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

Author:

Dawkins E. C. M.12ORCID,Stober G.3ORCID,Janches D.1ORCID,Carrillo‐Sánchez J. D.12ORCID,Lieberman R. S.1ORCID,Jacobi C.4ORCID,Moffat‐Griffin T.5ORCID,Mitchell N. J.56ORCID,Cobbett N.5,Batista P. P.7ORCID,Andrioli V. F.78ORCID,Buriti R. A.9ORCID,Murphy D. J.10ORCID,Kero J.11ORCID,Gulbrandsen N.12ORCID,Tsutsumi M.1314ORCID,Kozlovsky A.15ORCID,Kim J. H.16ORCID,Lee C.16ORCID,Lester M.17ORCID

Affiliation:

1. ITM Physics Laboratory NASA Goddard Space Flight Center Greenbelt MD USA

2. Department of Physics Catholic University of America Washington DC USA

3. Microwave Physics Institute of Applied Physics University Bern Bern Switzerland

4. Institute for Meteorology Leipzig University Leipzig Germany

5. British Antarctic Survey Cambridge UK

6. University of Bath Bath UK

7. National Institute for Space Research (INPE) São José dos Campos Brazil

8. China‐Brazil Joint Laboratory for Space Weather NSSC/INPE São José dos Campos Brazil

9. Department of Physics Federal University of Campina Grande Campina Grande Brazil

10. Australian Antarctic Division Kingston TAS Australia

11. Swedish Institute of Space Physics (IRF) Kiruna Sweden

12. Tromsø Geophysical Observatory UiT—The Arctic University of Norway Tromsø Norway

13. National Institute of Polar Research Tachikawa Japan

14. The Graduate University for Advanced Studies (SOKENDAI) Tokyo Japan

15. Sodankylä Geophysical Observatory University of Oulu Oulu Finland

16. Division of Atmospheric Sciences Korea Polar Research Institute Incheon S. Korea

17. Department of Physics and Astronomy University of Leicester Leicester UK

Abstract

AbstractThe 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.

Funder

Heliophysics Division

Korea Polar Research Institute

Deutsche Forschungsgemeinschaft

Science and Technology Facilities Council

Natural Environment Research Council

NASA Engineering and Safety Center

Australian Antarctic Division

Publisher

American Geophysical Union (AGU)

Subject

General Earth and Planetary Sciences,Geophysics

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