A simple model for computing the spectral radiance of clear skies

A simple model for computing the spectral radiance of clear skies

From standard and observed atmospheric profiles, the spectral sky radiance is computed on the basis of the Lowtran-6 numerical code. Then, a simple model for its calculation is built, based on Bliss—Kondrat'yev theoretical considerations. Some comparisons of spectral sky radiances are shown. At...

Ausführliche Beschreibung

Gespeichert in:
Bibliographische Detailangaben
Veröffentlicht in:Solar energy 1988, Vol.40 (4), p.321-333
1. Verfasser: Berger, X.
Format: Artikel
Sprache:eng
Schlagworte:
Earth, ocean, space
Exact sciences and technology
External geophysics
Meteorology
Radiative transfer. Solar radiation
Online-Zugang:Volltext
Tags: Tag hinzufügen
Keine Tags, Fügen Sie den ersten Tag hinzu!
Beschreibung
Zusammenfassung:From standard and observed atmospheric profiles, the spectral sky radiance is computed on the basis of the Lowtran-6 numerical code. Then, a simple model for its calculation is built, based on Bliss—Kondrat'yev theoretical considerations. Some comparisons of spectral sky radiances are shown. At last, the total sky emissivity ϵ is obtained, and the function ϵ = f( t dew) is discussed, where t dew is the dewpoint temperature.
ISSN:0038-092X
1471-1257
DOI:10.1016/0038-092X(88)90005-9