2024-03-29T05:50:01Z
https://nagoya.repo.nii.ac.jp/oai
oai:nagoya.repo.nii.ac.jp:00020047
2023-01-26T04:14:44Z
879:1183:1640:1738
A HIGH-RESOLUTION QUICK-SCAN INTERFEROMETER FOR SOLAR STUDIES AT 3.75 GHz
TANAKA, Haruo
58681
KAKINUMA, Takakiyo
58682
ENOME, Shinzo
58683
TORII, Chikayoshi
58684
TSUKIJI, Yoshio
58685
KOBAYASHI, Shoji
58686
1969-03-30
A (32+2)-element compound interferometer for solar observations at 3.75 GHz has been in operation since August 1967. The HPBW is 23 seconds of arc for the compound and 1.1 minutes of arc for the 32-element adding interferometer. The outputs of these two kinds of interferometers are recorded at the same time with the sum and difference channels of two circularly polarized components. Artificial scanning of once each ten seconds by the adding interferometer has become possible since August 1968 for the observation of the rapidly changing burst.
departmental bulletin paper
The Research Institute of Atmospherics, Nagoya University
1969-03-30
Proceedings of the Research Institute of Atmospherics, Nagoya University
16
113
126
http://hdl.handle.net/2237/22009
0077-264X
eng