HETEROGENEOUS STRUCTURE OF THE SURFACE OF PARTICLES OF THE LUNAR REGOLITH. A LUNA-16 SAMPLE

dc.contributor.author	Dikov Y.P.
dc.contributor.author	Ivanov A.V.
dc.contributor.author	Barsukov V.L.
dc.contributor.author	Rekharskiy V.I.
dc.contributor.author	Vasil'yev O.V.
dc.date.accessioned	2020-10-09T09:00:45Z
dc.date.available	2020-10-09T09:00:45Z
dc.date.issued	1989
dc.identifier	https://elibrary.ru/item.asp?id=31148961
dc.identifier.citation	Transactions (Doklady) of the USSR Academy of Sciences. Earth Science Sections, 1989, , 2, 217-220
dc.identifier.issn	0891-5571
dc.identifier.uri	https://repository.geologyscience.ru/handle/123456789/17883
dc.description.abstract	One of the most effective methods of studying the surfaces of particles in samples of the lunar regolith is X-ray photoelectron spectroscopy. In this investigation, an ES-2401 instrument was used for X-ray photoelectron spectroscopy. The particles are multilayered and bear the traces of a variety of processes that influenced regolith development on the moon: evaporation as a result of a meteorite impact, followed by condensation of target material, development of endogenetic gas condensates, condensation of evaporated meteorite material, and reduction of the particle surface by the solar wind.
dc.title	HETEROGENEOUS STRUCTURE OF THE SURFACE OF PARTICLES OF THE LUNAR REGOLITH. A LUNA-16 SAMPLE
dc.type	Статья

Files in this item

Files	Size	Format	View
There are no files associated with this item.