@article{oai:nagoya.repo.nii.ac.jp:00019752,
 author = {柿沼, 隆清 and KAKINUMA, Takakiyo},
 issue = {1-2},
 journal = {空電研究所報告},
 month = {Mar},
 note = {From the observations with 4000 Mc/s interferometer, the flux density of the quiet sun component at 3750 Mc/s in 1957-58 is estimated at 122X10^-22W・m^-2(c/s)^-1. This value is about 1.6 times higher than the value at sunspot minimum. The recent interferometric observations suggest that the change of the quiet sun component at 9400 Mc/s during the sunspot cycle is only a few %. From the spectrum of the brightness of the center of the solar disk, derived from the eclipse observation at 9400, 3750, 2000 and 1000 Mc/s, the electron density of the corona around 1958 is estimated to be about 1.5-2.0 times higher than Alen-Baumbach' value.},
 pages = {15--18},
 title = {太陽活動最盛期附近におけるマイクロ波太陽電波の静かな太陽成分について},
 volume = {12},
 year = {1962}
}