@article{oai:nagoya.repo.nii.ac.jp:00019709,
 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},
 issue = {1-2},
 journal = {空電研究所報告},
 month = {Mar},
 note = {Outline of the equipment used for solar radio observations at Toyokawa station which are in operation since the begining of IGY is described together with the method of tabulation. Percentage variation of the S-component versus frequency is calculated for the first half-year period of IGY, which shows a peak near 4000 Mc/s. Left-hand polarization of S-component prevails in this period at frequencies below 3750 Mc/s and there are many cases where the sense of polarization reverses between 3750 and 9400 Mc/s. Experiment has been made for detecting linear polarization at a frequency of 3750 ± 5 Mc/s, but we have yet no data to show the existence of linear polarization for both S-component and outstanding occurrences.},
 pages = {67--73},
 title = {IGYにおけるマイクロ派太陽電波の観測},
 volume = {8},
 year = {1958}
}