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Resolving the HONO formation mechanism in the ionosphere via ab initio molecular dynamic simulations
Solar emission produces copious nitrosonium ions (NO(+)) in the D layer of the ionosphere, 60 to 90 km above the Earth’s surface. NO(+) is believed to transfer its charge to water clusters in that region, leading to the formation of gaseous nitrous acid (HONO) and protonated water cluster. The dynam...
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| 出版年: | Proc Natl Acad Sci U S A |
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| 主要な著者: | , , , , , |
| フォーマット: | Artigo |
| 言語: | Inglês |
| 出版事項: |
National Academy of Sciences
2016
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| 主題: | |
| オンライン･アクセス: | https://ncbi.nlm.nih.gov/pmc/articles/PMC4855577/ https://ncbi.nlm.nih.gov/pubmed/27071120 https://ncbi.nlm.nih.govhttp://dx.doi.org/10.1073/pnas.1601651113 |
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