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Observation of the Radio Radiation Flux of the Sun and Flares at a Wavelength of 5 cm

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Abstract

The results of long-term mesoscale observations in the microwave range are reviewed. The rationale for the resumption of observations at the Havana Radio Astronomy Station is justified. Domestic observations at a wavelength of λ5 cm have a long observation interval and can effectively complement the global series of observations. A comparative analysis of the results of solar observation in the radio range and satellite observations in the UV and X-ray range is performed. The value of continuous observations for the assessment of space weather factors is shown.

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Funding

The study was supported by the Russian Foundation for Basic Research (project nos. 18-02-00098 and 18-52-34004) and the Ministry of Science, Technology, and the Environment of Cuba.

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Authors and Affiliations

  1. Mountain Astronomical Station, State Astronomical Observatory, Russian Academy of Sciences, Kislovodsk, Russia

    A. G. Tlatov

  2. Kalmyk State University, Elista, Russia

    A. G. Tlatov

  3. Special Astrophysical Observatory of the Russian Academy of Sciences, St. Petersburg Branch, St. Petersburg, Russia

    V. M. Bogod

  4. Institute of Geophysics and Astronomy of Cuba, Havana, Cuba

    O. Pons, M. Rodriges, R. Estrada & S. Pablo

Authors
  1. A. G. Tlatov
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  2. V. M. Bogod
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  3. O. Pons
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  4. M. Rodriges
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  5. R. Estrada
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  6. S. Pablo
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Correspondence to A. G. Tlatov.

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Tlatov, A.G., Bogod, V.M., Pons, O. et al. Observation of the Radio Radiation Flux of the Sun and Flares at a Wavelength of 5 cm. Geomagn. Aeron. 60, 1087–1092 (2020). https://doi.org/10.1134/S0016793220080241

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  • DOI: https://doi.org/10.1134/S0016793220080241

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