2024-03-29T00:46:31Z
https://nagoya.repo.nii.ac.jp/oai
oai:nagoya.repo.nii.ac.jp:00019699
2023-01-26T06:44:18Z
879:1183:1689:1715
太陽電波の観測と二三の考察
DATA ON SOLAR RADIO EMISSION WITH SOME NOTES
柿沼, 隆清
高柳, 利男
太陽電波研究室一同
Kakinuma, Takakiyo
Takayanagi, Toshio
other members of Radio Astronomy Section
open access
The results of observations by 3750 and 9400 Mc/s radiometers are tabulated. The daily flux density at both frequencies has a correlation coefficient of 0.95, and the S-component 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 yet a remarkable structure of frequency spectrum 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.
名古屋大学空電研究所
1957-05-25
jpn
departmental bulletin paper
VoR
http://hdl.handle.net/2237/21745
https://nagoya.repo.nii.ac.jp/records/19699
0465-7756
空電研究所報告
7
1-2
66
99
https://nagoya.repo.nii.ac.jp/record/19699/files/bulria_7_1-2_66.pdf
application/pdf
5.1 MB
2018-02-21