Simultaneous observations of solar radio bursts in the Crimea and in Cuba
Abstract
It is found that there is difference between fine-structure details of solar bursts on two records of noise-storm intensity received simultaneously at two distant points with the same equipment at a frequency of 220 MHz. The observational results could be explained by the high directivity (of the order of 10 arcmin) of the emission of the fine structure of the type I burst sources.
- Publication:
-
Izvestiya Ordena Trudovogo Krasnogo Znameni Krymskoj Astrofizicheskoj Observatorii
- Pub Date:
- 1976
- Bibcode:
- 1976IzKry..54..220I
- Keywords:
-
- Fine Structure;
- Noise Storms;
- Solar Radio Bursts;
- Astronomical Models;
- Cuba;
- Radio Telescopes;
- Radiometers;
- Sunspots;
- Synchronism;
- Time Dependence;
- U.S.S.R.;
- Solar Physics