@article{oai:nagoya.repo.nii.ac.jp:00019721,
 author = {鎌田, 哲夫 and 中島, 淳 and KAMADA, Tetsuo and NAKAJIMA, Jun},
 issue = {1-2},
 journal = {空電研究所報告},
 month = {Mar},
 note = {This report discribes the statistical results obtained in five years from 1955 to 1959, about SEA which is caused by the solar flare disturbances. The important matters resolve itself into the following points. That is, (1) The basic modes and types of SEA are determincd from among the abnormal increase of the intensity of atmospherics. (2) In order to determined the abnormal increase of the intensity of atmospherics as SEA, it is necessary to observe three frequency component about 10, 20 and 30 Kc/s simultaneously. (3) The results obtained have intensified the conception that to observe SEA is the most useful means for watching SF and SRO on the sun.},
 pages = {29--37},
 title = {長波帯におけるSEA現象の統計的性質},
 volume = {10},
 year = {1960}
}