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Scientist
Moskovskij Gosudarstvennyj University
Gosudarstvennyj Astronomicheskij Inst., Moscow, Russia
A Mechanism for the Formation of the CN Lines in the Solar Photosphere.
A Mechanism for the Formation of the CN Lines in the Solar Photosphere.
A study of periodicities in the Sun's barycentric motion during 2045 years.
Model of the Photosphere Based on the Rotational Temperatures of CH, NH, OH, C2, CN, and CO Molecules
On a Spurious Correction to the Tidal Force
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