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Fast drift burst observations with the new Ondřejov radiospectrograph

  • Solar Physics Letters
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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.

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References

  • Benz, A.O., Magun, A., Stehling, W., Su, H.: 1992, Solar Phys. 141, 335.

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  • Krüger, A.: 1979, Introduction to Solar Radio Astronomy and Radio Physics, D. Reidel Publ. Comp., Dordrecht, Holland.

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  • Jiřič K.: 1992, Publications of Astron. Inst. Czech. Acad. Sci.81, Ondřejov, Czech Republic.

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Authors and Affiliations

  1. Astronomical Institute, Czech Academy of Sciences, 251 65, Ondřejov, Czech Republic

    K. Jiřička, M. Karlický, O. Kepka & A. Tlamicha

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  1. K. Jiřička
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  2. M. Karlický
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  3. O. Kepka
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  4. A. Tlamicha
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Jiřička, K., Karlický, M., Kepka, O. et al. Fast drift burst observations with the new Ondřejov radiospectrograph. Sol Phys 147, 203–206 (1993). https://doi.org/10.1007/BF00675495

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  • DOI: https://doi.org/10.1007/BF00675495

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