Physics
Scientific paper
Jan 1995
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1995em%26p...68..385k&link_type=abstract
Earth, Moon, and Planets, Volume 68, Issue 1-3, pp. 385-388
Physics
Scattering Of Shortwave Solar Radiation, Particle Size Distribution, Particle Refractive Index
Scientific paper
Interaction between planetary atmospheres and small bodies is connected with radiation effects. Submicron particles in the Earth's upper atmosphere strongly influence the scattering of the shortwave solar radiation. Based on the mutual connection between the environmental and radiation field structures it is possible to determine the physical characteristics of the particle set in this environment. Generaly, the diffused radiation field in the real atmosphere is given by a sum of elementary and multiple scattering components. Solving the inverse problems always leads to complicated integral equations. A major part of the diffused radiation field in the upper atmosphere is due to the first order scattering. The paper presents a new method for determination of the effective complex refractive index and size distribution of the particles based on the radiance data. The solution of integral equations is to be found in the space of quadratically integrable and continuous functionsf ∈L 2.
No associations
LandOfFree
Theory of Optical Identification of Submicron Particles in High Atmosphere 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 Theory of Optical Identification of Submicron Particles in High Atmosphere, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Theory of Optical Identification of Submicron Particles in High Atmosphere will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-1820637