Citation

Abstract

Since 1967, radio scientists have used the Deep Space Network (DSN) 26and 64-meter antenna stations to investigate pulsars, to study the effects of solar corona on radio signals, and to observe radio emissions of X-ray sources. Very long baseline interferometry (VLBI) techniques have also been used for highresolution studies of quasars. Several VLBI observations that were accomplished during the reporting period are summarized.

Details

Volume
IV
Published
August 15, 1971
Pages
47–48
File Size
161.1 KB