Zobrazeno 1 - 10
of 67
pro vyhledávání: '"Natalia Artemieva"'
Autor:
Alessandro Morbidelli, Qing-Zhu Yin, Harry Becker, Natalia Artemieva, Wladimir Neumann, Kai Wünnemann, Gregory J. Archer, Meng-Hua Zhu, David C. Rubie, James M.D. Day
Publikováno v:
Nature Astronomy. 5:1286-1296
Abundances of the highly siderophile elements (HSEs) in silicate portions of Earth and the Moon provide constraints on the impact flux to both bodies, but only since ~100 Myr after the beginning of the Solar System (hereafter tCAI). The earlier impac
Autor:
E. D. Podobnaya, O. P. Popova, Natalia Artemieva, Vladimir Svetsov, Vladimir V Shuvalov, D. O. Glazachev
Publikováno v:
Izvestiya, Physics of the Solid Earth. 57:698-709
—Destruction on the Earth’s surface caused by a shock wave is one of the most important and dangerous effects from asteroid and comet impacts. The overpressure and wind speed behind the shock wave front, leading to various dangerous effects, can
Autor:
M Van Ginneken, Bastien Soens, Eduardo Bolea-Fernandez, Natalia Artemieva, Stepan M. Chernonozhkin, Luigi Folco, Frank Vanhaecke, Ph. Claeys, C González de Vega, Joke Belza, Steven Goderis, Billy P. Glass, Matthew J. Genge
Publikováno v:
Nature Communications, Vol 12, Iss 1, Pp 1-12 (2021)
Nature Communications
Nature Communications
Fractionation effects related to evaporation and condensation had a major impact on the current elemental and isotopic composition of the Solar System. Although isotopic fractionation of moderately volatile elements has been observed in tektites due
Autor:
Thomas Kenkmann, Natalia Artemieva
Publikováno v:
Meteoritics & Planetary Science. 56:1024-1070
The number of newly discovered and confirmed impact structures on earth is growing continuously. In this review paper, the main attributes of 198 confirmed impact structures and 10 further structures, for which final confirmation based on the identif
Autor:
M. N. Rao, L. E. Nyquist, P. D. Asimow, D. K. Ross, S. R. Sutton, T. H. See, C. Y. Shih, D. H. Garrison, S. J. Wentworth, J. Park, Natalia Artemieva
Large impact-melt pockets in shergottites contain both Martian regolith components and sulfide/sulfite bleb clusters that yield high sulfur concentrations locally compared to bulk shergottites. The regolith may be the source of excess sulfur in the s
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::1f838d7438fd0dee9a923724cf6d2ff8
https://resolver.caltech.edu/CaltechAUTHORS:20211209-456542000
https://resolver.caltech.edu/CaltechAUTHORS:20211209-456542000
Autor:
Matthias Van Ginneken, Steven Goderis, Natalia Artemieva, Vinciane Debaille, Sophie Decrée, Ralph Harvey, Katherine Huwig, Lutz Hecht, Shuying Yang, Felix Kaufmann, Bastien Soens, Munir Humayun, Flore Van Maldeghem, Matthew Genge, Philippe Claeys
Introduction: Impactors several tens up to 200 m in size are likely to suffer complete disruption and to produce large airbursts, similarly to the Tunguska event over Russia in 1908 [e.g., 1]. Observations and numerical modeling of medium sized impac
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::57704432b483ad6af18018c29ab9901c
https://doi.org/10.5194/epsc2021-679
https://doi.org/10.5194/epsc2021-679
Description of the CdC Campo del Cielo (CdC, Figure 1) is a 4000-year-old [1, 2] strewn field in the south of the Chaco province, Argentina, which was caused by an impact of IA iron octahedrite [3]. This strewn field has an extremely elongated patter
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::fd6c305dc776ce73addbd29eb78a9200
https://doi.org/10.5194/epsc2021-106
https://doi.org/10.5194/epsc2021-106
Publikováno v:
Icarus. 333:71-86
Fine dust from impact ejecta settles slowly in an atmosphere, whereas large chunks of ejecta easily traverse the surrounding gas on nearly parabolic trajectories. In order to study the effects of the interaction of impact ejecta with an atmosphere, w
Publikováno v:
Icarus. 327:60-71
In this paper we present the results of numerical modeling of the Chelyabinsk dust train during the first 3 min after the meteoroid entry which are in qualitative agreement with observations. Then we analyze the possibility of plume formation after i
Autor:
Felix E. D. Kaufmann, S. Yang, K. A. Huwig, Natalia Artemieva, Sophie Decrée, Vinciane Debaille, Ralph P. Harvey, Bastien Soens, M. van Ginneken, Ph. Claeys, Matthew J. Genge, Steven Goderis, Munir Humayun, F. van Maldeghem, Lutz Hecht
Publikováno v:
Science Advances
Science advances, 7 (14
Science advances, 7 (14
Large airbursts, the most frequent hazardous impact events, are estimated to occur orders of magnitude more frequently than crater-forming impacts. However, finding traces of these events is impeded by the difficulty of identifying them in the recent
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::8aaf2179145b8b0037aaf5b5e176f1ba