Radio observations of venus and the interpretations.

摘要: The radio observations of Venus are reviewed and compared with theoretical microwave spectra computed for a variety models the Venusian environment. considered (a) CO2-N2 atmosphere, (b) an atmosphere dust (the aeolosphere model), (c) cloud model various loss mechanisms in cloud. effect polarization on surface emissivity has been included all computations. It is shown how place limits upon acceptable models, example, density size particles required model. some severe restrictions radar at short centimeter wavelengths, thereby emphasizing importance such experiments. These same show that Mariner II can not be interpreted terms phenomena provide new interpretation phase effect.