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Observation of solar radio emission by the 22-m radio telescope at the Crimean Astrophysical Observatory at 2.25 mm and 8.15 mm wavelengths

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Abstract

The results are given of observation of solar radio emission of the S-component at 8.15 mm-λ, and 2.25 mm-λ made with the 22 m radio telescope of the Crimean Astrophysical Observatory. Solar radio images are obtained at both wavelengths. The data are presented of radio emission intensity and brightness temperatures of 10 sources of the S-component as well as the result of a flare observed. The sources of the S-component appear to be opaque at millimetre wavelengths.

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Authors and Affiliations

  1. Crimean Astrophysical Observatory, AS U.S.S.R.

    V. A. Efanov, A. G. Kislyakov, I. G. Moiseev & A. I. Naumov

  2. Radio-Physical Research Institute Gorky, University, Gorky, U.S.S.R.

    V. A. Efanov, A. G. Kislyakov, I. G. Moiseev & A. I. Naumov

Authors
  1. V. A. Efanov
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  2. A. G. Kislyakov
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  3. I. G. Moiseev
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  4. A. I. Naumov
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Efanov, V.A., Kislyakov, A.G., Moiseev, I.G. et al. Observation of solar radio emission by the 22-m radio telescope at the Crimean Astrophysical Observatory at 2.25 mm and 8.15 mm wavelengths. Sol Phys 8, 331–340 (1969). https://doi.org/10.1007/BF00155380

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  • DOI: https://doi.org/10.1007/BF00155380

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