Fast drift burst observations with the new Ondřejov radiospectrograph
Solar Physics Letters
Received:
Abstract
The new 100–4200 MHz Ondřejov radiospectrograph and the high-time resolution 3 GHz radiometer are described and the observations of fast drift bursts during the increased solar activity of September 5–7, 1992 are presented and analyzed.
Keywords
Solar Activity Fast Drift Drift Burst Burst Observation Fast Drift Burst
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References
- Benz, A.O., Magun, A., Stehling, W., Su, H.: 1992, Solar Phys. 141, 335.Google Scholar
- Initial Results from Yohkoh, 1992, Publications of Astron. Soc. Jap. 44 (5), L41–L214.Google Scholar
- Krüger, A.: 1979, Introduction to Solar Radio Astronomy and Radio Physics, D. Reidel Publ. Comp., Dordrecht, Holland.Google Scholar
- Jiřič K.: 1992, Publications of Astron. Inst. Czech. Acad. Sci.81, Ondřejov, Czech Republic.Google Scholar
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© Kluwer Academic Publishers 1993