Long‐Term Trends of the Meteor Altitude Distribution, Mesospheric density and Gravity Wave Momentum Flux Observed by the high-latitude meteor radars
ID:3211 View Protection:ATTENDEE Updated Time:2024-04-12 23:14:22 Hits:1925 Invited speech

Start Time:2024-05-18 15:20(Asia/Shanghai)

Duration:10min

Session:S10 主题10、行星科学与空间物理 » S10-1主题10、行星科学与空间物理 专题10.10、专题10.11(18日下午,4F国际会议厅)

No files

Abstract
The mesosphere and lower thermosphere (MLT) region is strongly modulated by gravity wave (GW) perturbations, and the momentum flux of GW is essential in quantitatively understanding and modeling atmospheric structure at all altitudes. In this study, we present the seasonal variations, long-trend of mesospheric density and GW momentum flux observed by the meteor radars at Davis Station (68.6°S, 77.9°E), in Antarctica, Svalbard (78.3°N, 16°E), Tromsø (69.6°N, 19.2°E) in the Arctic. In general, u’w’ decreases and v’w’ increases as altitude increasing, and westward maximum of u’w’ and northward maximum of v’w’ in spring and autumn at upper altitude. the momentum flux u’w’ and v’w’ is anti-correlated with the background winds (u/v). The seasonal variations in the Davis Station meteor radar relative densities in the southern polar mesopause are mainly dominated by an annual oscillation (AO). The mesopause relative densities observed by the Tromsø meteor radars at high latitudes in the Northern Hemisphere show mainly an AO and a relatively weak semiannual oscillation (SAO).
 
Keywords
MLT,meteor radar,gravity wave
Speaker
易稳
副教授 中国科学技术大学

Submission Author
易稳 中国科学技术大学
薛向辉 中国科学技术大学
Submit Comment
Verify Code Change Another
All Comments
Important Date
  • Conference Date

    May 17

    2024

    to

    May 20

    2024

  • Mar 31 2024

    Draft paper submission deadline

  • Mar 31 2024

    Contribution Submission Deadline

  • May 20 2024

    Registration deadline

Sponsored By
青年地学论坛理事会
Organized By
厦门大学近海海洋环境科学国家重点实验室
中国科学院城市环境研究所
自然资源部第三海洋研究所
Contact Information
Previous Conferences