Nakajima, Hiroshi (Author)
Ishiguro, Masato (Author)
Orchiston, Wayne (Author)
Akabane, Kenji (Author)
Enome, Shinzo (Author)
Hayashi, Masa (Author)
Kaifu, Norio (Author)
Nakamura, Tsuko (Author)
Tsuchiya, Atsushi (Author)
Abstract: The radio astronomy group at the Tokyo Astronomical Observatory was founded in 1948 immediately after WWII, and decided to put its main research efforts into solar radio astronomy. The first radio telescope was completed in 1949 and started routine observations at 200 MHz. Since then, the group has placed its emphasis on observations at meter and decimeter wavelengths, and has constructed various kinds of radio telescopes and arrays operating at frequencies ranging from 60 to 800 MHz. In addition, radio telescopes operating at 3, 9.5 and 17 GMHz were constructed. In parallel with the observationally-based research, theoretical research on solar radio emission also was pursued. In this paper, we review the instrumental, observational and theoretical developments in solar radio astronomy at the Tokyo Astronomical Observatory in the important period from 1949 through to the 1960s.
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