Theory of Radio Transmission by Tropospheric Scattering Using Very Narrow Beams
- 1 March 1955
- journal article
- Published by Institute of Electrical and Electronics Engineers (IEEE) in Proceedings of the IRE
- Vol. 43 (3) , 281-290
- https://doi.org/10.1109/JRPROC.1955.278133
Abstract
Calculations have been made for communication over a 300-km path between antennas, each consisting of a paraboloid of diameter 100 λ. It is assumed that, under normal atmospheric conditions, transmission over this distance is due to scattering by atmospheric irregularities and that the scattering phenomena are described by the formula used by Booker and Gordon. Over this path, the effect of spread in the direction of arrival of scattered power should become noticeable for beamwidths less than about 1.5 degrees. For the 0.73 degree-beams assumed, spread in the angle of arrival should show up quite markedly for synchronized beam swinging-that is, when the beams at both transmitter and receiver are swung imultaneously so that their axes continue to intersect. When the beams are swung 1 degree to one side of the great circle path, the reduction in power received should be about 7 db, as compared with more than 40 db that would occur for propagation purely in the vertical plane containing trsmitter and receiver. Narrowing the antenna beams to very small values is an important key to increasing circuit radio-frequency bandwidth capability, although at the expense of increasing antenna "aperture-medium coupling loss" (so-called "gain loss"). For the assumed circuit average bandwidth should be about 6 mcp, the loss being of the order of 10 db. For beams much larger than 1.5 degrees, the bandwidth should be limited by the medium to about 3 mcp, with negligible loss.Keywords
This publication has 6 references indexed in Scilit:
- A statistical survey of atmospheric index-of-refraction variationTransactions of the IRE Professional Group on Antennas and Propagation, 1953
- Radio Transmission beyond the Horizon in the 40-to 4,000-MC BandProceedings of the IRE, 1953
- Scattering of Electromagnetic Waves by Atmospheric Turbulence: Stellar Scintillation and the Spectrum of Turbulence in the Free AtmosphereNature, 1950
- Apparatus for Recording Fluctuations in the Refractive Index of the Atmosphere at 3.2 Centimeters Wave-LengthReview of Scientific Instruments, 1950
- A Theory of Radio Scattering in the TroposphereProceedings of the IRE, 1950
- A Recording Microwave RefractometerReview of Scientific Instruments, 1950