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Detection of solar wind-produced water in irradiated rims on silicate minerals

The solar wind (SW), composed of predominantly ∼1-keV H(+) ions, produces amorphous rims up to ∼150 nm thick on the surfaces of minerals exposed in space. Silicates with amorphous rims are observed on interplanetary dust particles and on lunar and asteroid soil regolith grains. Implanted H(+) may re...

Ausführliche Beschreibung

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Bibliographische Detailangaben
Hauptverfasser: Bradley, John P., Ishii, Hope A., Gillis-Davis, Jeffrey J., Ciston, James, Nielsen, Michael H., Bechtel, Hans A., Martin, Michael C.
Format: Artigo
Sprache:Inglês
Veröffentlicht: National Academy of Sciences 2014
Schlagworte:
Online Zugang:https://ncbi.nlm.nih.gov/pmc/articles/PMC3918814/
https://ncbi.nlm.nih.gov/pubmed/24449869
https://ncbi.nlm.nih.govhttp://dx.doi.org/10.1073/pnas.1320115111
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