1951Papers in Meteorology and GeophysicsOpen access

Studies of the Distribution of the Ultraviolet Sky Radiation (II )

Kyo Sekihara

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Abstract

Regarding the calculation of the secondary scattering of the solar radiation from the clear sky, a modification of the theoretical formula of A. Hamm. ad and S. Chapman (Phil.. Mag.1939)was done considering the effect of polarization cansed by primary scattering. A quantitative treatment became possible by the new formula in the vicinity of the zenith, that is, in the range from 0° to 45° of the zenith angle.

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Regarding the calculation of the secondary scattering of the solar radiation from the clear sky, a modification of the theoretical formula of A. Hamm. ad and S. Chapman (Phil.. Mag.1939)was done considering the effect of polarization cansed by primary scattering. A quantitative treatment became possible by the new formula in the vicinity of the zenith, that is, in the range from 0° to 45° of the zenith angle.

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Available abstract

Regarding the calculation of the secondary scattering of the solar radiation from the clear sky, a modification of the theoretical formula of A. Hamm. ad and S. Chapman (Phil.. Mag.1939)was done considering the effect of polarization cansed by primary scattering. A quantitative treatment became possible by the new formula in the vicinity of the zenith, that is, in the range from 0° to 45° of the zenith angle.

Key concepts: Zenith, Sky, Diffuse sky radiation, Radiation, Polarization (electrochemistry), Scattering, Physics, Ultraviolet

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