Citation
Abstract
Since 1967, radio scientists have used the DSN 26- and 64-m antenna stations to investigate pulsars, the effects of the solar corona on radio signals, to observe radio emissions of X-ray sources, and have used very long baseline interferometry techniques for high-resolution studies of quasars. The various experiments are identified and summarized, and the published results are indicated.
Details
- Volume
- III
- Published
- June 15, 1971
- Pages
- 46–51
- File Size
- 405.3 KB