Preprints
https://doi.org/10.5194/egusphere-2026-2356
https://doi.org/10.5194/egusphere-2026-2356
30 Apr 2026
 | 30 Apr 2026
Status: this preprint is open for discussion and under review for Atmospheric Chemistry and Physics (ACP).

Meteoroids as a source of metal ion clouds in Earth’s upper thermosphere

Gang Chen, Yimeng Xu, Guotao Yang, Wuhu Feng, Jiyao Xu, Shaodong Zhang, Guozhu Li, Hanxian Fang, Lifang Du, Haoran Zheng, Xuewu Cheng, Faquan Li, Yuchang Xun, Kaiming Huang, and Chunxiao Yan

Abstract. Advances in lidar technology have enabled the detection of Metal Ion Clouds (MICs) at altitudes between 120–300 km in the Earth’s thermosphere. Observations from a Ca+ lidar in Beijing, China, reveal that these MICs are characterized by tightly packed, stripe-like structures that span extensive areas, covering hundreds to thousands of square kilometers. Some of these stripes extend downward to the Main Metal Layer (MML) around 100 km, and some clouds descend with tidal winds and merge into the underlying MML. While arriving the altitudes of Mesosphere and Low-Thermosphere (MLT), they lead to an increase in Sporadic-E (Es) layer density, and even trigger the formation of a new Es layer. The metal ions in the upper thermosphere will eventually sink into the MML and significantly affect its density variations. The striped structure of MICs and their direct effects on Es and MML suggest they originate from meteoroid trails, challenging traditional views on meteoric input.

Competing interests: The contact author has declared that none of the authors has any competing interests.

Publisher's note: Copernicus Publications remains neutral with regard to jurisdictional claims made in the text, published maps, institutional affiliations, or any other geographical representation in this paper. While Copernicus Publications makes every effort to include appropriate place names, the final responsibility lies with the authors. Views expressed in the text are those of the authors and do not necessarily reflect the views of the publisher.
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Gang Chen, Yimeng Xu, Guotao Yang, Wuhu Feng, Jiyao Xu, Shaodong Zhang, Guozhu Li, Hanxian Fang, Lifang Du, Haoran Zheng, Xuewu Cheng, Faquan Li, Yuchang Xun, Kaiming Huang, and Chunxiao Yan

Status: open (until 11 Jun 2026)

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Gang Chen, Yimeng Xu, Guotao Yang, Wuhu Feng, Jiyao Xu, Shaodong Zhang, Guozhu Li, Hanxian Fang, Lifang Du, Haoran Zheng, Xuewu Cheng, Faquan Li, Yuchang Xun, Kaiming Huang, and Chunxiao Yan
Gang Chen, Yimeng Xu, Guotao Yang, Wuhu Feng, Jiyao Xu, Shaodong Zhang, Guozhu Li, Hanxian Fang, Lifang Du, Haoran Zheng, Xuewu Cheng, Faquan Li, Yuchang Xun, Kaiming Huang, and Chunxiao Yan
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Latest update: 01 May 2026
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Short summary
A new lidar for calcium ion (Ca+) observations has been operated in Yanqing, Beijing, China. Cloud-like Ca+ are observed to occur at altitudes of 120–300 km, and these clouds are composed of striped structures. These Ca+ are found to descend into Es layer and the main metal layer, and increase their ion density. According to the stripe-like structures and their influence on the metal ion layers, we believe that these metal ions observed by the lidar in Beijing come from meteoroids trails
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