Radio bursts of very short duration: Fine structure of solar flare emissions
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...
I tiakina i:
| I whakaputaina i: | Geofísica Internacional |
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| Ngā kaituhi matua: | , |
| Hōputu: | Artigo |
| Reo: | Inglês |
| I whakaputaina: |
Universidad Nacional Autónoma de México
2006
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| Ngā marau: | |
| Urunga tuihono: | https://www.redalyc.org/articulo.oa?id=56845406 |
| Ngā Tūtohu: |
Kāore He Tūtohu, Me noho koe te mea tuatahi ki te tūtohu i tēnei pūkete!
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