Characterization of two solar active regions by activity in the radio range

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Published: Apr 1, 2000
DOI: https://doi.org/10.22201/igeof.00167169p.2000.39.2.277
Keywords:
Active regions, coronal magnetic structures, radioemission

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Adolfo L. Méndez Berhondo
Astronomy Department, Institute of Geophysics and Astronomy, La Lisa, Ciudad de La Habana, Cuba
Ramón E. Rodríguez Taboada
Astronomy Department, Institute of Geophysics and Astronomy, La Lisa, Ciudad de La Habana, Cuba
Asdai Díaz Rodríguez
Astronomy Department, Institute of Geophysics and Astronomy, La Lisa, Ciudad de La Habana, Cuba

Abstract

Based on a statistical analysis we present the results of a comparative study for two active regions. In order to estimate the coronal magnetic field structure we consider jointly the fluctuations of the noise storm background continuum, spectral classifica- tion of the microwave bursts taking place in them, the morphology of the active regions, and the metric-centimetric wavelength band distribution of the activity.

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How to Cite
Méndez Berhondo, A. L., Rodríguez Taboada, R. E., & Díaz Rodríguez, A. (2000). Characterization of two solar active regions by activity in the radio range. Geofisica Internacional, 39(2), 201–203. https://doi.org/10.22201/igeof.00167169p.2000.39.2.277
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Vol. 39 No. 2 (2000): April 1, 2000
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Article
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