Open AccessПодъем пылевых частиц при воздействии лазерного излучения на хондритовую мишень и возможность моделирования плазменно-пылевых процессов у поверхности Луны
Author(s) -
И.Н. Бурдонский,
А.Г. Леонов,
В.Н. Юфа,
А.П. Голубь,
С.И. Попель,
А.М. Садовский
Publication year - 2020
Publication title -
pisʹma v žurnal tehničeskoj fiziki
Language(s) - English
Resource type - Journals
eISSN - 1726-7471
pISSN - 0320-0116
DOI - 10.21883/pjtf.2020.20.50157.18362
Subject(s) - meteoroid , regolith , astrobiology , talc , shock wave , surface (topology) , materials science , nonlinear system , mechanics , physics , composite material , geometry , mathematics , quantum mechanics
The results of the first study on experimental modeling of the rise of dust particles by a shock wave above a target surface, performed on the Saturn installation, are presented. The interaction of laser radiation with a porous chondritic target, the surface of which contains fine particles of talc, is investigated. The results of experimental modeling can be used to describe the rise of dust particles from zones of nonlinear and linear elastic deformations of the regolith material, which characterize the impact of the meteoroid on the surface of the Moon.