Models of lunar dust motion dynamics and methods of producing streams of charged dust particles in a laboratory environment

Abstract

The article presents basic physical parameters of lunar dust, models of its motion over the surface of the moon under the influence of space environment factors and a review of methods for obtaining dust streams in a laboratory environment.

About the authors

N. D. Syomkin

Samara State Aerospace University

Author for correspondence.
Email: semkin@ssau.ru

Doctor of Technical Science

Professor of the Department of Radio Engineering and Medical Diagnostic Systems

Russian Federation

A. S. Vidmanov

Samara State Aerospace University

Email: jkt13@rambler.ru

Postgraduate Student of the Department of Radio Engineering and Medical Diagnostic Systems

Russian Federation

References

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