Physics
Scientist
Institute of Solar-Terrestrial Physics, Siberian Branch, Russian Academy of Sciences
Asymmetry of the contours of the Fe X 6374-Å coronal line
On the existence of the east-west asymmetry in the optical observations of the solar corona
The green coronal line above an active region at the solar limb on 5 Aug. of 1989.
The projection effect when solar activity phenomena are mapped in galactic coordinates
The Sayan Observatory coronograph.
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