Physics
Scientific paper
Sep 1988
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988soph..116..391a&link_type=abstract
Solar Physics (ISSN 0038-0938), vol. 116, no. 2, 1988, p. 391-399. CAICYT-supported research.
Physics
6
Astronomical Photometry, Diurnal Variations, Irradiance, Solar Oscillations, Annual Variations, Attenuation Coefficients, Photometers, Solar Terrestrial Interactions
Scientific paper
Monochromatic extinction coefficients at four wavelengths have been obtained over a period of more than two years at the Observatorio del Teide (Izaña Tenerife) using a full disc, direct sunlight, quadruple photometer devoted to the detection of integral luminosity oscillations of the Sun. The mean extinction coefficients (0.13 at 500 nm) show a seasonal variation of about 15%, the best atmospheric conditions being in winter and autumn. Moreover, in anyone day the extinction coefficient in the afternoon is always lower than the one in the morning by ≡7%. A one-year period fluctuation, with an amplitude of ≡0.035 mag, has been identified in the instrumental magnitudes outside the atmosphere, and is interpreted as the variation produced by the different Sun-Earth distance from winter to summer.
Andersen B.
Domingo Vicente
Jimenez Arturo
Jones Allan
Korzennik Sylvain
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