ON THE PROPAGATION OF RADIO EMISSION IN THE CROWN OF THE QUIET SUN WITH MAGNETIC FIELD

Автор(и)

  • N. Tsvyk Radio Astronomy Institute of NASU, Kharkiv, Україна

DOI:

https://doi.org/10.18524/1810-4215.2013.26.83958

Ключові слова:

quiet Sun, crown, radioemission, refraction

Анотація

There are searching for factors that influ­ence on the brightness temperature distribution of the quiet Sun at decameter radio waves which may explain the ellipsoidal shape and other features in the radio brightness profile.

 

Посилання

Stanislavsky А.А., Кoval А.А.: 2013, Radiofizika i radioastronomia, 18 (in press.).

Brazhenko A.I., Кoval А.А. et al.: 2012, Radiofizika i

radioastronomia, 17, 3.

Sykora J. et al.: 2003, Solar Phys., 212, 301.

Perebejnos V.A. et al.: 2011, Izv. CRAO, 107, 64.

Thejappa G., Kundu M.R.: 1994, Solar Physics, 149, 31.

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Опубліковано

2013-11-21

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