Density, Random Processes, Short Wave Radiation, Spectrum Analysis, Statistical Distributions, Sun, Ultraviolet Spectra

Scientific paper

The paper considers the intensity of the solar optical line spectrum to be a random function of wavelength, assuming the function to be stationary within a spectral region of about 100 A. Single point distribution functions of this random function are examined, and it is shown that the dispersion of fluctuations of spectral intensity in the center of the solar disk decreases smoothly from the short to long wave (from violet to red) regions of the spectrum. Intensity fluctuations also strongly decrease from the center to the limb.

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