RUS  ENG
Full version
JOURNALS // Pis'ma v Zhurnal Èksperimental'noi i Teoreticheskoi Fiziki // Archive

Pis'ma v Zh. Èksper. Teoret. Fiz., 2012 Volume 95, Issue 4, Pages 198–204 (Mi jetpl2441)

This article is cited in 55 papers

PLASMA, HYDRO- AND GAS DYNAMICS

Dusty plasma system in the surface layer of the illuminated part of the moon

A. P. Golub'a, G. G. Dol'nikovb, A. V. Zakharovb, L. M. Zelenyib, Yu. N. Izvekovaa, S. I. Kopnina, S. I. Popela

a Institute of Dynamics of Geospheres, Russian Academy of Sciences, Moscow
b Space Research Institute, Russian Academy of Sciences, Moscow

Abstract: The dusty plasma system in the surface layer of the illuminated part of the Moon has been considered. The maximum height of the dust rise has been determined. It has been shown that a dead zone, where dust particles cannot rise over the surface of the Moon, is absent near a lunar latitude of $80^\circ$. The size and height distributions of dust have been determined.

Received: 11.01.2012
Revised: 23.01.2012


 English version:
Journal of Experimental and Theoretical Physics Letters, 2012, 95:4, 182–187

Bibliographic databases:


© Steklov Math. Inst. of RAS, 2024