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Information × Registration Number 0212U006552, 0111U006167 , R & D reports Title Magnetic activity of the Sun and solar-terrestrial connections in the new 24th cycle. popup.stage_title Head Lozitsky Vsevolod, Registration Date 11-05-2012 Organization Taras Shevchenko Kiev university popup.description2 On a base of observations of full solar eclipses of 1851-2010, the dependence was studied between indexes of photometrical and geometrical flattening of solar corona and level and phase of solar activity. It was shown that strong magnetic fields of 500-2000 G occur in active and quiet prominences on hights of 5-12 Mm; magnetic fields in quiet prominences are in 3-5 times less than in active ones. The semi-empirical model of global poloidal circulation in convection zone of the Sun was calculated. Product Description popup.authors Єфіменко В.М. Андрієць О.С. Бабій В.П. Ботигіна О.О. Венглінський Є.Р. Камінський С.В. Криводубський В.Н. Курочка Є.В. Лейко У.М. Лозицька Н.Й. Лозицький В.Г. Осика О.Б. Пішкало М.І. Садовенко Є.В. popup.nrat_date 2020-04-02 Close