Citation
Abstract
Since 1967, radio scientists have used the Deep Space Network 26- and 64-mdiameter antenna stations to investigate pulsars, to study the effect of solar corona on radio signals, and to observe radio emissions from X-ray sources. More recently, very long baseline interferometry (VLBI) techniques have been used for highresolution studies of quasars. During the reporting period, VLBI observations were made of quasars and also of the Mariner 9 spacecraft. Support was also provided by the 64-m-diameter antenna for the measurement of cosmic background noise.
Details
- Volume
- VIII
- Published
- April 15, 1972
- Pages
- 24–28
- File Size
- 310.5 KB