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References

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  1. X. Mie, Am. Phys. 4, 377 (1908).
  2. S. Chandrasekhar, Radiative Transfer (Clarendon Press, Oxford, 1950).
  3. K. Sekihara, WMO Technical Note 104, Proceedings of WMO/IUGG Symposium, Bergen, Norway (1968).
  4. D. Deirmendjian, Electromagnetic Scattering on Spherical Polydispersions (Elsevier, New York, 1969).
  5. G. W. Kattawar, G. N. Plass, Appl. Opt. 7, 869 (1968).
    [CrossRef] [PubMed]
  6. G. W. Kattawar, G. N. Plass, Appl. Opt. 8, 1169 (1969).
    [CrossRef] [PubMed]
  7. H. Grassl, Contrib. Atmos. Phys. 43, 255 (1970).

1970

H. Grassl, Contrib. Atmos. Phys. 43, 255 (1970).

1969

1968

1908

X. Mie, Am. Phys. 4, 377 (1908).

Chandrasekhar, S.

S. Chandrasekhar, Radiative Transfer (Clarendon Press, Oxford, 1950).

Deirmendjian, D.

D. Deirmendjian, Electromagnetic Scattering on Spherical Polydispersions (Elsevier, New York, 1969).

Grassl, H.

H. Grassl, Contrib. Atmos. Phys. 43, 255 (1970).

Kattawar, G. W.

Mie, X.

X. Mie, Am. Phys. 4, 377 (1908).

Plass, G. N.

Sekihara, K.

K. Sekihara, WMO Technical Note 104, Proceedings of WMO/IUGG Symposium, Bergen, Norway (1968).

Am. Phys.

X. Mie, Am. Phys. 4, 377 (1908).

Appl. Opt.

Contrib. Atmos. Phys.

H. Grassl, Contrib. Atmos. Phys. 43, 255 (1970).

Other

S. Chandrasekhar, Radiative Transfer (Clarendon Press, Oxford, 1950).

K. Sekihara, WMO Technical Note 104, Proceedings of WMO/IUGG Symposium, Bergen, Norway (1968).

D. Deirmendjian, Electromagnetic Scattering on Spherical Polydispersions (Elsevier, New York, 1969).

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Figures (2)

Fig. 1
Fig. 1

Circumsolar radiation in percent of incoming radiation for different aerosol types at an optical depth of 1.0 and 0.45-μ wavelength. Dashed curves show the results for a point source. For comparison, values for a cumulus cloud are included.

Fig. 2
Fig. 2

Contribution of scattered radiation to the measured signals of direct solar radiation. The symbols are explained within the text.

Tables (1)

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Table I Circumsolar Radiation in Percent of Incoming Radiation at the Top of the Atmosphere

Equations (2)

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Haze C :             n ( r ) = 4.97 · 10 6 · r 2 · exp ( - 15.1186 r ) , Haze M :             n ( r ) = 5.33 · 10 4 · r · exp ( - 8.944 r ) .
C n = i = 1 m P i P · Q · α i · Δ φ i .

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