Physics
Scientist
A new approach to the study of the large-scale structure of the solar corona on the basis of measurements of solar wind parameters.
A new method to study the large-scale structure of the solar corona on the basis of solar wind measurements.
Dynamics of heavy ion fluxes in the solar wind and certain characteristics of the solar corona.
Dynamics of heavy ion fluxes of the solar wind and some characteristics of the solar corona.
Erratm: "A new method to study the large-scale structure of the solar corona on the basis of solar wind measurments" [Kosm. Issled., Tom 28, Vyp. 6, p. 890 - 902 (Nov-Dec 1990)].
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