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Information × Registration Number 0306U003274, 0103U002153 , R & D reports Title Magnetic fields dinamics in Solar active regions popup.stage_title ДОСЛІДЖЕННЯ СИЛ, ЯКІ ПРИВОДЯТЬ ДО ВИХОДУ МАГНІТНОГО ПОЛЯ НА ПОВЕРХНЮ СОНЦА Head Gopasyuk O.S., Registration Date 27-02-2006 Organization Scientific-research institute "Crimean astrophysical observatory" popup.description2 It is shown the velocity of drift of magnetic structures depends directly as the angular velocity of stellar rotation. It is found that the both the equivalent width and the depth of the MnI 539.4 nm line profile decrease with increasing strength of magnetic field in plage. The full width at half maximum does not show any significant regular changes. Product Description popup.authors popup.nrat_date 2020-04-02 Close