Physics
Scientist
St. Petersburg, 196140 Russia
Pulkovo Observatory
Can we Observe the Temperature Inhomogeneities and Magnetic Flux Tubes as the Fine Structure on the Extreme Limb of the Sun?
Informativity of the Response and Contribution Functions for Diagnostics Velocities in Solar and Stellar Atmospheres
On the Sunspot Structure
The Contribution of Magnetic Flux Tubes to Brightness Fluctuations on the Extreme Limb of the Sun
The Largescale Variation in Nature of the Solar Granulation with 10-MINUTE Period
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