Preprints
https://doi.org/10.5194/egusphere-2024-1259
https://doi.org/10.5194/egusphere-2024-1259
30 Apr 2024
 | 30 Apr 2024
Status: this preprint is open for discussion and under review for Atmospheric Chemistry and Physics (ACP).

Dominant role of charged meteoric smoke particles in the polar mesospheric clouds

Liang Zhang, Zhongfang Liu, and Brian Tinsley

Abstract. Polar mesospheric clouds (PMCs), composed of ice particles, are sensitive to solar activity and atmospheric dynamics, and have been suggested as a potential indicator of climate change. However, the microphysical processes of PMCs, especially the mechanism of ice nucleation, remain poorly understood. This study presents an analysis of satellite PMC data, which reveals that the mean ice particle radius (r) and concentration (N) in PMCs are primarily influenced by the PMC height (h), rather than by the mean environment temperature (T). Additionally, the ice particle column concentration (Nc) exhibits a surprising decrease with latitude. These results support the hypothesis that charged meteoric smoke particles (MSPs) act as ice nuclei, based on which we propose the charged-MSPs nucleation (CMN) scheme for the PMC formation. In contrast to the conventional growth-sedimentation (GS) scheme, in the CMN scheme the nucleation occurs throughout the PMC altitude range, ice particles grow mainly in situ, and the ice particle radius is determined by the competition for the limited water vapor rather than by sedimentation. The CMN scheme provides new pathways for solar activity and atmospheric dynamics to affect PMCs, and can explain a number of puzzling phenomena in the GS scheme.

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Liang Zhang, Zhongfang Liu, and Brian Tinsley

Status: open (until 11 Jun 2024)

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Liang Zhang, Zhongfang Liu, and Brian Tinsley
Liang Zhang, Zhongfang Liu, and Brian Tinsley

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Short summary
This study finds that ice particles are sensitive to PMC height rather than temperature, based on which the CMN scheme is proposed for PMC formation. The concentration of charged-MSPs rapidly increases with altitude in line with electrons, and the competition for the limited water vapor results in the opposite distribution of ice particle radius. The CMN scheme provides explanations for a number of puzzling phenomena, and new pathways for solar activity and atmospheric dynamics to affect PMCs.