Metal layer depletion during the super substorm on 4 November 2021

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Publicado en:Atmospheric Chemistry and Physics vol. 25, no. 21 (2025), p. 14763-14776
Autor principal: Chen, Gang
Otros Autores: Xu, Yimeng, Yang, Guotao, Zhang, Shaodong, Ren, Zhipeng, Hu, Pengfei, Yu, Tingting, Wu, Fuju, Du, Lifang, Zheng, Haoran, Cheng, Xuewu, Li, Faquan, Zhang, Min
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024 7 |a 10.5194/acp-25-14763-2025  |2 doi 
035 |a 3268540327 
045 2 |b d20251101  |b d20251114 
084 |a 123615  |2 nlm 
100 1 |a Chen, Gang  |u School of Earth and Space Science and Technology, Wuhan University, Wuhan 430072, China 
245 1 |a Metal layer depletion during the super substorm on 4 November 2021 
260 |b Copernicus GmbH  |c 2025 
513 |a Journal Article 
520 3 |a Metal layer forms as a result of meteoric ablation and exist as a layer of metal elements between approximately 80 and 105 km altitude, and it provides information about the physics and chemistry of the boundary between the atmosphere and space. There are some studies about the wind field disturbances in Mesosphere and Low Thermosphere (MLT) region and the plasma variations in ionospheric E-region during magnetic storms, but no study on the impact of storms on the metal atom layers in mesosphere. During the super substorm on 4 November 2021, the atmospheric metal layers were observed to decrease by observations from three lidars at the mid-latitudes of China. The Na, Ca and Ni densities on the storm day were significantly lower than in other days in October and November. The <inline-formula><mml:math display="inline" id="M1"><mml:mrow class="chem"><mml:mi mathvariant="normal">O</mml:mi><mml:mo>/</mml:mo><mml:msub><mml:mi mathvariant="normal">N</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> column density ratio observed by the Global Ultraviolet Imager (GUVI) on the storm day was much higher than on quiet days, and the numerical simulation results demonstrate a substantial increase in atomic oxygen density at the heights of the metal layer. The increase in oxygen density may lead to the formation of more metal compounds, thus more metal atoms are consumed. This is an interesting phenomenon that magnetic storm can perturb the atmospheric metal layer through chemical reactions. 
653 |a E region 
653 |a Mesosphere 
653 |a Wind fields 
653 |a Chemical reactions 
653 |a Metals 
653 |a Heavy metals 
653 |a Ablation 
653 |a Altitude 
653 |a Thermosphere 
653 |a Physics 
653 |a Ionosphere 
653 |a Atomic oxygen 
653 |a General circulation models 
653 |a Lower mantle 
653 |a Storms 
653 |a Magnetic storms 
653 |a Metal compounds 
653 |a Numerical simulations 
653 |a Lasers 
653 |a Density ratio 
653 |a Meteors & meteorites 
653 |a Geomagnetic storms 
653 |a Ultraviolet imagery 
653 |a Mathematical models 
653 |a Atoms & subatomic particles 
653 |a Oxygen 
653 |a Environmental 
700 1 |a Xu, Yimeng  |u School of Earth and Space Science and Technology, Wuhan University, Wuhan 430072, China 
700 1 |a Yang, Guotao  |u National Space Science Center, Chinese Academy of Sciences, Beijing 100190, China 
700 1 |a Zhang, Shaodong  |u School of Earth and Space Science and Technology, Wuhan University, Wuhan 430072, China; School of Physics and Electronic Science, Guizhou Normal University, Guiyang 550025, China 
700 1 |a Ren, Zhipeng  |u Key Laboratory of Earth and Planetary Physics, Institute of Geology and Geophysics, Chinese Academy of Sciences, Beijing 100029, China 
700 1 |a Hu, Pengfei  |u School of Earth and Space Science and Technology, Wuhan University, Wuhan 430072, China 
700 1 |a Yu, Tingting  |u Key Laboratory of Earth and Planetary Physics, Institute of Geology and Geophysics, Chinese Academy of Sciences, Beijing 100029, China 
700 1 |a Wu, Fuju  |u School of Physics, Henan Normal University, Xinxiang 453007, China 
700 1 |a Du, Lifang  |u National Space Science Center, Chinese Academy of Sciences, Beijing 100190, China 
700 1 |a Zheng, Haoran  |u National Space Science Center, Chinese Academy of Sciences, Beijing 100190, China 
700 1 |a Cheng, Xuewu  |u Innovation Academy for Precision Measurement Science and Technology, Chinese Academy of Sciences, Wuhan 430071, China 
700 1 |a Li, Faquan  |u Innovation Academy for Precision Measurement Science and Technology, Chinese Academy of Sciences, Wuhan 430071, China 
700 1 |a Zhang, Min  |u School of Earth and Space Science and Technology, Wuhan University, Wuhan 430072, China 
773 0 |t Atmospheric Chemistry and Physics  |g vol. 25, no. 21 (2025), p. 14763-14776 
786 0 |d ProQuest  |t Advanced Technologies & Aerospace Database 
856 4 1 |3 Citation/Abstract  |u https://www.proquest.com/docview/3268540327/abstract/embedded/CH9WPLCLQHQD1J4S?source=fedsrch 
856 4 0 |3 Full Text  |u https://www.proquest.com/docview/3268540327/fulltext/embedded/CH9WPLCLQHQD1J4S?source=fedsrch 
856 4 0 |3 Full Text - PDF  |u https://www.proquest.com/docview/3268540327/fulltextPDF/embedded/CH9WPLCLQHQD1J4S?source=fedsrch