@article{oai:nagoya.repo.nii.ac.jp:00019708,
 author = {柿沼, 隆清 and KAKINUMA, Takakiyo},
 issue = {1-2},
 journal = {空電研究所報告},
 month = {Mar},
 note = {The intensity and polarization of solar radio bursts have been observed at 9400, 3750, 2000 and 1000 Mc/s since July 1957. In this paper the results of observations during 6 months are described. In most bursts at microwave frequencies, the difference in the intensity of two circularly polarized components is observed. At 3750 Mc/s, the bursts of small degree of polarization (less than 10%) are predominant, compared with other frequencies. At 2000 and 1000 Mc/s the circularly polarized bursts were occasionally observed, but not at 9400 and 3750 Mc/s. In most bursts observed at four frequencies, the sense of polarization reverses near 3750 or 2000 Mc/s and the degree of polarization is generally small at 3750 Mc/s. At 9400 Mc/s, it seems that the sense of polarization correlates with the position of the source on the solar disk. Further observations will be continued to investigate the relation between them.},
 pages = {60--66},
 title = {マイクロ波帯における太陽電波バーストの偏波について I},
 volume = {8},
 year = {1958}
}