Citation
Abstract
Since 1967, radio scientists have used the Deep Space Network 26- and 64-m 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 high-resolution studies of quasars. During the reporting period, VLBI observations were made in support of investigations of quasars. Support was also provided from the 64-m antenna for the mapping of nearby spiral galaxies.
Details
- Volume
- VII
- Published
- February 15, 1972
- Pages
- 29–31
- File Size
- 208.9 KB