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.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.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.title | HETEROGENEOUS STRUCTURE OF THE SURFACE OF PARTICLES OF THE LUNAR REGOLITH. A LUNA-16 SAMPLE | |
| dc.type | Статья |