Abstract

Observations of the mesospheric Ni layer have been performed by lidar in January-March 2018 at Kuehlungsborn/Germany (54°N, 12°E). These soundings provide only the second Ni data set after initial observations by Collins et al. at Chatanika/Alaska (65°N, 147°W)[1]. We utilized for the first time a transition from the low-lying excited Ni(3D) state at 341 nm. For all soundings, nightly mean peak densities varied between ~280 cm−3 and 450 cm3, which is a factor of ~40 less than previously reported for Chatanika [1]. The observed Ni abundance is especially important if compared with the abundance of other metals like Fe, and with their respective abundances in evaporating meteoroids, which form the source of the metal layer in the upper mesosphere. Here, we present exemplarily a sounding from January 8, 2018. Beside the Ni raw data and density profiles we show a temperature profile as measured simultaneously be the co-located RMR lidar and the temperature variation due to gravity waves and tides.

Highlights

  • Ablation of meteoroids entering the Earth’s atmosphere forms a metal layer between ~80 and 110 km

  • Lidar observations of the metal concentrations as well as measurements of chemical reaction rates and modelling of meteoroid heating revealed a complex interplay of different factors determining the height-dependent concentrations of the particular metal atoms [10]

  • Simultaneous soundings with a co-located RMR lidar provided independent temperature observations and allowed to deduce information about activity of gravity and tidal waves for that night

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Summary

Introduction

Ablation of meteoroids entering the Earth’s atmosphere forms a metal layer between ~80 and 110 km. Lidar observations of the metal concentrations as well as measurements of chemical reaction rates and modelling of meteoroid heating revealed a complex interplay of different factors determining the height-dependent concentrations of the particular metal atoms [10]. They observed peak densities of ~16,000 cm-3 and a total abundance of 2.7 x 10-10 cm-2, which is about 0.8 times the typical Fe abundance at this site.

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