@article{oai:nagoya.repo.nii.ac.jp:00020274,
 author = {小林, 勝司 and 高田, 重利 and KOBAYASHI, Shoji and TAKATA, Shigetoshi},
 journal = {Proceedings of the Research Institute of Atmospherics, Nagoya University},
 month = {Mar},
 note = {波長8cm電波太陽写真儀は、位相の安定化と感度の向上を目指して改良が行なわれた。それと共に受信機の機器構成が複雑になり配置が広く分散したので、マイクロプロセッサを採用した制御系を製作した。この制御系は、バックエンドの制御、フロントエンド・第2中間周波増幅器部の制御に大きく機能を分けてあり、各部を一点で集中管理して写真儀での観測及び較正、装置の監視等が迅速容易に行なえるようにした。また各部を独立で動かす事も可能にし、ハードウエア・ソフトウエア共インタフエースを標準化したモジュールで構成する事により保守、拡張、修正を仕易くした。, The λ 8-cm radioheliograph at Toyakawa has been improved in performance of phase stability and sensitivity with an introduction of a low-noise frontend receiver for each antenna and of phase-stable coaxial cable for the transmission of reference frequency and IF signals. The total system of the radioheliograph, thus, becomes complex and is distributed along arrays, a central control system is developed. This system consists of two microprocessors, one of which is used for the backend receivers, and the other for the 2nd IF and frontend receivers respectively. Main tasks of this system are routine control and monitoring of the total system, and to execute simple test jobs such as phase calibration of each antenna, etc. Maintenance, modification, and extension of the system are easily done in both software and hardware aspects by standardization of interfaces.},
 pages = {93--104},
 title = {波長8cm電波太陽写真儀の制御装置},
 volume = {29},
 year = {1982}
}