Evidence of high frequency gravity wave forcing on the meridional residual circulation at the mesopause region

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• 作者：Fabio Vargas^a ; ^{fvargas@illinois.edu" class="auth_mail" title="E-mail the corresponding author} ; Gary Swenson^a ; ¹ ; ^{swenson1@illinois.edu" class="auth_mail" title="E-mail the corresponding author} ; Alan Liu^b ; ² ; ^{alan.liu@erau.edu" class="auth_mail" title="E-mail the corresponding author}
• 关键词：Residual meridional circulation ; Gravity waves ; Wave drag ; Nightglow
• 刊名：Advances in Space Research
• 出版年：2015
• 出版时间：1 November 2015
• 年：2015
• 卷：56
• 期：9
• 页码：1844-1853
• 全文大小：3053 K

文摘

Data of high frequency gravity wave propagation direction from globally distributed stations indicate a meridional preference of mesospheric gravity waves to be globally oriented toward the summer pole. This orientation is opposite to the mean residual circulation (from summer to winter pole) at mesospheric altitudes. We discuss here a number of dynamic mechanisms including filtering that may be responsible for the preferential wave orientation, and the effects of the gravity wave forcing imposed on the meridional flow due to dissipative waves. Using nightglow image data recorded in three distinct latitude stations, we have estimated the meridional wave drag (i.e, deceleration) of about -4.6±0.2$-4.6\pm 0.2$ m/s/day during the summer, and 3.8±0.2$3.8\pm 0.2$ m/s/day during the winter, which is significant because the meridional flow has small magnitude. This is a component of dynamic forcing in the mesopause region, not heretofore recognized.