Citation
Abstract
Since 1967 radio scientists have used the DSN 26- and 64-m antenna stations to investigate pulsars, to study the effects of solar corona on radio signals, and to observe radio emissions of X-ray sources. More recently, very long baseline interferometry (VLBI) techniques have been used for high resolution studies of quasars. During the reporting period, several proposals were received for extension of VLBI observations which had reported the startling expansion of quasar 3C279.
Details
- Volume
- V
- Published
- October 15, 1971
- Pages
- 42–44
- File Size
- 162.5 KB