Physics
Scientific paper
Apr 1993
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993jats...50.1122s&link_type=abstract
Journal of the Atmospheric Sciences (ISSN 0022-4928), vol. 50, no. 8, p. 1122-1132.
Physics
13
Radiant Flux Density, Solar Flux Density, Solar Radiation, Solar Terrestrial Interactions, Water Vapor, Aerosols, Atmospheric Attenuation, Cloud Physics
Scientific paper
This paper presents model calculations of the influence on solar absorption of water vapor, solar zenith angle, cloud-top altitude, and cloud optical thickness. The model results indicate a somewhat complex relation between the solar net fluxes at the surface and at the top of the atmosphere. It is pointed out that cloud altitude and optical depth have a large impact on solar atmospheric absorption; high clouds decrease solar absorption by the atmosphere whereas low clouds increase it. This difference between solar atmospheric absorption for low and high clouds increases with cloud optical depth. An intriguing result is that changes of total atmospheric absorption with cloud-top height are nearly completely compensated by corresponding changes in the net flux at the top of the atmosphere, thus leaving the surface solar net flux constant. Furthermore, this paper provides a very simple parameterization for estimating the clear-sky solar atmospheric absorption as a function of solar zenith angle and the vertically integrated water vapor content of the atmosphere.
No associations
LandOfFree
Relationship between solar net radiative fluxes at the top of the atmosphere and at the surface does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.
If you have personal experience with Relationship between solar net radiative fluxes at the top of the atmosphere and at the surface, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Relationship between solar net radiative fluxes at the top of the atmosphere and at the surface will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-1372516