@article{oai:nagoya.repo.nii.ac.jp:00019571,
 author = {Radio, Astronomy Section},
 journal = {Proceedings of the Research Institute of Atmospherics, Nagoya University},
 month = {Mar},
 note = {The results of observations by 3750 Mc/s and 9400 Mc/s radiometers are tabulated. The daily flux density at both frequencies has a correlation coefficient of 0.95, and the S-componen t at 9400 Mc/s is 0.8 times as large as that at 3750 Mc/s. The sense of polarization at both frequencies is similar. The percentage polarization referring to the S-component of an isolated radio spot occasionally exceeds 30 percent at 9400 Mc/s, which is much larger than that at 3750 Mc/s. Some bursts show remarkable structure of frequency spectrum even at these super high-frequencies. The observations with an 8-element interferometer have been made for five hours every day for locating sources of outstanding occurrences. A burst occasionally occurs in an emissive region where no intense radiation is usually observed.},
 pages = {90--129},
 title = {DATA ON SOLAR RADIO EMISSION WITH SOME NOTES},
 volume = {4},
 year = {1957}
}