[en] Intensity scintillation observations covering the frequency range of 270 to 8085 MHz are analyzed to extract information about the solar wind. The data cover distance from the sun of approximately 5 to 100 solar radii. Multi-frequency observations at three frequencies from 270 to 470 MHz taken in 1976 and three-site-spaced receiver observations at 2295 MHz and single site observations at 1410 and 8085 MHz were made. The data were analyzed with the following objectives: to infer the shape of the electron density spectrum to estimate the solar wind velocity and random velocity near the sun to develop and test a method of single site velocity determination and to compare weak scattering theory and experiment