2024-03-29T01:26:08Z
https://nagoya.repo.nii.ac.jp/oai
oai:nagoya.repo.nii.ac.jp:00019708
2023-01-26T06:49:42Z
879:1183:1689:1716
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
POLARIZATION OF SOLAR RADIO BURSTS AT MICROWAVE FREQUENCIES. I.
柿沼, 隆清
KAKINUMA, Takakiyo
open access
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.
名古屋大学空電研究所
1958-03-20
jpn
departmental bulletin paper
VoR
http://hdl.handle.net/2237/21754
https://nagoya.repo.nii.ac.jp/records/19708
0465-7756
空電研究所報告
8
1-2
60
66
https://nagoya.repo.nii.ac.jp/record/19708/files/bulria_8_1-2_60.pdf
application/pdf
1.2 MB
2018-02-21