The system of 17 GHz is routinely working since 1978, that of 35 GHz since 1983, and that of 80 GHz since 1984. The systems of 1, 2, 3.75, and 9.4 GHz were working at Toyokawa observatory of the Research Institute of Atmospherics, Nagoya University since around 1979. They were moved to Nobeyama in Apr 1994 and has been working since then.
Observing Frequencies | 1, 2, 3.75, 9.4, 17, 35, 80 GHz |
Field of View | Full Sun |
Spatial Resolution | None (Observing the flux from the full Sun disk) |
Temporal Resolution | 0.1 sec |
NoRP before the unification with Toyokawa Polarimeters
References
Last Modified at
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