2024-03-29T07:30:26Z
https://nagoya.repo.nii.ac.jp/oai
oai:nagoya.repo.nii.ac.jp:00019608
2023-01-26T05:07:55Z
879:1183:1640:1703
OBSERVATIONS OF SOLAR RADIO EMISSION AT MICROWAVE FREQUENCIES
TANAKA, HARUO
KAKINUMA, TAKAKIYO
open access
Outline of the equipment used for radio observations at Toyokawa station which are in operation since the beginning of IGY is described together with the method of tabulation. Percentage variation of the S-component versus frequency is calculated for the first half-year period of IGY, which shows a peak near 4000 Mc/s. Left-hand polarization of S-component prevails in this period at frequencies below 3750 Mc/s and there are many cases where the sense of polarization reverses between 3750 and 9400 Mc/s. Experiment has been made for detecting liner polarization at a frequency of 3750±5 Mc/s, but we have yet no data to show the existence of linear polarization for both S-component and outstanding occurrences.
The Research Institute of Atmospherics, Nagoya University
1958-03-25
eng
departmental bulletin paper
VoR
http://hdl.handle.net/2237/21654
https://nagoya.repo.nii.ac.jp/records/19608
0077-264X
Proceedings of the Research Institute of Atmospherics, Nagoya University
5
81
89
https://nagoya.repo.nii.ac.jp/record/19608/files/Vol5-9.pdf
application/pdf
1.7 MB
2018-02-21