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Quiet sun from multifrequency radio observations on RATAN-600

  • Part IV Large-Scale Structure of the Corona
  • Conference paper
  • First Online:
Advances in Solar Physics

Part of the book series: Lecture Notes in Physics ((LNP,volume 432))

Abstract

We present several characteristics of the quiet Sun radio emission in the range 2–32 cm: the center-to-limb variation of brightness temperature, the radio radius for various positional angles, the brightness temperature spectrum at the center of the disk. These were obtained with the RATAN-600 radio telescope at wavelengths of 2.0, 2.3, 2.7, 3.2, 4.0, 8.2, 11.7, 20.7 and 31.6 cm simultaneously during the recent sunspot minimum (1984-87). The new data are in good agreement with those obtained during previous solar activity cycles both on RATAN-600 radio telescope and on other large instruments.

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Authors and Affiliations

  1. Main Astronomical Observatory, Pulkovo, 196140, St.Petersburg, Russia

    V. N. Borovik

Authors
  1. V. N. Borovik
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Editor information

G. Belvedere M. Rodonò G. M. Simnett

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© 1994 Springer-Verlag

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Borovik, V.N. (1994). Quiet sun from multifrequency radio observations on RATAN-600. In: Belvedere, G., Rodonò, M., Simnett, G.M. (eds) Advances in Solar Physics. Lecture Notes in Physics, vol 432. Springer, Berlin, Heidelberg. https://doi.org/10.1007/3-540-58041-7_217

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  • DOI: https://doi.org/10.1007/3-540-58041-7_217

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  • Publisher Name: Springer, Berlin, Heidelberg

  • Print ISBN: 978-3-540-58041-6

  • Online ISBN: 978-3-540-48420-2

  • eBook Packages: Springer Book Archive

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