@article{oai:nagoya.repo.nii.ac.jp:00019688,
 author = {田中, 春夫 and 柿沼, 隆清 and 神藤, 英彦 and 高柳, 利男 and 鳥居, 近吉 and TANAKA, Haruo and KAKINUMA, Takakiyo and JINDO, Hidehiko and TAKAYANAGI, Toshio and TORII, Chikayoshi},
 issue = {1-2},
 journal = {空電研究所報告},
 month = {Apr},
 note = {A 1.2 meter dish radio telescope for use at 9,400 MC was completed at the end of 1955. A circular-waveguide feed at the focus of the dish is connected directly to a turnstile circuit and 4 polarized components can be received by switching. The Dicke's modulation is performed statically by the circulator using a Faraday plate, and the modulation frequency is 500 c/s. S-component at 9,400 MC is 30% of that observed at 3750 MC refering to each quiet level. On the logarithmic scale, the height of outstanding occurrences are almost the same at two frequencies. Some bursts observed in January and February 1956 have no connection with each other at two frequencies, which suggests that remarkable frequency spectrum still exists at these high frequencies.},
 pages = {61--66},
 title = {9400MCにおける太陽電波の観測},
 volume = {6},
 year = {1956}
}