On a possible interpretation of the origin of the variable component of solar noise storms.
Abstract
The author shows that the observed linear dependence between the {event amplitude} and the solar storm background component can be naturally explained, if the variable component is considered as a result of random background component modulation. In this case one need not to account on a possibility of radio bursts overlapping during the emission.
- Publication:
-
Izvestiya Ordena Trudovogo Krasnogo Znameni Krymskoj Astrofizicheskoj Observatorii
- Pub Date:
- 1985
- Bibcode:
- 1985IzKry..72..208I
- Keywords:
-
- Cosmic Noise;
- Noise Storms;
- Periodic Variations;
- Solar Storms;
- Radio Frequencies;
- Solar Physics;
- Solar Radio Radiation:Storms