Characterization of two solar active regions by activity in the radio range
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 classification of the microwave bursts taking place i...
| Main Authors: | , , |
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| Format: | Article |
| Language: | English |
| Published: |
Universidad Nacional Autónoma de México, Instituto de Geofísica
2000-02-01
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| Series: | Geofísica Internacional |
| Subjects: | |
| Online Access: | http://www.geofisica.unam.mx/unid_apoyo/editorial/publicaciones/investigacion/geofisica_internacional/anteriores/2000/02/mendez.pdf |
| Summary: | 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 classification 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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| ISSN: | 0016-7169 |