[特邀报告]Long‐Term Trends of the Meteor Altitude Distribution, Mesospheric density and Gravity Wave Momentum Flux Observed by the high-latitude meteor radars

Long‐Term Trends of the Meteor Altitude Distribution, Mesospheric density and Gravity Wave Momentum Flux Observed by the high-latitude meteor radars
编号:3211 稿件编号:1377 访问权限:仅限参会人 更新:2024-04-12 23:14:22 浏览:473次 特邀报告

报告开始:2024年05月18日 15:20 (Asia/Shanghai)

报告时间:10min

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摘要
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).
 
关键字
MLT,meteor radar,gravity wave
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易稳
副教授 中国科学技术大学

稿件作者
易稳 中国科学技术大学
薛向辉 中国科学技术大学
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