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

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...

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Bibliographic Details
Published in:Geomagnetism and Aeronomy 2020-12, Vol.60 (8), p.1087-1092
Main Authors: Tlatov, A. G., Bogod, V. M., Pons, O., Rodriges, M., Estrada, R., Pablo, S.
Format: Article
Language:English
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Summary: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.
ISSN:0016-7932
1555-645X
0016-7940
DOI:10.1134/S0016793220080241