Microwave radiation of solar coronal holes: results of observations at RT-22 of the Scientific Research Institute “CrAO” during 2003-2006

  • С.А. Самисько Crimean Astrophysical Observatory, Nauchny, Crimea, Ukraine, 98409
  • Л.И. Цветков Crimean Astrophysical Observatory, Nauchny, Crimea, Ukraine, 98409

Abstract

Results of identification of solar coronal holes with the depressions and increases of radio brightness by means of observations at RT-22 of the SRI “CrAO” in the range 2.0–3.5 сm during 2004-2006 are presented. Inhomogeneities in the distribution of microwave radiation of coronal holes, quiet Sun and small spots are studied by means of observations at RT-22 of the solar eclipses on May, 2003, October, 2005 and March, 2006.

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Published
2008-12-26
How to Cite
Самисько С., Цветков Л., 2008. Izvestiya Krymskoi Astrofizicheskoi Observatorii, vol. 104, no. 1, pp. 83-92. Available at: https://jn.craocrimea.ru/index.php/izvcrao/article/view/593 (Accessed: 2December2020)
Section
Research articles