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 |
| _version_ | 1797727355281604608 |
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| author | Asdai Díaz Rodríguez Ramón E. Rodríguez Taboada Adolfo L. Méndez Berhondo |
| author_facet | Asdai Díaz Rodríguez Ramón E. Rodríguez Taboada Adolfo L. Méndez Berhondo |
| author_sort | Asdai Díaz Rodríguez |
| collection | DOAJ |
| description | 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. |
| first_indexed | 2024-03-12T10:58:38Z |
| format | Article |
| id | doaj.art-7ba84d96485141a7b00f8b5ccaa8d2d5 |
| institution | Directory Open Access Journal |
| issn | 0016-7169 |
| language | English |
| last_indexed | 2024-03-12T10:58:38Z |
| publishDate | 2000-02-01 |
| publisher | Universidad Nacional Autónoma de México, Instituto de Geofísica |
| record_format | Article |
| series | Geofísica Internacional |
| spelling | doaj.art-7ba84d96485141a7b00f8b5ccaa8d2d52023-09-02T06:02:06ZengUniversidad Nacional Autónoma de México, Instituto de GeofísicaGeofísica Internacional0016-71692000-02-01392201203Characterization of two solar active regions by activity in the radio rangeAsdai Díaz RodríguezRamón E. Rodríguez TaboadaAdolfo L. Méndez BerhondoBased 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.http://www.geofisica.unam.mx/unid_apoyo/editorial/publicaciones/investigacion/geofisica_internacional/anteriores/2000/02/mendez.pdfActive regionscoronal magnetic structuresradioemission |
| spellingShingle | Asdai Díaz Rodríguez Ramón E. Rodríguez Taboada Adolfo L. Méndez Berhondo Characterization of two solar active regions by activity in the radio range Geofísica Internacional Active regions coronal magnetic structures radioemission |
| title | Characterization of two solar active regions by activity in the radio range |
| title_full | Characterization of two solar active regions by activity in the radio range |
| title_fullStr | Characterization of two solar active regions by activity in the radio range |
| title_full_unstemmed | Characterization of two solar active regions by activity in the radio range |
| title_short | Characterization of two solar active regions by activity in the radio range |
| title_sort | characterization of two solar active regions by activity in the radio range |
| topic | Active regions coronal magnetic structures radioemission |
| url | http://www.geofisica.unam.mx/unid_apoyo/editorial/publicaciones/investigacion/geofisica_internacional/anteriores/2000/02/mendez.pdf |
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