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Sihane Merouane

Explore the profile of Sihane Merouane including associated specialties, affiliations and a list of published articles. Areas
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Articles 6
Citations 41
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Recent Articles
1.
Levasseur-Regourd A, Agarwal J, Cottin H, Engrand C, Flynn G, Fulle M, et al.
Space Sci Rev . 2022 Jan; 214. PMID: 35095119
This review presents our understanding of cometary dust at the end of 2017. For decades, insight about the dust ejected by nuclei of comets had stemmed from remote observations from...
2.
Varmuza K, Filzmoser P, Fray N, Cottin H, Merouane S, Stenzel O, et al.
J Chemom . 2020 May; 34(4):e3218. PMID: 32355406
The instrument COSIMA (COmetary Secondary Ion Mass Analyzer) onboard of the European Space Agency mission Rosetta collected and analyzed dust particles in the neighborhood of comet 67P/Churyumov-Gerasimenko. The chemical composition...
3.
Hilchenbach M, Fischer H, Langevin Y, Merouane S, Paquette J, Ryno J, et al.
Philos Trans A Math Phys Eng Sci . 2017 May; 375(2097). PMID: 28554975
The cometary dust particle instrument COSIMA (COmetary Secondary Ion Mass Analyser) onboard ESA's Rosetta mission has collected about 31 000 dust particles in the inner coma of comet 67P/Churyumov-Gerasimenko since...
4.
Fray N, Bardyn A, Cottin H, Altwegg K, Baklouti D, Briois C, et al.
Nature . 2016 Sep; 538(7623):72-74. PMID: 27602514
The presence of solid carbonaceous matter in cometary dust was established by the detection of elements such as carbon, hydrogen, oxygen and nitrogen in particles from comet 1P/Halley. Such matter...
5.
Schulz R, Hilchenbach M, Langevin Y, Kissel J, Silen J, Briois C, et al.
Nature . 2015 Jan; 518(7538):216-8. PMID: 25624103
Comets are composed of dust and frozen gases. The ices are mixed with the refractory material either as an icy conglomerate, or as an aggregate of pre-solar grains (grains that...
6.
Binzel R, Morbidelli A, Merouane S, Demeo F, Birlan M, Vernazza P, et al.
Nature . 2010 Jan; 463(7279):331-4. PMID: 20090748
Telescopic measurements of asteroids' colours rarely match laboratory reflectance spectra of meteorites owing to a 'space weathering' process that rapidly reddens asteroid surfaces in less than 10(6) years. 'Unweathered' asteroids...