The 1976 Mars solar conjunction resulted in complete occultations of the Viking spacecraft by the sun at solar minimum. During the conjunction period, coherent 3.5‐ and 13‐cm wavelength radio waves from the orbiters passed through the solar corona and were received with the 64‐m antennas of the NASA Deep Space Network. Data were obtained within at least 0.3 and 0.8 Rs of the photosphere at the 3.5‐ and 13‐ cm wavelengths, respectively. The data can be used to determine the plasma density integrated along the radio path, the velocity of density irregularities in the coronal plasma, and the spectrum of the density fluctuations in the plasma. Observations of integrated plasma density near the south pole of the sun generally agree with a model of the corona which has an 8:1 decrease in plasma density from the equator to the pole. Power spectra of the 3.5‐ and 13‐cm signals at a heliocentric radial distance of about 2 Rs have a ½‐power width of several hundred hertz and vary sharply with proximate geometric miss distance. Spectral broadening indicates a marked progressive increase in plasma irregularities with decreasing ray altitude at scales between about 1 and 100 km.