Abstract

Measurements of the direct solar and diffuse sky irradiances are used for deriving optical and physical features of the atmospheric aerosols: optical depth, size distribution, and complex refractive index. Sky irradiance is measured by means of a sky-radiometer (aureolemeter), which consists essentially of a photometer with annexed interferential filters for the selection of the wavelengths at which to operate, and a pointing system. The device used in the authors' research program, manufactured by the Japanese Company Prede (Tokyo), operates at the following wavelengths: 0.315, 0.400, 0.500, 0.870, 0.940 and 1.040 /spl mu/m. Measurements are undertaken in the two following different ways. Almucantar: pointing along a conical surface with the same zenith angle of the Sun. Principal plane, the instrument aims the sky along a plane with the same azimuth angle of the Sun. The two quantities considered in their scheme of data elaboration are the direct solar irradiance V and the ratio R between the diffuse and the direct irradiance.

Full Text
Published version (Free)

Talk to us

Join us for a 30 min session where you can share your feedback and ask us any queries you have

Schedule a call