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High-resolution observations of solar radio bursts with multi-element compound interferometers at 3.75 and 9.4 GHz

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Abstract

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: (1) 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 GHz. (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 burst of December 16, 1967.

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Authors and Affiliations

  1. Research Institute of Atmospherics, Nagoya University, Toyokawa, Aichi, Japan

    Shinzo Énomé, Takakiyo Kakinuma & Haruo Tanaka

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  1. Shinzo Énomé
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  2. Takakiyo Kakinuma
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  3. Haruo Tanaka
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Énomé, S., Kakinuma, T. & Tanaka, H. High-resolution observations of solar radio bursts with multi-element compound interferometers at 3.75 and 9.4 GHz. Sol Phys 6, 428–441 (1969). https://doi.org/10.1007/BF00146477

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  • DOI: https://doi.org/10.1007/BF00146477

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