Radio bursts of very short duration: Fine structure of solar flare emissions
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| Format: | Artículo científico |
| Language: | en |
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Universidad Nacional Autónoma de México
2006
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| _version_ | 1876476535577247744 |
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| author | A. L. Méndez Berhondo |
| author_facet | A. L. Méndez Berhondo |
| contents | Radio bursts of very short duration: Fine structure of solar flare emissions A. L. Méndez Berhondo R. E. Rodríguez Taboada Ciencias de la Tierra spikes Solar radio emission polarization diagram The fine time structure of sub-second radio events of solar flare emissions is described on the multichannel polarimeter ofStation Basovizza at 237, 327, and 408 MHz frequencies. We selected the February 8 and July 9, 1982 solar radio bursts, bothassociated to gamma flares. We considered only events with more than 100 solar flux units. The relationship between theintensity of the impulsive radio events and the background radio emission is discussed. 2006 artículo científico 0016-7169 https://www.redalyc.org/articulo.oa?id=56845406 en http://www.redalyc.org/revista.oa?id=568 Geofísica Internacional application/pdf Universidad Nacional Autónoma de México Geofísica Internacional (México) Num.4 Vol.45 |
| format | Artículo científico |
| id | redalyc_56845406 |
| institution | Redalyc |
| language | en |
| publishDate | 2006 |
| publisher | Universidad Nacional Autónoma de México |
| spellingShingle | Radio bursts of very short duration: Fine structure of solar flare emissions A. L. Méndez Berhondo Ciencias de la Tierra spikes Solar radio emission polarization diagram Radio bursts of very short duration: Fine structure of solar flare emissions A. L. Méndez Berhondo R. E. Rodríguez Taboada Ciencias de la Tierra spikes Solar radio emission polarization diagram The fine time structure of sub-second radio events of solar flare emissions is described on the multichannel polarimeter ofStation Basovizza at 237, 327, and 408 MHz frequencies. We selected the February 8 and July 9, 1982 solar radio bursts, bothassociated to gamma flares. We considered only events with more than 100 solar flux units. The relationship between theintensity of the impulsive radio events and the background radio emission is discussed. 2006 artículo científico 0016-7169 https://www.redalyc.org/articulo.oa?id=56845406 en http://www.redalyc.org/revista.oa?id=568 Geofísica Internacional application/pdf Universidad Nacional Autónoma de México Geofísica Internacional (México) Num.4 Vol.45 |
| title | Radio bursts of very short duration: Fine structure of solar flare emissions |
| topic | Ciencias de la Tierra spikes Solar radio emission polarization diagram |
| url | https://www.redalyc.org/articulo.oa?id=56845406 |