Citation
Abstract
Since 1967 radio astronomers have used the Deep Space Network (DSN) 26- and 64-meter diameter antenna stations to investigate the Moon, planets, pulsars, and radio galaxies to study the effects of solar corona on radio signals, and to observe radio emissions from X-ray sources. Very Long Baseline Interferometry (VLBI) techniques have been used for high-resolution studies of quasars, suspected black holes, and other radio sources. The high-power transmitter capability of the Goldstone 64-meter antenna has been used for radar-ranging to the planets in support of various planetary space missions and for the study of comets and asteroids. The overseas facilities in Spain and Australia have been used, on a noninterference basis with space mission operations, by host country radio astronomers. The background for the DSN support, past performance, and current plans for continued support of these activities are discussed. Various experiments of the past year are identified and summarized.
Details
- Volume
- 42-53
- Published
- October 15, 1979
- Pages
- 46–47
- File Size
- 259.1 KB