Climatology of Interhemispheric Mesopause Temperatures Using the High‐Latitude and Middle‐Latitude Meteor Radars

Author:

Yi Wen1234ORCID,Xue Xianghui134ORCID,Reid Iain M.56ORCID,Murphy Damian J.7ORCID,Hall Chris M.8ORCID,Tsutsumi Masaki9ORCID,Ning Baiqi10,Li Guozhu10ORCID,Yang Guotao2ORCID,Li Na11ORCID,Chen Tingdi134ORCID,Dou Xiankang112ORCID

Affiliation:

1. CAS Key Laboratory of Geospace Environment School of Earth and Space Sciences University of Science and Technology of China Hefei China

2. State Key Laboratory of Space Weather Chinese Academy of Sciences Beijing China

3. CAS Center for Excellence in Comparative Planetology Hefei China

4. Mengcheng National Geophysical Observatory School of Earth and Space Sciences University of Science and Technology of China Hefei China

5. ATRAD Pty Ltd. Thebarton SA Australia

6. School of Physical Sciences University of Adelaide Adelaide SA Australia

7. Australian Antarctic Division Kingston Tasmania Australia

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

9. National Institute of Polar Research Tachikawa Japan

10. Key Laboratory of Earth and Planetary Physics Institute of Geology and Geophysics Chinese Academy of Sciences Beijing China

11. National Key Laboratory of Electromagnetic Environment China Research Institute of Radiowave Propagation Qingdao China

12. Electronic Information School, Wuhan University Wuhan China

Funder

National Natural Science Foundation of China

Publisher

American Geophysical Union (AGU)

Subject

Space and Planetary Science,Earth and Planetary Sciences (miscellaneous),Atmospheric Science,Geophysics

Reference50 articles.

1. Long‐term distribution of meteors in a solar cycle period observed by VHF meteor radars at near‐equatorial latitudes;Batubara M.;Journal of Geophysical Research: Space Physics,2018

2. Comparison of simultaneous wind measurements using colocated VHF meteor radar and MF spaced antenna radar systems

3. Comparison of atmospheric parameters derived from meteor observations with CIRA

4. A comparison of ambipolar diffusion coefficients in meteor trains using VHF radar and UV lidar

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