High-resolution observations of solar radio bursts with multi-element compound interferometers at 3.75 and 9.4 GHz
✍ Scribed by Shinzo Énomé; Takakiyo Kakinuma; Haruo Tanaka
- Publisher
- Springer
- Year
- 1969
- Tongue
- English
- Weight
- 528 KB
- Volume
- 6
- Category
- Article
- ISSN
- 0038-0938
No coin nor oath required. For personal study only.
✦ Synopsis
High-resolution observations of solar radio bursts made simultaneously with multi-element compound interferometers at 3.75 and 9.4 GHz are presented.
Preliminary results are: (l) The burst of December 16, 1967 showed a change in polarization distribution in the radio source, which suggests a magnetic field change in the source. (2) The existence of the multi-source burst is also confirmed at 3.75 G}-1z. (3) The source size of the impulsive burst is estimated to be ~0.'5. (4) Among the GRF bursts there seem to be two kinds; one has a large angular size and the other has a small one.
A brief discussion is given of the bm'st o1" December 16, 1967.