Solar Corona, Magnetic Fields, Heating and Cyclic Variations
- O.G.Badalyan, V.N.Obridko, J.Sykora
Brightness of the coronal green line and prediction for activity cycles 23 and 24
Solar Phys., 2001, 199, 421
- O. G. Badalyan and V. N. Obridko
Solar magnetic fields and the intensity of the green coronal line
Astronomy Reports, Vol. 48, №8, 2004, pp. 678-687,engltranslated fromAstronomicheski Zhurnal, Vol. 81, № 8, 2004, pp. 746-756, rus
- O.G. Badalyan, V.N. Obridko, J. Sykora
Temporal variations of the solar corona rotation
11th European Solar Physics Meeting, The Dynamic Sun: Challenges for Theory and Observations, 11 – 16 September 2005 2005, Leuven, Belgium, SP-600 – December 2005, ESA Publication Division, ESTEC, P.O. Dox 299, 2200 AG Noordwijk, The Netherlands, Ed. D.Danesy, S.Poeds, A. De Groof, J. Andres.
- O.G. Badalyan and V.N. Obridko
Two regularities in the coronal green-line brightness – magnetic field coupling and the heating of the corona
Solar Physics (2006) 238: 271–292
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