Physics
Scientist
Glavnaya Astronomicheskaya Observatoriya, Kislovodsk, Russia
A solar source of intensified variations (duration about one hour) of the IMF.
Chromospheric cavity, filament and coronal hole in Hα and radio emission.
Dimension and structure of the solar attractor using the values of the solar magnetic field energy in solar cycle 21.
Global solar cycle in the distribution of the green and red coronal emission. Period 1940 - 1989.
Large-scale structure of solar magnetic cyclicity
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