Affiliation:
1. National Radio Astronomy Observatory, Charlottesville, Virginia 22903;
2. Harvard-Smithsonian Center for Astrophysics, Cambridge, Massachusetts 02138;
Abstract
▪ Abstract Since the first radio astronomy observations in the 1930s, the angular resolution of radio telescopes has improved from tens of degrees to better than one thousandth of a second of arc. This advancement has been the result of technological innovations such as stable, sensitive, short-wavelength radio receivers, digital correlators, atomic clocks, and high-speed tape recorders, as well as the development of sophisticated image processing algorithms implemented on inexpensive, fast, digital computers.
Subject
Space and Planetary Science,Astronomy and Astrophysics
Cited by
42 articles.
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