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Solar Cycle and Long‐Term Trends in the Observed Peak of the Meteor Altitude Distributions by Meteor Radars

Dawkins, E.C.M.; Stober, G.; Janches, D.; Carrillo‐Sánchez, J.D.; Lieberman, R.S.; Jacobi, C.; Moffat-Griffin, T. ORCID: https://orcid.org/0000-0002-9670-6715; Mitchell, N.J.; Cobbett, N.; Batista, P.P.; Andrioli, V.F.; Buriti, R.A.; Murphy, D.J.; Kero, J.; Gulbrandsen, N.; Tsutsumi, M.; Kozlovsky, A.; Kim, J.H.; Lee, C.; Lester, M.. 2023 Solar Cycle and Long‐Term Trends in the Observed Peak of the Meteor Altitude Distributions by Meteor Radars. Geophysical Research Letters, 50 (2), e2022GL101953. 11, pp. 10.1029/2022GL101953

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© 2022 Commonwealth of Australia and The Authors. This article has been contributed to by U.S. Government employees and their work is in the public domain in the USA.
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Abstract/Summary

The mesosphere/lower thermosphere (MLT, 80–100 km) region is an important boundary between Earth's atmosphere below and space above and may act as a sensitive indicator for anthropogenic climate change. Existing observational and modeling studies have shown the middle atmosphere and the MLT is cooling and contracting because of increasing greenhouse gas emissions. However, trend analyses are highly sensitive to the time periods covered, their length, and the measurement type and methodology used. We present for the first time the linear and 11-year solar cycle responses in the meteor ablation altitude distributions observed by 12 meteor radars at different locations. Decreasing altitudes were seen at all latitudes (linear trends varying from −10.97 to −817.95 m dec−1), and a positive correlation with solar activity was seen for most locations. The divergence of responses at high latitudes indicates an important and complex interplay between atmospheric changes and dynamics at varying time scales.

Item Type: Publication - Article
Digital Object Identifier (DOI): 10.1029/2022GL101953
ISSN: 0094-8276
Additional Keywords: meteor, altitude, mesosphere, meteor radar, climate change, mesopause
Date made live: 26 Jan 2023 12:21 +0 (UTC)
URI: https://nora.nerc.ac.uk/id/eprint/533919

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