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- W3023212311 abstract "The ablation of interplanetary dust particles is the source of the metal atoms – Na, Fe, Mg, K, and Ca – that occur in layers between 80 and 100 km. The relative abundances of these metal atoms are quite different from their relative abundances in chondritic meteorites, mostly because elements ablate with widely different efficiencies. Sporadic E layers are concentrated layers of metallic ions and electrons that occur above 90 km and have an important influence on radio communications. Meteoric smoke particles, formed by the condensation of metallic compounds, are the major source of nuclei for noctilucent clouds." @default.
- W3023212311 created "2020-05-13" @default.
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- W3023212311 date "2003-01-01" @default.
- W3023212311 modified "2023-09-27" @default.
- W3023212311 title "MESOSPHERE | Metal Layers" @default.
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- W3023212311 doi "https://doi.org/10.1016/b0-12-227090-8/00218-9" @default.
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