LOGIN TO YOUR ACCOUNT

Username
Password
Remember Me
Or use your Academic/Social account:

CREATE AN ACCOUNT

Or use your Academic/Social account:

Congratulations!

You have just completed your registration at OpenAire.

Before you can login to the site, you will need to activate your account. An e-mail will be sent to you with the proper instructions.

Important!

Please note that this site is currently undergoing Beta testing.
Any new content you create is not guaranteed to be present to the final version of the site upon release.

Thank you for your patience,
OpenAire Dev Team.

Close This Message

CREATE AN ACCOUNT

Name:
Username:
Password:
Verify Password:
E-mail:
Verify E-mail:
*All Fields Are Required.
Please Verify You Are Human:
fbtwitterlinkedinvimeoflicker grey 14rssslideshare1
Eiden, Reiner (2011)
Publisher: Co-Action Publishing
Journal: Tellus A
Languages: English
Types: Article
Subjects:
The application of the theory of primary scattering to describe and interpret the spectral distribution of the sky radiance is discussed. It is shown that within the solar aureole the influence of the scattering of higher order can be neglected. Theoretical calculations of the spectral distribution of the sky radiance, carried out by Bullrich et al. (1965) based on an exponential aerosol size distribution with an upper limiting particle radius r = 10 ?, have been extended to r = 150 ?. The detailed study of the influence of these “giant” particles revealed that aerosol particles of r >30 ? have no effect on the sky radiation any more. Representative measurements taken at Mainz, Germany, at the research station Jungfraujoch in the High Alps, Switzerland, and on the island of Maui, Hawaii, are analyzed and interpreted by comparison with theoretical values. Some measurements required a modification of the basic model of the turbid atmosphere. The exponent of the aerosol size distribution generally a constant has to be considered a function of the particle size. Furthermore, the exponent of the aerosol size distribution was found to be a function of height at least in case of subsidence. The exponent increases with height.DOI: 10.1111/j.2153-3490.1968.tb00379.x
  • The results below are discovered through our pilot algorithms. Let us know how we are doing!

    • de Bary, E. 1964. Influence of multiple scattering on the intensity and polarization of diffuse sky radiation. Appl. Optics 3, 1293-1303.
    • de Bary, E., Braun, B. & Bullrich, K. 1965. Tables Related to Light Scattering i n a Turbid Atmopshere, vol. 1-111. Air Force Cambridge Research Lab. Special Rept. No. 33.
    • Bullrich, K., de Bary, E. & Moller, F. 1952. Die Farbe des Himmels. Beofis. Pura Appl. 23, 66-110.
    • Bullrich, K . & Eiden, R. 1964. Optical transmission of the atmosphere in Hawaii. Final technical report. Contract DA-91-EUC-2964.
    • Bullrich, K., Eiden, R., Jaenicke, R. & Nowak, W. 1966. Optical transmission of the atmosphere in Hawaii. 11. Final technical report. Contract DA-91-591-EUC-3458. QeofiS. Pura Appl. I n press.
    • Bugnolo, D S. 1960. On the question of multiple scattering in the troposphere. J. of Qeophys. Rw. 65, 879-884.
    • Coulson, K., Dave, J. & Sekera, 2. 1960. Tables Related to Radiation from a Planetary Atm. with Rayleigh Scattering. Univ. of Calif. Press, Berkeley, Los Angeles.
    • Coulson, K. L., Bouricius, G. M. &Gray, E. L. 1965. Optical reflection properties of natural surfaces. J . of aeophys. Rw. 80, No. 18, 460-4611.
    • Danzer, K. & Bullrich, K. 1966. Calculations of the influence of aerosolparticles with certain intervals of radii on the scattering coefficient and the sky radiance. Optik 24, 577-594.
    • Deirmendjian, D. 1959. Theory of the solar aureole (part 11).Ann. de Qeophys. 15, No. 2, 218-249.
    • Dirmhirn, I. 1964. Das Strahlungsfeld irn Lebensraum. Akademische Verlagsgesellschaft, Frankfurt/Main.
    • Eiden, R. 1966. The elliptical polarization of light scattered by a volume of atmospheric air. Appl. Optics 5, 569-575.
    • Eiden, R. 1966. Messungen und Berechnungen der spektralen sonnennahen Himmelsstrahlung mit Hilfe neuer experimenteller und theoretischer Methoden. Dissertation. Mainz.
    • Giinther, S. 1949. Die Himmelshelligkeit in der Nahe der Sonne. Optik 5, 240-257.
    • Hanel, G . 1967. Vorbereitende Studien zur Messung des Brechungsindex atmospharischer Aerosolteilchen mit vorlaufigen Messergebnissen des Realteils bei verschiedenen relativen Luftfeuchtigkeiten. Diplomarbeit. Mainz.
    • van de Hulst, H. C. 1957. Light Scattering by Small Particles. John Wiley and Sons,New York.
    • Jaenicke, R. & Junge, Chr. 1966. Studien zur oberen Grenzgrosse des natiirlichen Aerosols. Beitr. Phya. Atmos. I n press.
    • Junge, Chr. E. 1952. Gesetzmassigkeiten in der Grossenverteilung atmospharischer Aerosole iiber dem Kontinent. Ber. Dtsch. Wetterdienst U.S. Zone, No. 35, pp. 261-276.
    • Junge, Chr. E. 1963. Air Chemistry and Radioactivity. Academic Press, New York and London.
    • Kasten, F. 1962. Sichtweite und Albedo, insbesondere irn Polargebiet. 11. Beitr. Phys. Atm. 35, 18-42.
    • Middleton, W. E. K. & Mungall, A. G. 1952. The luminous directional reflectance of snow. J. of Opt. SOC4.2, No. 8, 572-579.
    • Mie, G. 1908. Beitrage zur Optik triiber Medien. Ann. Phs. 25, 377-445.
    • Moller, F., de Bary, E. & Bullrich, K. 1954. Beitrage zur Erklarung von Himmelsfarbe und Helligkeit. 2. Meteor. 8, 303.
    • Newkirk, G. & Eddy, J. A. 1964. Light scattering by particles in the upper atmosphere. J . of Atm. Sciences 21, 35-60.
    • Robinson, E. 1962. Effects of air pollution on visivility. I n Air Pollution, vol. I. Hersg. A. C. Stern. Academic Press, New York and London.
    • Sekihara, K. & Murai, M. 1961. On the measurement of atmospheric extinction of solar radiation and the sun's aureole. Met. and Qeophys. 7 , 557-74.
    • Spankuch, D. 1965. uber den Einfluss der Dunstschichtung auf die Strahldichteverteilung des wolkenlosen Himmels. 2. Meteor. 17, 202-208.
    • Volz, F. 1954. Die Optik und Meteorologie der atmosphiirischen Triibung. Ber. Dtsch. Wetterdienstes, No. 13, vol. 2.
    • Volz, F. 1956. Optik des Dunstes. I n Handbuch der Qeophys., Vol. VIII. Berlin.
    • Volz, F. 1961. Photometer mit Selen-Photoelement zur spektralen Messung der Sonnenstrahlung und zur Bestimmung der Wellenlangenabhlingigkeit der Dunsttriibung. Arch. Met. Qeophys. Biokl. 10, 100.
  • No related research data.
  • No similar publications.

Share - Bookmark

Cite this article

Collected from