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The variability of photospheric granulation and total radio flux of quiet sun in the centimetric waveband during a solar cycle

  • Session 4. The Surface Fine Structure as a Probe of the Solar Interior
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  • First Online:
High Resolution in Solar Physics

Part of the book series: Lecture Notes in Physics ((LNP,volume 233))

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Abstract

We studied the variability of the total solar radio flux in eight frequencies, in the centimetric range during more than a solar cycle (1964–1978), and the possible relationship it has with the variability of the photospheric granulation.

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References

  • Kundu M. R.:19569 Solar Radio Astronomy, Interscience. New York.

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  • Macris C. J.: 1955, Observatory, 75, 122.

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  • Macris C. J., Rösch J.: 1983a, C. R. Acad. des France, 296. II, 265.

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  • Macris C. J., Müller R., Rösch J., Roudier Th.: 1983b, Commun. by J. Rösch in the Meeting at Sacramento Peak, July 25, 1983.

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Authors and Affiliations

  1. Astronomical Institute, National Observatory of Athens, P. 0. BOX 20048, 11810, Athens, GREECE

    D. Dialetis, C. Macris & Th. Prokakis

Authors
  1. D. Dialetis
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  2. C. Macris
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  3. Th. Prokakis
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Editor information

Richard Muller

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© 1985 Springer-Verlag

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Dialetis, D., Macris, C., Prokakis, T. (1985). The variability of photospheric granulation and total radio flux of quiet sun in the centimetric waveband during a solar cycle. In: Muller, R. (eds) High Resolution in Solar Physics. Lecture Notes in Physics, vol 233. Springer, Berlin, Heidelberg. https://doi.org/10.1007/BFb0022426

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  • DOI: https://doi.org/10.1007/BFb0022426

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  • Publisher Name: Springer, Berlin, Heidelberg

  • Print ISBN: 978-3-540-15678-9

  • Online ISBN: 978-3-540-39608-6

  • eBook Packages: Springer Book Archive

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