Abstract
The contribution from correction ΔT to the brightness temperature of hydrometeor formations that arises owing to the effect of multiple scattering of radio waves is investigated as a function of thickness s of the hydrometeor layer, zenith observation angle Θ, and scattering properties of the medium. The calculations are performed with the use of a radiophysical precipitation model developed earlier. It is shown that dependence ΔT(s) has a peak and that ΔT depends weakly on Θ in the angular range 0°–50° and increases with the parameter characterizing backward scattering.
Talk to us
Join us for a 30 min session where you can share your feedback and ask us any queries you have
Schedule a callMore From: Journal of Communications Technology and Electronics
Disclaimer: All third-party content on this website/platform is and will remain the property of their respective owners and is provided on "as is" basis without any warranties, express or implied. Use of third-party content does not indicate any affiliation, sponsorship with or endorsement by them. Any references to third-party content is to identify the corresponding services and shall be considered fair use under The CopyrightLaw.
