2021
DOI: 10.1016/j.jqsrt.2020.107468
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Lidar observations of the upper atmospheric nickel layer at Beijing (40N,116E

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Cited by 8 publications
(12 citation statements)
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“…One dye laser excites the Na resonance fluorescence transition at 589 nm (Jiao et al., 2015). The second is frequency‐doubled to produce light at 341 nm with an average pulse energy of ∼30 mJ, which is used for Ni resonance fluorescence scattering (Wu et al., 2021). A 1200‐mm‐diameter Cassegrain telescope, coupled with the receiver unit (optical filters, photomultiplier tubes, and photon counters), detects Rayleigh scattering from air molecules and resonant fluorescence scattering from the Ni and Na layers.…”
Section: Methodsmentioning
confidence: 99%
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“…One dye laser excites the Na resonance fluorescence transition at 589 nm (Jiao et al., 2015). The second is frequency‐doubled to produce light at 341 nm with an average pulse energy of ∼30 mJ, which is used for Ni resonance fluorescence scattering (Wu et al., 2021). A 1200‐mm‐diameter Cassegrain telescope, coupled with the receiver unit (optical filters, photomultiplier tubes, and photon counters), detects Rayleigh scattering from air molecules and resonant fluorescence scattering from the Ni and Na layers.…”
Section: Methodsmentioning
confidence: 99%
“…The initial measurements of the Ni layer made by this lidar were analyzed by Wu et al. (2021): for 25 nights of measurements, the Ni peak density ranged from 98 to 460 cm −3 with the peak altitude between 80 and 88 km. In the present paper, this initial data set is substantially increased: from April 2019 to March 2020 and April 2021 to August 2021, we obtained 1090 hr of Ni and Na number density data, covering 126 nights of observations at Yanqing.…”
Section: Methodsmentioning
confidence: 99%
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