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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...
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| Hauptverfasser: | , , , , , , |
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| Format: | Artigo |
| Sprache: | Inglês |
| Veröffentlicht: |
National Academy of Sciences
2014
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| 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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