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