Abstract
Since 1993 it is known that there is a good correlation between the scintillation in the solar irradiance and solar image quality (Seykora, 1993). This effect is now being used in a number of experiments to evaluate solar image quality and to measure site seeing. In this paper we explore further the calibration of this scintillation (σI) in terms of the Fried parameter (r0) taking into account variations in the refractive index structure constant C 2N with height (h), zenith distance (ζ) dependence and the effects of wind velocities. A variant in the scintillometer setup is proposed which decreases sharply the dependance on C 2N , ζ, and the wind velocities. It uses an array of scintillometers. The same array can be used to measure theC 2N profile with height. Some preliminary results of the calibration of current NSO site survey measurements are presented.
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Beckers, J.M., Leon, E., Mason, J. et al. Solar Scintillometry: Calibration of Signals and its Use for Seeing Measurements. Solar Physics 176, 23–36 (1997). https://doi.org/10.1023/A:1004988028580
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DOI: https://doi.org/10.1023/A:1004988028580