The occulting disk of the sun at radio wavelengths.
Solar occulting disk diameter at radio wavelengths derived from consideration of slightly deviated rays
Bracewell, R. N.↗
Engineering topics
Publications and source records attributed to Hollweg, J. V..
Solar occulting disk diameter at radio wavelengths derived from consideration of slightly deviated rays
Solar wind turbulence properties deduced from radio astronomical measurements
Solar wind interaction with moon, discussing core/ surface layer conductivity and lunar limb shock wave formation
Radio ray scattering resulting from traversing anisotropically turbulent solar corona, noting refraction effect on signal pulse arrival time
Solar corona delay effects on pulsar signals due to inhomogeneities in coronal electron density
Statistical ray analysis of radio wave scattering by anisotropically turbulent nonhomogeneous solar corona