טוען...
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...
שמור ב:
| הוצא לאור ב: | Geofísica Internacional |
|---|---|
| Main Authors: | , |
| פורמט: | Artigo |
| שפה: | Inglês |
| יצא לאור: |
Universidad Nacional Autónoma de México
2006
|
| נושאים: | |
| גישה מקוונת: | https://www.redalyc.org/articulo.oa?id=56845406 |
| תגים: |
הוספת תג
אין תגיות, היה/י הראשונ/ה לתייג את הרשומה!
|