@article{oai:nagoya.repo.nii.ac.jp:00020047,
 author = {TANAKA, Haruo and KAKINUMA, Takakiyo and ENOME, Shinzo and TORII, Chikayoshi and TSUKIJI, Yoshio and KOBAYASHI, Shoji},
 journal = {Proceedings of the Research Institute of Atmospherics, Nagoya University},
 month = {Mar},
 note = {A (32+2)-element compound interferometer for solar observations at 3.75 GHz has been in operation since August 1967. The HPBW is 23 seconds of arc for the compound and 1.1 minutes of arc for the 32-element adding interferometer. The outputs of these two kinds of interferometers are recorded at the same time with the sum and difference channels of two circularly polarized components. Artificial scanning of once each ten seconds by the adding interferometer has become possible since August 1968 for the observation of the rapidly changing burst.},
 pages = {113--126},
 title = {A HIGH-RESOLUTION QUICK-SCAN INTERFEROMETER FOR SOLAR STUDIES AT 3.75 GHz},
 volume = {16},
 year = {1969}
}