Investigation of dominant traveling 10-day wave components using long-term MERRA-2 database

Earth, Planets and Space

Wei Li¹  Shaodong Zhang²  Yun Gong²  Kaiming Huang²  Chunming Huang²  Gang Chen² 

[1] School of Electronic Information, Wuhan University, Wuhan, Hubei, China;School of Electronic Information, Wuhan University, Wuhan, Hubei, China;Key Laboratory of Geospace Environment and Geodesy, Ministry of Education, Wuhan, Hubei, China;

关键词: 10-day waves;    Travelling planetary wave;    Middle atmosphere;   

DOI  :  10.1186/s40623-021-01410-7

来源: Springer

【 摘 要 】

The eastward- and westward-traveling 10-day waves with zonal wavenumbers up to 6 from surface to the middle mesosphere during the recent 12 years from 2007 to 2018 are deduced from MERRA-2 data. On the basis of climatology study, the westward-propagating wave with zonal wave number 1 (W1) and eastward-propagating waves with zonal wave numbers 1 (E1) and 2 (E2) are identified as the dominant traveling ones. They are all active at mid- and high-latitudes above the troposphere and display notable month-to-month variations. The W1 and E2 waves are strong in the NH from December to March and in the SH from June to October, respectively, while the E1 wave is active in the SH from August to October and also in the NH from December to February. Further case study on E1 and E2 waves shows that their latitude–altitude structures are dependent on the transmission condition of the background atmosphere. The presence of these two waves in the stratosphere and mesosphere might have originated from the downward-propagating wave excited in the mesosphere by the mean flow instability, the upward-propagating wave from the troposphere, and/or in situ excited wave in the stratosphere. The two eastward waves can exert strong zonal forcing on the mean flow in the stratosphere and mesosphere in specific periods. Compared with E2 wave, the dramatic forcing from the E1 waves is located in the poleward regions.

【 授权许可】

CC BY