Characteristics of the radiation of polar coronal holes on the Sun in a wide range of radio waves

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Published: Jun 15, 2022
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DOI: https://doi.org/10.34898/aat.vol3.iss2.pp22-26
Keywords:
Sun coronal holes radio emission

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O.A. Golubchina
St. Petersburg Branch of the Special Astrophysical Observatory, St. Petersburg 196140, Russia

Abstract

The paper presents a brief overview of the main results of observations of the radio emission in polar coronal holes on the Sun obtained in a wide range of wavelengths with various radio telescopes. We analyze the results of observations of the polar coronal hole with RATAN–600 in a wide centimeter wavelength range of (1.03–30.7) cm. The obtained physical characteristics of the coronal hole above the north pole of the Sun are compared with the characteristics of the coronal holes located at lower latitudes.

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How to Cite
Golubchina O. , 2022. Acta Astrophysica Taurica, vols. 3, nos. 2, pp. 22–26. DOI: 10.34898/aat.vol3.iss2.pp22-26
Issue
Vol. 3 No. 2 (2022)
Section
Magnetism and activity of the Sun and stars – 2021 Conference proceedings
Copyright and publishing rights for texts published in Acta Astrophysica Taurica is retained by the authors, with first publication rights granted to the journal.Texts are free to use with proper attribution and link to the licensing (Creative Commons Attribution 4.0 International).

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