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- Title
Spectral characteristics of large-scale radio emission areas in coronal holes.
- Authors
Prosovetsky, D. V.; Grigor’eva, I. Yu.; Kochanov, A. A.
- Abstract
The spectra of the coronal hole radio emission in solar cycles 23 and 24 have been studied based on RATAN-600 data in the 4–16.5 GHz range at frequencies of 5.7 and 17 GHz and 327 MHz. It has been found that bright features of coronal hole microwave emission at 17 GHz and dark features at 5.7 GHz can exist in coronal holes when the spectral index is 1.25–1.5 in the 6.5–16.5 GHz range; the radio spectrum in this range is flat when coronal holes are indiscernible against the background of a quiet Sun. The possible vertical scale of the solar atmosphere over coronal holes is discussed.
- Subjects
SOLAR radio emission; SOLAR spectra; CORONAL holes; SOLAR cycle; SOLAR atmosphere; MICROWAVES
- Publication
Geomagnetism & Aeronomy, 2013, Vol 53, Issue 7, p867
- ISSN
0016-7932
- Publication type
Article
- DOI
10.1134/S0016793213070177