@article{oai:nagoya.repo.nii.ac.jp:00019590,
 author = {柿沼, 隆清 and KAKINUMA, Takakiyo},
 issue = {1},
 journal = {空電研究所報告},
 month = {Sep},
 note = {From the eclipse observation on Feb. 14, 1953, it is concluded that the radio solar disk is about 1.06 times larger than the optical disk. While，experimental record pattern，obtained from the interferometer，do not agree with the calculated one corresponding to uniform distribution over the radio disk. Experimental pattern is obtained if the excess region is about 2.5 times brighter than the optical disk of the uniform temperature，about 1.9x10^4°K. This assumption can also fully explain the variation of radio intensities in the later part of the eclipse when no active zones are covered.},
 pages = {36--38},
 title = {4,000MC帶における太陽面上の輻射強度分布について},
 volume = {4},
 year = {1953}
}