Espectros de radioemisión solar con máximo en la banda de longitudes de onda centimétricas cortas: marzo a mayo de 1976

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Published: Apr 1, 1992
DOI: https://doi.org/10.22201/igeof.00167169p.1992.31.2.582
Keywords:
Solar radioemission, Active regions

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R. E. Rodríguez Toboada
Academia de Ciencias de Cuba. La Habana. Cuba.
N. G. Peterova
Academia de Ciencias de Cuba. La Habana. Cuba.
S. B. Akhmedov
Academia de Ciencias de Cuba. La Habana. Cuba.

Abstract

The most important characteristics of the 2.0 to 9.0 cm wavelength range of the active region related to the groups No. 10+11, 16 and 24 of the 1976 year (Solar Data Clasification) were determined using low, medium and high resolving power solar observations in Cuba and USSR. This material was analyzed according to the "Peculiar Source" theory, and the observed behavior is explained by the appearance of such elements in the active region. A new explanation for the empirical regularity of the short centimetric reinforcement of the spectra in active regions with high great burst possibility, which are associated with pro ton events, and bursts with the same character is proposed.

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Rodríguez Toboada, R. E., Peterova, N. G., & Akhmedov, S. B. (1992). Espectros de radioemisión solar con máximo en la banda de longitudes de onda centimétricas cortas: marzo a mayo de 1976. Geofisica Internacional, 31(2), 169–173. https://doi.org/10.22201/igeof.00167169p.1992.31.2.582
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Vol. 31 No. 2 (1992): April 1, 1992
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Article
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References

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