ON THE PROPAGATION OF RADIO EMISSION IN THE CROWN OF THE QUIET SUN WITH MAGNETIC FIELD
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.
Yazar: | |
---|---|
Materyal Türü: | Makale |
Dil: | English |
Baskı/Yayın Bilgisi: |
Odessa I. I. Mechnykov National University
2013-11-01
|
Seri Bilgileri: | Odessa Astronomical Publications |
Konular: | |
Online Erişim: | http://oap.onu.edu.ua/article/view/83958 |