Preliminary investigation into using the sun as a source for G/T (Gain to System Noise Temperature) measurements

Physics

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Antennas, Atmospheric Correction, Error Analysis, Noise Temperature, Solar Flux Density, Solar Radio Emission, Atmospheric Attenuation, Refraction, Standards, Wave Functions

Scientific paper

A preliminary investigation into determining the solar flux density, the atmospheric correction factor, and the star shape correction factor for use in G/T measurements above 5 GHz was conducted. An estimate of errors is also included. Preliminary results show an improved algorithm for determining diffusive and refractive attenuation, a viable technique for estimating the solar flux density from daily AFGL flux density measurements and a centimeter/millimeter wave spectrum function, and the possibility of reducing star shape correction factor errors by use of an effective solar RF diameter.

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