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- W1775981192 abstract "Abstract Ground‐based resonance lidar has been used to detect the mesospheric nickel (Ni) layer. The Ni layer is detected through absorption in the 3d 8 ( 3 F)4s 2 → 3d 9 ( 2 D)4p transition at 337.1 nm and reemission in both the 3d 9 ( 2 D)4p → 3d 8 ( 3 F)4s 2 and 3d 9 ( 2 D)4p → 3d 9 ( 2 D)4s transitions at 337.1 and 339.4 nm, respectively. Results from wintertime lidar observations on two nights (27–28 November and 20–21 December 2012) at Chatanika, Alaska (65°N, 147°W), are presented. The wintertime Ni layer has a peak concentration of 1.6 × 10 4 cm −3 at 87 km, with a column abundance of 2.7 × 10 10 cm −2 , centroid height of 88 km, and root‐mean‐square width of 6.4 km. The midwinter abundance of mesospheric iron (Fe) at Chatanika is 3.4 × 10 10 cm −2 , indicating a ratio of Fe to Ni of 1.2 in the upper atmosphere. This is significantly lower than the value of 18 for the ratio of Fe to Ni in chondrite meteorites." @default.
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- W1775981192 date "2015-01-28" @default.
- W1775981192 modified "2023-10-14" @default.
- W1775981192 title "First lidar observation of the mesospheric nickel layer" @default.
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- W1775981192 doi "https://doi.org/10.1002/2014gl062716" @default.
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