Solar Cycle and Long‐Term Trends in the Observed Peak of the Meteor Altitude Distributions by Meteor Radars
E. C. M. Dawkins, Gunter Stober, Diego Janches, Juan Diego Carrillo‐Sánchez, R. S. Lieberman, Christoph Jacobi, Tracy Moffat‐Griffin, N. J. Mitchell, Neil Cobbett, P. P. Batista, V. F. Andrioli, R. A. Buriti, D. J. Murphy, Johan Kero, Njål Gulbrandsen, Masaki Tsutsumi, Alexander Kozlovsky, Jeong‐Han Kim, Chang-Sup Lee, M. Lester
Abstract
Abstract 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.