Investigation of Sun microwave emission intensity, reflected by rough sea surface

Describes the experimental investigation of natural microwave noise signal quasi-mirror reflection at sea surface roughnesses. While the weather was cloudless, the authors used the Sun as a source of this signal. Experiments were carried in a “Sun track” mode, when the solar zenith angle was more than 45 degrees, and were conducted to obtain zenith section of that “track”. The experiments were compared to solar emission intensity data, the state of the atmosphere and wave parameters. After generalisation and normalisation these data were given in dependence of wind force and large-scale riffle waving dispersion of slopes