6–10 Sept 2021
Online
Europe/Rome timezone

Features of the physical characteristics of the radiation of polar coronal holes in the Sun according to observations in the radio range

9 Sept 2021, 11:13
13m
Online

Online

Poster Session 2 - The Solar Atmosphere: Heating, Dynamics and Coupling Poster Session 10.2

Speaker

Olga Golubchina (Features of the physical characteristics of the radiation of polar coronal holes in the Sun according to observations in the radio range)

Description

The article presents a brief overview of the main results of observations of the radio emission of polar coronal holes (CD) on the Sun, obtained in a wide range of wavelengths (m-mm) on various radio telescopes. The results of observations of the polar coronal hole (CD) on RATAN-600 in a wide centimeter wavelength range (1.03-30.7) are analyzed. The obtained physical characteristics of the CD over the North Pole of the Sun are compared with the characteristics of the CD located at lower latitudes.

Primary author

Olga Golubchina (Features of the physical characteristics of the radiation of polar coronal holes in the Sun according to observations in the radio range)

Presentation materials